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Sample records for max planck institute

  1. Max-Planck-Institut fur Mathematik

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    . Auera a Max-Planck-Institut for Chemical Energy Conversion, Stiftstraße 34-36, D-45470 M¨ulheim a.d.R, Germany; b Max-Planck-Institute for Mathematics in the Sciences, Inselstraße 22, D-04103 Leipzig, Germany-MO integral transformation, the calculation of the MP2 energy and the potential usage of tensors in low rank

  2. Max-Planck-Institut fur Mathematik

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    Max-Planck-Institut f¨ur Mathematik in den Naturwissenschaften Leipzig Local Thermal Equilibrium;#12;Local Thermal Equilibrium States in Relativistic Quantum Field Theory Michael Gransee Abstract. It is well-known that thermal equilibrium states in quan- tum statistical mechanics and quantum field theory

  3. Max-Planck-Institut fur Mathematik

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    , Leipzig, Germany 4) Max Planck Institute for Mathematics in the Sciences, Leipzig, Germany 1 #12;We Helmholtz free energy of the solution as a function of radius of gyration and the cosolvent concentration within gyration volume. After minimization of the total Helmholtz free energy with respect to its

  4. Max-Planck-Institut f ur Mathematik

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    by the equations: (1.1) (# t +D)u = 0, u(x; 0) = #, and Bu = 0. The specific heat # is a section to the dual bundle V # . Let #(#, #, D, B)(t) := # M u# be the total heat energy content. As t # 0, there is a completeMax-Planck-Institut fË? ur Mathematik in den Naturwissenschaften Leipzig Heat content asymptotics

  5. Max-Planck-Institut fr biologische Kybernetik Max Planck Institute for Biological Cybernetics

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    and analysis of human psychophysical experiments. · Good understanding of the English language in speaking Position in Human Motion Simulation The Max Planck Institute for Biological Cybernetics in Tübingen laws of perception will be implemented into the control framework of motion-based simulators. Human

  6. Max-Planck-Institut fur Mathematik

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    , topology and information geometry. This research is motivated by a theory of info- max principles, where we operationally by coding theorems: These entropies quantify the amount of physical resources needed probability. Optimal tests are known in state tomog- raphy with respect to natural measures of efficiency [WF

  7. MAX-PLANCK-INSTITUT A Recursion Planning Analysis of

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    Waldmann, Uwe

    Richard Barnett David Basin Jane Hesketh MPI­I­92­230 July 1992 k I N F O R M A T I K Im Stadtwald W 6600 Saarbr¨ucken Germany #12;Authors' Addresses Richard Barnett ICL Cavendish Road, Stevenage, Herts SG1 3DS, UK R.D.Barnett@ste0404.wins.icl.co.uk David Basin, Max-Planck-Institut f¨ur Informatik Im

  8. Jung-Jin Lee PhD Candidate, Max Planck Institute for Biological Cybernetics

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    Jung-Jin Lee PhD Candidate, Max Planck Institute for Biological Cybernetics I have been trained, and Action at Max Planck Institute for Biological Cybernetics, I conduct research on human factors and Behavioral Sciences! ! ! ! ! ! ! 2011 - present Korea University, Seoul, South Korea Master of Engineering

  9. 07. September 2007 Julia Ducke 1 Max-Planck-Institut fr

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    07. September 2007 Julia Ducke 1 Max-Planck-Institut für Mikrostrukturphysik HalleWeb 2.0-Workshop Wiki Erfahrungen mit Web 2.0 Erfahrungsbericht aus der Bibliothek des MPI für Mikrostrukturphysik #12;07. September 2007 Julia Ducke 2 Max-Planck-Institut für Mikrostrukturphysik HalleWeb 2.0-Workshop #12

  10. Dr. Anke Henning -Curriculum vitae Business: Max Planck Institute for Biological Cybernetics

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    Dr. Anke Henning - Curriculum vitae Business: Max Planck Institute for Biological Cybernetics MRZ Department Spemannstrasse 41 72076 Tübingen Germany Tel : +49 7071 601 723 anke.henning thesis: Prof. H.J. Hinneberg Structural investigations of CrSi2-films by TEM. 09.1999 - 05.2000 Exchange

  11. INTEGRAL EQUATIONS FOR KINEMATIC DYNAMO MODELS Max-Planck-Institut fur Aeronomie, Katlenburg-Lindau, Germany1

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    Dobler, Wolfgang

    INTEGRAL EQUATIONS FOR KINEMATIC DYNAMO MODELS W. Dobler Max-Planck-Institut f¨ur Aeronomie of the induction equation and boundary conditions at infinity into an integral equation. We show that the integral of integration by parts and shows that an arbitrary gradient can be added to or subtracted from j(x) 1 Address

  12. [10] K. Mehlhorn and C. Uhrig. The Minimum Cut Algorithm of Stoer and Wagner. Unpublished manuscript, Max Planck Institute for Computer Science. Available at

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    Fegaras, Leonidas

    [10] K. Mehlhorn and C. Uhrig. The Minimum Cut Algorithm of Stoer and Wagner. Unpublished manuscript, Max Planck Institute for Computer Science. Available at http://www.mpi­sb.mpg.de/guide/staff/uhrig, pp 238--248, May 1997. [15] P. Selinger, M. Astrahan, D. Chamberlin, R. Lorie, and T. Price. Access

  13. Technologietransfer fr die Max-Planck-Gesellschaft

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    markets inventions in the fields of biology and medicine as well as in chemistry, physics and technology and creates new jobs in Ger- many as a business location. Every year, Max Planck Innovation evaluates 140. These spin-offs have since resulted in the creation of over 2,650 jobs. Die Max-Planck-Innovation GmbH ist

  14. Princeton, Max Planck Society launch new research center for...

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    of the Federal Republic of Germany in New York Busso von Alvensleben meet to sign an agreement launching the new Max Planck Princeton Research Center for Plasma Physics....

  15. 2/2007 B56133 MaxPlanckResearchSCIENCE MAGAZINE OF THE MAX PLANCK SOCIETY

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    ;2 / 2 0 0 7 M A X P L A N C K R E S E A R C H 3 A shared duty ­ Politics is never sim- ple there: the Institutes for Astronomy, Nuclear Physics, Medical Research and Comparative Public an abbreviated version of the chapter on "Politics in an Aging Society" in this issue (page 54 ff.), which deals

  16. Max-Planck-Institut f ur Mathematik

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    prove a non­commutative Varadhan Lemma for quantum spin systems with Bose­Einstein statistics and mean systems of random processes with symmetrised initial­ terminal conditions; Feynman­Kac formula; Bose­Einstein

  17. Max-Planck-Institut f ur Mathematik

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    ­wave pulses in Bose­Einstein condensates, see e.g. [19, 23]. Notice that the KP equation has originally been

  18. Max-Planck-Institut f ur Mathematik

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    transition, the so­called Bose­Einstein condensation: a macroscopic portion of the system is described by one already in 1925 by Bose and Einstein. A rigorous understanding of condensation e#ects in various ultra an enormous impetus by the first experimental realisation of Bose­Einstein condensation in 1995. A many

  19. Max-Planck-Institut f ur Mathematik

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    of the infinite system. 1 Introduction The phenomenon known as Bose­Einstein condensation (hereafter abbreviated BEC) was predicted by Einstein (1925) on the basis of ideas of the Indian physi­ cist Bose (1924 on the concept of Bose­Einstein condensation. This initiated several the­ oretical studies; a recent account

  20. Max-Planck-Institut f ur Mathematik

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    as a model for Bose­Einstein con­ densation, motivated by the success of the famous 1995 experiments temperature, they undergo a phase transition, the so called Bose­Einstein condensation. This formally means that a macroscopic portion, the condensate, is described by one single­particle wave function. Bose­Einstein

  1. Max-Planck-Institut fur Mathematik

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    computational packages, we perform a symmetry classification of destabilizing bifurcations in bidirectional is the equivariant degree and the "Equivariant Degree Maple c Library Package" that performs exact computations is completely taken over by the "Equivariant Degree Maple c Library Package". This equivariant degree approach

  2. Max-Planck-Institut fur Mathematik

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    of these coordinates. Keywords Many Body interactions · Kac-type potentials for crystal plasticity · Lattice free for reference-free plasticity by Stephan Luckhaus and Jens Wohlgemuth Preprint no.: 111 2013 #12;#12;Noname manuscript No. (will be inserted by the editor) Study of a model for reference-free plasticity Stephan

  3. Max-Planck-Institut fur Mathematik

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    at the price of an additional surface energy. We study analytically a two-dimensional variational model domains. We first derive the scaling regimes of the minimal energy in terms of the volume of the film opposing types of energies, namely, the stored strain energy due to the crystallographic misfit

  4. Max-Planck-Institut fur Mathematik

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    -assembly in dif- ferent physico-chemical systems like micelle formation, proteins folding, macro- and microphase solutes [10, 12] like methane [11] and short hydrophobic chain molecules [6, 8] were considered. In 2002, based on the results of their computer simulations, that this effect is reminiscent of a first

  5. Max-Planck-Institut fur Mathematik

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    , in terms of the Rayleigh number Ra, that characterizes the relative strength of the driving mechanism appearing are the kinematic viscosi

  6. Max-Planck-Institut fur Mathematik

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    computational tasks. PACS numbers: 89.75.Hc, 05.45.-a, 05.65.+b, 89.75.-k In 1948, Alan Turing proposed several

  7. Max-Planck-Institut fur Mathematik

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    ]. In these applications the efficient calculation of quantities like potential energy function or interparticle forces introduce and study the grid-based rank-structured tensor method for fast and accurate calculation cells in a box the numerical cost scales linearly in the grid-size, n as O(NL). For periodic boundary

  8. Max-Planck-Institut fur Mathematik

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    anisotropy of the cosmic background radiation map (CMB) obtained by space missions, the investigation

  9. Max-Planck-Institut f ur Mathematik

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    ­qubit and three­qubit Schmidt­Correlated states by Ming­Jing Zhao, Zong­Guo Li, Bo Li, Shao­Ming Fei, Zhi­Xi Wang­Correlated states Ming­Jing Zhao 1 , Zong­Guo Li 2 , Bo Li 1 , Shao­Ming Fei 1,3 , Zhi­Xi Wang 1 , and Xian­Qing Li

  10. Max-Planck-Institut f ur Mathematik

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    with Arbitrary Pure or Mixed States by Ming­Jing Zhao, Zong­Guo Li, Shao­Ming Fei, Zhi­Xi Wang, and Xianqing Li , Zong­Guo Li 2 , Shao­Ming Fei 1,3 , Zhi­Xi Wang 1 , and Xianqing Li­Jost 3 1 School of Mathematical

  11. Max-Planck-Institut f ur Mathematik

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    tensor space, by means a tensor given in a typical representation format (Tucker, hierarchical or tensor. Examples by using topological tensor products of standard Sobolev spaces are given. 2010 AMS Subject, the aim is to compress the best as possible the information or to extract a few modes representing some

  12. Research Report 2008 Max Planck Institute

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    -37073 Göttingen ­ www.ds.mpg.de Editing: Dr. Kerstin Mölter Photos: Prof. Dr. Markus Engstler, Dr Emergent Geographical Community Structures: Universalities and National Differences Criticality

  13. Max-Planck-Institut fur Mathematik

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    , we consider the N - 1 dimensional hyper-plane XN,m given by XN,m := x RN , 1 N N i=1 xi = m . We-1 XN,m denotes the N - 1 dimensional Hausdorff measure restricted to the hy- perplane XN

  14. MaxPlanckInstitut f ur Mathematik

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    =1 #(x i ). (1) For a real number m, we consider the N - 1 dimensional hyper­plane XN,m given by XNN,m (dx) := 1 Z exp (-H(x)) H N-1 #XN,m (dx). (2) Here, H N-1 #XN,m denotes the N - 1 dimensional

  15. Max-Planck-Institut fur Mathematik

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    approximation method to the problems of electronic structure calculations were developed in [11, 12, 10 Key words: Tensor-structured methods, fast wavelet transform, multilevel methods, canon- ical tensor]. Applications to high-dimensional dynamics including chemical master equation were described in [5, 3]. The QTT

  16. Max-Planck-Institut fur Mathematik

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    , if A is the subsemigroup generated by elements of Hilb(B) that lie on the extremal rays of B, and K[B] = gIg i

  17. Max-Planck-Institut fur Mathematik

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    , and the connections among the funds being determined by the cross-correlation coeffi- cients, using a winner-take a stock network to investigate the interactions among the stocks. Schweitzer and Stanley [27

  18. Max-Planck-Institut fur Mathematik

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    × n fully pop- ulated matrix. The required storage and execution time for the corresponding standard with the state-of-the-art iterative solvers which also can be found in highly efficient parallel versions

  19. Max-Planck-Institut fur Mathematik

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    American Power Grid Network (NAPGN). Our work may shed light on interpreting the exponential degree American Power Grid Network (NAPGN) [18], etc. This new class of networks give birth to several questions

  20. Max-Planck-Institut f ur Mathematik

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    , Cambridge, CB3 OWA e­mail: D.M.A.Stuart@damtp.cam.ac.uk Abstract The long­time asymptotics is analyzed for finite energy solutions of the 1D SchrË?odinger equation coupled to a nonlinear oscillator. The coupled to the free SchrË?odinger equation. The proofs use the strategy of Buslaev­Perelman [3, 4]: the linerization

  1. Max-Planck-Institut fur Mathematik

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    ]. In this brief report we present an experimental de- termination of the entanglement of formation for arbi- trary j=1 aija ij = 1 . (2) The entanglement of formation of | is defined as the partial entropy

  2. MaxPlanckInstitut f ur Mathematik

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    present an experimental de­ termination of the entanglement of formation for arbi­ trary dimensional pure a # ij = 1 . (2) The entanglement of formation of |## is defined as the partial entropy with respect

  3. Max-Planck-Institut fur Mathematik

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    methods to measure the entanglement of formation, and the lower bound of the convex-roof extension the entanglement of mixed states: the channel capacity and the distillable entanglement. The convex-roof extension fundamental tests of quantum mechanics [38], and more efficient quantum gates [39]. In particular, hybrid

  4. Max-Planck-Institut fur Mathematik

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    (pseudotrajectories) of dynamical sys- tems is now a well-developed part of the global theory of dynamical systems Laboratory, Saint-Petersburg State Univeristy, 14th Line 29B, Vasilyevsky Island, St.Petersburg 199178 give an upper bound for the length of shadowable pseudotrajectories for non-hyperbolic systems

  5. Max-Planck-Institut fur Mathematik

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    developed part of the global theory of dynamical systems (see, for example, the monographs [7,9]). Often] and structurally stable systems (satisfying Axioma A and the strong transversality condition) have shadowing-Petersburg State Univeristy, 14th line of Vasilievsky island, 29B, Saint-Petersburg, 199178, Russia; sergey

  6. MAX-PLANCK-INSTITUT Workshop on

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    Waldmann, Uwe

    and Related Methods Marseille, France, April 28-30, 1993 David Basin, Reiner Ha.b.nle, Bertram Fronhofer for Tableaux S. Briining: Search Space Pruning by Checking Dynamic Term Growth M. Buchheit, F. M. Donini, A. Mondadori: The Complexity of Proof-Search with Analytic Tableaux and Related Sys- tems M. D'Agostino, D

  7. Max-Planck-Institut fur Mathematik

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    of Classical and Quantum Loop Diagrams 31 4.4. The Zero-Point Energy of the Stochastic Field 33 5. Outlook 34 suitable energy differences. By adding a classical stochastic background field, we even ob- tain all loop Expansion 18 3.5. A Perturbation Expansion of the Classical Energy 20 3.6. The Classical Scattering Operator

  8. Max-Planck-Institut fur Mathematik

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    for Mathematics in the Sciences, Leipzig, Germany bEge University, Izmir, Turkey Abstract We consider

  9. Max-Planck-Institut fur Mathematik

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    . Leipzig, Germany. 1 #12;The energy we study, defined on partitions of D, is: E(1, . . . , N ) = N i,j=1 i gradient descent for an energy in which the area of each surface in the network is weighted by a possibly, robust algorithms for simulating the L2 gradient flow of energy (2). Two important rules defining

  10. MAX-PLANCK-INSTITUT Preprints of

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    Waldmann, Uwe

    for Classification Problem Solving Karsten Poeck and Martin Tins Knowledge-based Processing ofMedical Language

  11. Max-Planck-Institut fur Mathematik

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    and deliberatively choosing among them is an important ability, not only in humans and animals, but also such as coordination. This is studied in a virtual robotics scenario. 1 Introduction Evaluating different possibilities

  12. MAX-PLANCK-INSTITUT Finding k points with a smallest

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    ;set Au (B +p), where B +p := {b +p : bEB}. We also want to insert and delete elements in A and B--element in the set Au (B +p), where B +p := {b +p : bEB}. Moreover, it should be possible to insert and delete

  13. Max Planck Institute for Molecular Genetics, October 21st, 2002

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    Spang, Rainer

    EyeConjunctivitis Itching, rashSkinDermatitis Coughing, wheezing, shortness of breath LungsAsthma Sneezing, rhinorrhea

  14. MaxPlanckInstitut fur Physik Munich, Germany

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    of the neutrino and its absolute mass-scale by searching for the neutrinoless double­beta decay of 76Ge. The goal

  15. MAX-PLANCK-INSTITUT.. ( Lower Bounds for Set Intersection

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    . Mehlhorn R. Raman C. Uhrig MPI- I-92-127 October 1992 o mPD_ _ _ _ _ _ _ IN F 0 R M AT I K _ _ _ _ __ Im Stadtwald 66123 Saarbrücken Germany #12;Lower Bounds for Set Intersection Queries P. Dietz K. Mehlhorn R. Raman C. Uhrig MPI-I-92-127 October 1992 #12;Lower Bounds for Set Intersection Queries PAUL DIETZ KURT

  16. Paul Blom: Research Director, Max Planck Institute for Polymer Research |

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeeding access| Department ofStephenSkinner,PastPatent80Paul Adams Print

  17. Bernstein Center for Computational Neuroscience (BCCN) Gttingen Georg-August-Universitt Gttingen, Max-Planck-Institut fr Dynamik und Selbstorganisation, Max-Planck-Institut fr biophysikalische Chemie, Max-Planck-Institut fr experimentelle Medizin,

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    Gollisch, Tim

    die Sehrinde tausendfach wiederholt, bezeichnen Forscher als Pinwheel (deutsch: Windrad), denn Gebiete derselben Orientierungspräferenz treffen an einem Punkt zusammen ­ wie die Flügel eines Spielzeug-Windrades

  18. American Institute of Aeronautics and Astronautics Does jerk have to be considered in linear motion simulation?

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    American Institute of Aeronautics and Astronautics 1 Does jerk have to be considered in linear by Max Planck Institute for Biological Cybernetics. Published by the American Institute of Aeronautics

  19. Nanomaterials Theory Institute Center for Nanophase Materials Sciences

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    Pennycook, Steve

    Organizer, CECAM Symposium at Psi-k 2010 on Organic Electronics for Energy Research, Berlin, Germany, 2010 Haber Institute of the Max Planck Society, Berlin, Germany 2005­2009 Research Assistant Professor of the Max Planck Society, Germany, 2008-1011 Organization Committee, Conference on Computational Physics

  20. Physik Department -Technische Universitat Munchen Max-Planck-Institut fur Physik

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    sensitive astronomy light sensors in the far-infrared region of the spectrum, and could be used in future the first attempt towards quantitative, automated, and functional evaluation of blood-borne cellular-area, automated quantitation of captured cells and rapid evaluation of functional cellular parameters (e.g. size

  1. 21st IAEA Fusion Energy Conference, Chengdu, 16 21 October 2006 1 Max-Planck-Institut

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    and Fabrication Experienced Gained during Design, Fabrication and Testing of Components Assembly of the W7-X as well as for the assembly. For diagnostics, cooling, plasma heating and other purposes adequate port 20 planar coils 2 types Cold mass ~ 400 tonnes Plasma vessel Central support ring W7-X is a fully

  2. Rainer Held > Guest Researcher - Max-Planck Institute for Solid State

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-RichProton DeliveryRadioactive Materials

  3. Curriculum Vitae Arne Max Erich Winguth, Ph.D.

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    Winguth, Arne

    in an earth system model", two months summer salary, 2005. [9] Visiting Scientist, Max Planck Institute for Meteorology, Germany, "Development of marine carbon cycle in an earth system model", two months summer salary of marine carbon cycle in an earth system model", two months summer salary, 2003. [12] University

  4. Makromolekulare Chemie SS 04: Ulrich Jonas, Max-Planck-Institut fr Polymerforschung, Ackermannweg 10, 55128 Mainz, Tel.

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    Jonas, Ulrich - Institute of Electronic Structure and Laser, Foundation for Research and Technology

    coating: reduces adhesion of adhesive layer and allows release of rolled up tapes etc. (silicones, alkyds Example: Adhesive Tape adhesive layer primer backing release coating tack: in adhesives tack describes

  5. Name e-mail position Institution 1 Arndt, Max m.arndt@ged.rwth-aachen.de PhD RWTH-Aachen University, Geologie Endogene Dynamik, Aachen, Germany

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    Cesare, Bernardo

    Name e-mail position Institution 1 Arndt, Max m.arndt@ged.rwth-aachen.de PhD RWTH-Aachen University, Geologie Endogene Dynamik, Aachen, Germany 2 Billia, Marco marco.billia@alumni.ethz.ch PhD Department of Geology, University of Otago, New Zealand 3 Boutonnet, Emmanuelle emmanuelle.boutonnet@ens-lyon.fr PhD

  6. One Hundred Years of the Fritz Haber Institute Bretislav Friedrich,* Dieter Hoffmann, and Jeremiah James

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    Friedrich, Bretislav

    ), is not only one of the oldest and most tradition-rich institutes of the Max Planck Society (MPG), but also one of the most distinguished, with the highest number of affiliated Nobel laureates of any KWG/ MPG institute its walls over the past century, but so too do the diverse abilities and personalities

  7. Fokker-Planck equation for the energy cascade in turbulence Research Institute for Electrical Communication, Tohoku University, 2-1-1 Katahira, Aoba-ku, Sendai 980-77, Japan

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    Peinke, Joachim

    Fokker-Planck equation for the energy cascade in turbulence A. Naert Research Institute for Electrical Communication, Tohoku University, 2-1-1 Katahira, Aoba-ku, Sendai 980-77, Japan R. Friedrich; revised manuscript received 5 August 1997 We present a detailed analysis of the energy dissipation

  8. Driven Drops on Heterogeneous Substrates: Onset of Sliding Motion Max-Planck-Institut fur Physik komplexer Systeme, Nothnitzer Strasse 38, D-01187 Dresden, Germany

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    Knobloch, Edgar

    and are responsible, for instance, for the observed hysteresis between advancing and receding contact angles, as well November 2006) Pinning and depinning of driven drops on heterogeneous substrates is studied as a function energy [1,2]. Likewise, a drop in a temperature gradient moves towards lower temperatures as a result

  9. 32 Jahresbericht Max-Planck-Gesellschaft 2014 Annual Report Max Planck Society 2014

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    Falge, Eva

    are a possible solution, and automotive companies like Honda and Toyota have invested billions in a potential new industrial sector. Today, some 15 years down the line, the challenge of "age- ing societies" has not changed industrial robots. Toy ro- bots, robots that can provide emotional support and miniature robots able to carry

  10. Earth Syst. Dynam., 4, 187198, 2013 www.earth-syst-dynam.net/4/187/2013/

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    Zuyev, Sergei

    Planck Research School for Earth System Modelling, Hamburg, Germany 2Max Planck Institute for Meteorology

  11. Planck 2010

    ScienceCinema (OSTI)

    None

    2011-10-06

    Planck 2010 From the Planck Scale to the ElectroWeak Scale The conference will be the twelfth one in a series of meetings on physics beyond the Standard Model, organized jointly by several European groups: Bonn, CERN, Ecole Polytechnique, ICTP, Madrid, Oxford, Padua, Pisa, SISSA and Warsaw as part of activities in the framework of the European network UNILHC.Topics to be discussed: Supersymmetry Supergravity & string phenomenology Extra dimensions Electroweak symmetry breaking LHC and Tevatron Physics Collider physics Flavor & neutrinos physics Astroparticle & cosmology Gravity & holography Strongly coupled physics & CFT Registration: registration will be open until May 1st. Registration fees amount to 150 CHF and cover the cost of the coffee breaks and the social dinner. Payment has to be made online. The deadline for registration has been postponed to May 7th. However, after May 3th, we shall not accept any talk request any more. The meeting will be partly supported by ° the Marie Curie Initial Training Network "UNILHC" PITN-GA-2009-23792, ° the ERC Advanced Grant "MassTeV" 226371, ° and the CERN-TH unit.

  12. Matrix Groups Max Neunhffer

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    St Andrews, University of

    Matrix Groups Max Neunhöffer Introduction GAP examples Matrix groups in GAP Schreier-Sims Problems Group algebras SLPs Constructive recognition The problem Troubles Matrix Groups Max Neunhöffer University of St Andrews GAC 2010, Allahabad #12;Matrix Groups Max Neunhöffer Introduction GAP examples

  13. Populations Voss, R.; /Garching, Max Planck Inst., MPE; Ajello...

    Office of Scientific and Technical Information (OSTI)

    study the populations of X-ray sources in the Milky Way in the 15-55 keV band using a deep survey with the BAT instrument aboard the Swift observatory. We present the logN-logS...

  14. 6 MaxPlanckForschung 3 | 09 PERSPEKTIVEN

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    Falge, Eva

    der Karibikinsel Barbados eine zweijährige em- pirische Feldstudie. Die Wissenschaftler konzentrieren HALO. Auf Barbados sind die Bedingungen für die Messungen ideal. Die Insel liegt in der Karibik relativ Barbados gibt es je nach Jahreszeit unterschiedlichste Strömungsmuster oder Wolkenformatio- nen. Im Winter

  15. Max Planck Society for the Advancement of Science

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    the electrical activity in the brain by means of electrodes on the head is a handy tool to study brain function as it is noninvasive and easy to apply. The interpretation of the EEG signal remains, however, difficult. The main this very question for the first time. By combining recordings of both EEG and individual neurons in trained

  16. VOLUME 80, NUMBER 20 P H Y S I C A L R E V I E W L E T T E R S 18 MAY 1998 Long-Range Time Correlations in Plasma Edge Turbulence

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    van Milligen, Boudewijn

    Euratom-Ciemat, 28040 Madrid, Spain 3 Max-Planck-Institut für Plasmaphysik, Euratom Association, 85740

  17. Confinement Study of Net-Current Free Toroidal Plasmas Based on

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    , Australia 3) Max-Planck-Institut für Plasmaphysik, EURATOM Association, Germany 4) CIEMAT, Spain 5

  18. Ocean Carbon Cycle Models from the Carbon Dioxide Information Analysis Center (CDIAC)

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    •\tPacific data-model intercomparison from Patrick Wetzel (Max Planck Institute for Meteorology, Germany)

  19. CATMA: a complete Arabidopsis GST database Mark L. Crowe1,2,*, Carine Serizet1,2

    E-Print Network [OSTI]

    Gent, Universiteit

    de Biotecnologia, Campus de Cantoblanco, 28049-Madrid, Spain and 9 Max-Planck-Institute for Molecular

  20. CMB Anomalies after Planck

    E-Print Network [OSTI]

    Schwarz, Dominik J; Huterer, Dragan; Starkman, Glenn D

    2015-01-01

    Several unexpected features have been observed in the microwave sky at large angular scales, both by WMAP an by Planck. Among those features is a lack of both variance and correlation on the largest angular scales, alignment of the lowest multipole moments with one another and with the motion and geometry of the Solar System, a hemispherical power asymmetry or dipolar power modulation, a preference for odd parity modes and an unexpectedly large cold spot in the Southern hemisphere. The individual p-values of the significance of these features are in the per mille to per cent level, when compared to the expectations of the best-fit inflationary $\\Lambda$CDM model. Some pairs of those features are demonstrably uncorrelated, increasing their combined statistical significance and indicating a significant detection of CMB features at angular scales larger than a few degrees on top of the standard model. Despite numerous detailed investigations, we still lack a clear understanding of these large-scale features, whi...

  1. Proton Decay and the Planck Scale

    E-Print Network [OSTI]

    Larson, Daniel T.

    2009-01-01

    LBNL- 56556 PROTON DECAY AND THE PLANCK SCALE DANIEL T.ph/0410035v1 2 Oct 2004 PROTON DECAY AND THE PLANCK SCALE ?without grand uni?cation, proton decay can be a powerful

  2. Primordial power spectrum from Planck

    E-Print Network [OSTI]

    Dhiraj Kumar Hazra; Arman Shafieloo; Tarun Souradeep

    2014-12-18

    Using modified Richardson-Lucy algorithm we reconstruct the primordial power spectrum (PPS) from Planck Cosmic Microwave Background (CMB) temperature anisotropy data. In our analysis we use different combinations of angular power spectra from Planck to reconstruct the shape of the primordial power spectrum and locate possible features. Performing an extensive error analysis we found the dip near $\\ell\\sim750-850$ represents the most prominent feature in the data. Feature near $\\ell\\sim1800-2000$ is detectable with high confidence only in 217 GHz spectrum and is apparently consequence of a small systematic as described in the revised Planck 2013 papers. Fixing the background cosmological parameters and the foreground nuisance parameters to their best fit baseline values, we report that the best fit power law primordial power spectrum is consistent with the reconstructed form of the PPS at 2$\\sigma$ C.L. of the estimated errors (apart from the local features mentioned above). As a consistency test, we found the reconstructed primordial power spectrum from Planck temperature data can also substantially improve the fit to WMAP-9 angular power spectrum data (with respect to power-law form of the PPS) allowing an overall amplitude shift of $\\sim2.5\\%$. In this context low-$\\ell$ and 100 GHz spectrum from Planck which have proper overlap in the multipole range with WMAP data found to be completely consistent with WMAP-9 (allowing amplitude shift). As another important result of our analysis we do report the evidence of gravitational lensing through the reconstruction analysis. Finally we present two smooth form of the PPS containing only the important features. These smooth forms of PPS can provide significant improvements in fitting the data (with respect to the power law PPS) and can be helpful to give hints for inflationary model building.

  3. Primordial power spectrum from Planck

    SciTech Connect (OSTI)

    Hazra, Dhiraj Kumar; Shafieloo, Arman; Souradeep, Tarun E-mail: arman@apctp.org

    2014-11-01

    Using modified Richardson-Lucy algorithm we reconstruct the primordial power spectrum (PPS) from Planck Cosmic Microwave Background (CMB) temperature anisotropy data. In our analysis we use different combinations of angular power spectra from Planck to reconstruct the shape of the primordial power spectrum and locate possible features. Performing an extensive error analysis we found the dip near ? ? 750–850 represents the most prominent feature in the data. Feature near ? ? 1800–2000 is detectable with high confidence only in 217 GHz spectrum and is apparently consequence of a small systematic as described in the revised Planck 2013 papers. Fixing the background cosmological parameters and the foreground nuisance parameters to their best fit baseline values, we report that the best fit power law primordial power spectrum is consistent with the reconstructed form of the PPS at 2? C.L. of the estimated errors (apart from the local features mentioned above). As a consistency test, we found the reconstructed primordial power spectrum from Planck temperature data can also substantially improve the fit to WMAP-9 angular power spectrum data (with respect to power-law form of the PPS) allowing an overall amplitude shift of ? 2.5%. In this context low-? and 100 GHz spectrum from Planck which have proper overlap in the multipole range with WMAP data found to be completely consistent with WMAP-9 (allowing amplitude shift). As another important result of our analysis we do report the evidence of gravitational lensing through the reconstruction analysis. Finally we present two smooth form of the PPS containing only the important features. These smooth forms of PPS can provide significant improvements in fitting the data (with respect to the power law PPS) and can be helpful to give hints for inflationary model building.

  4. Velocity-Dependent Dynamic Curvature Gain for Redirected Walking Christian T. Neth

    E-Print Network [OSTI]

    and Cognitive Engineering, Korea University Betty J. Mohler Max Planck Institute for Biological Cybernetics 8 m Institute for Biological Cybernetics; Reutlingen University Jan L. Souman Max Planck Institute for Biological Cybernetics David Engel Max Planck Institute for Biological Cybernetics Uwe Kloos Reutlingen

  5. Planck Surveyor On Its Way to Orbit

    ScienceCinema (OSTI)

    None

    2010-01-08

    An Ariane 5 rocket carried the Planck Surveyor and a companion satellite into space May 14, 2009 from the European Space Agency (ESA) base on the northwest coast of South America. Once in orbit beyond the moon, Planck will produce the most accurate measurements ever made of the relic radiation from the big bang, plus the largest set of CMB data ever recorded. Berkeley Labs long and continuing involvement with Planck began when George Smoot of the Physics Division proposed Plancks progenitor to ESA and continues with preparations for ongoing data analysis for the U.S. Planck team at NERSC, led by Julian Borrill, co-leader of the Computational Cosmology Center

  6. Planck Surveyor On Its Way to Orbit

    ScienceCinema (OSTI)

    Borrill, Julian

    2013-05-29

    An Ariane 5 rocket carried the Planck Surveyor and a companion satellite into space May 14, 2009 from the European Space Agency (ESA) base on the northwest coast of South America. Once in orbit beyond the moon, Planck will produce the most accurate measurements ever made of the relic radiation from the big bang, plus the largest set of CMB data ever recorded. Berkeley Labs long and continuing involvement with Planck began when George Smoot of the Physics Division proposed Plancks progenitor to ESA and continues with preparations for ongoing data analysis for the U.S. Planck team at NERSC, led by Julian Borrill, co-leader of the Computational Cosmology Center.

  7. Atmos. Chem. Phys., 15, 1043510452, 2015 www.atmos-chem-phys.net/15/10435/2015/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    , Tampere University of Technology, P.O. Box 692, 33101 Tampere, Finland 5Max-Planck-Institut für Kernphysik

  8. Structure-property maps and optimal inversion in configurational thermodynamics Bjrn Arnold,1,* Alejandro Daz Ortiz,1, Gus L. W. Hart,2 and Helmut Dosch3

    E-Print Network [OSTI]

    Hart, Gus

    ,* Alejandro Díaz Ortiz,1, Gus L. W. Hart,2 and Helmut Dosch3 1Max Planck Institute for Metals Research

  9. Classically Semisimple Locally Finite Lie Superalgebras

    E-Print Network [OSTI]

    Penkov, Ivan

    . According to Work supported in part by an NSF GIG Grant, by the Max-Planck-Institute for Mathematics, Bonn

  10. Making CARS better Max Zimmerleya

    E-Print Network [OSTI]

    Potma, Eric Olaf

    Making CARS better Max Zimmerleya , Hyun Min Kima , Desiré Whitmorea , Vishnu Vardhan is presented of recent trends in coherent anti-Stokes Raman scattering (CARS) microscopy. We briefly discuss the influence of tissue scattering on the CARS signal, methods for controlling the CARS emission and prospects

  11. Cloud Security by Max Garvey

    E-Print Network [OSTI]

    Tolmach, Andrew

    Cloud Security Survey by Max Garvey #12;Cloudy Cloud is Cloudy What is the cloud? On Demand Service, performance SECaaS - Cloud hosted security measures Certifications - measurements for cloud security. #12;Cloud Questions If you have $0 security budget, could cloud be a security improvement? Who owns the data

  12. Yago: A Large Ontology from Wikipedia and WordNet

    E-Print Network [OSTI]

    Waldmann, Uwe

    Weikum MPI­I­2007­5-003 December 2007 #12;#12;Authors' Addresses Fabian M. Suchanek Max-Planck-Institute for Computer Science Campus E1 4 66123 Saarbr¨ucken Germany Gjergji Kasneci Max-Planck-Institute for Computer Science Campus E1 4 66123 Saarbr¨ucken Germany Gerhard Weikum Max-Planck-Institute for Computer Science

  13. Animations of Medical Training Scenarios in Immersive Virtual Environments

    E-Print Network [OSTI]

    Cybernetics Dept. of Brain and Cognitive Engineering, Korea University Betty J. Mohler Max Planck Institute Max Planck Institute for Biological Cybernetics ivelina.alexandrova@tuebingen.mpg.de Marcus Rall Tu of T¨ubingen Medical School Martin Breidt Max Planck Institute for Biological Cybernetics Uwe Kloos

  14. PREPARED FOR THE U.S. DEPARTMENT OF ENERGY, UNDER CONTRACT DE-AC02-76CH03073

    E-Print Network [OSTI]

    PREPARED FOR THE U.S. DEPARTMENT OF ENERGY, UNDER CONTRACT DE-AC02-76CH03073 PRINCETON PLASMA (Princeton, NJ USA) and the Max-Planck-Institut für Plasmaphysik, (Garching, Germany)and the Max-Planck-Institut für Plasmaphysik, (Garching, Germany)and the Max-Planck-Institut für Plasmaphysik, (Garching, Germany

  15. Kähler potentials for Planck inflation

    SciTech Connect (OSTI)

    Roest, Diederik; Scalisi, Marco; Zavala, Ivonne E-mail: m.scalisi@rug.nl

    2013-11-01

    We assess which Kähler potentials in supergravity lead to viable single-field inflationary models that are consistent with Planck. We highlight the role of symmetries, such as shift, Heisenberg and supersymmetry, in these constructions. Also the connections to string theory are pointed out. Finally, we discuss a supergravity model for arbitrary inflationary potentials that is suitable for open string inflation and generalise it to the case of closed string inflation. Our model includes the recently discussed supergravity reformulation of the Starobinsky model of inflation as well as an interesting alternative with comparable predictions.

  16. PHYSICS & ASTRONOMY_Personal Portrait 46 MaxPlanckResearch 3 | 15

    E-Print Network [OSTI]

    Falge, Eva

    's developments in spintronics that first made Facebook and Google possible, as well as many other computer on a hard drive. Parkin is considered to be one of the pioneers of spintronics, not least due to what

  17. Foto:MPIfrWissenschaftsgeschichteSkliSigurdsson 86 MaxPlanckForschung 1 | 12

    E-Print Network [OSTI]

    Falge, Eva

    bis zur Ökonomie ­ revolutioniert hat, indem sie zwischen den beiden Polen ,,wahr" und ,,falsch" ein

  18. 70 MaxPlanckForschung 2 | 12 Im Erdsystem zirkulieren gigantische Energiemengen: Winde wie dieser Taifun

    E-Print Network [OSTI]

    Falge, Eva

    Lichts in Zucker und liefern so den Brennstoff des Lebens. Die Geothermie knetet die Erde durch, während

  19. Call for Application Max-Planck Hebrew University Junior Fellows Program in Brain Research

    E-Print Network [OSTI]

    a Junior Fellows Program. Each Junior Fellowship is a three-year position (renewable up to five years and their integration (cells, synapses, dendrites, local circuits), experience-dependent adaptation and plasticity

  20. Photo:AndrewJ.Martinez 16 MaxPlanckResearch 3 | 09

    E-Print Network [OSTI]

    interested in what are known as cyclic nucleotide-gated channels (CNG chan- nels) and pacemaker channels (HCN channels). CNG

  1. Das Wissenschaftsmagazin der Max-Planck-Gesellschaft 2.2010 WIRTSCHAFTSPOLITIK

    E-Print Network [OSTI]

    Falge, Eva

    in Kohlen- dioxid-arme und erneuerbare Energien in den kommen- den Jahrzehnten die wichtigsten Triebfedern

  2. Spezial | 10 MaxPlanckForschung 3 das Dilemma scheint unauflsbar: Bis zum Jahr 2030

    E-Print Network [OSTI]

    Investitionschancen in Kohlen- dioxid-arme und erneuerbare Energien in den kommen- den Jahrzehnten die wichtigsten

  3. 2 | 10 MaxPlanckForschung 3 das Dilemma scheint unauflsbar: Bis zum Jahr 2030

    E-Print Network [OSTI]

    Investitionschancen in Kohlen- dioxid-arme und erneuerbare Energien in den kommen- den Jahrzehnten die wichtigsten

  4. Princeton, Max Planck Society launch new research center for plasma physics

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-Rich Matrices in HydrothermalMagneticAiter U.S.pso/about/jobs/|

  5. Heat Hyperbolic Diffusion in Planck Gas

    E-Print Network [OSTI]

    Miroslaw Kozlowski; Janina Marciak-Kozlowska

    2006-07-06

    In this paper we investigate the diffusion of the thermal pulse in Planck Gas. We show that the Fourier diffusion equation gives the speed of diffusion, v > c and breaks the causality of the thermal processes in Planck gas .For hyperbolic heat transport v

  6. WMAP OBSERVATIONS OF PLANCK ESZ CLUSTERS

    SciTech Connect (OSTI)

    Ma Yinzhe; Hinshaw, Gary; Scott, Douglas [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1 (Canada)

    2013-07-10

    We examine the Sunyaev-Zeldovich (SZ) effect in the seven year Wilkinson Microwave Anisotropy Probe (WMAP) data by cross-correlating it with the Planck Early-release Sunyaev-Zeldovich catalog. Our analysis proceeds in two parts. We first perform a stacking analysis in which the filtered WMAP data are averaged at the locations of the 175 Planck clusters. We then perform a regression analysis to compare the mean amplitude of the SZ signal, Y{sub 500}, in the WMAP data to the corresponding amplitude in the Planck data. The aggregate Planck clusters are detected in the seven year WMAP data with a signal-to-noise ratio of 16.3. In the regression analysis, we find that the SZ amplitude measurements agree to better than 25%: a = 1.23 {+-} 0.18 for the fit Y{sup wmap}{sub 500}= aY{sup planck}{sub 500}.

  7. Ralf Weisse and Hans von Storch, Helmholtz-Zentrum Geesthacht, Institute for Coastal Research, Contact: ralf.weisse@hzg.de Helmholtz-Zentrum Geesthacht Max-Planck-Strae 1 21502 Geesthacht Phone +49 (0)4152 87-2819 Fax +49 (0)4152 87-2818 www.hzg.de

    E-Print Network [OSTI]

    von Storch, Hans

    of offshore wind farms, their interplay with conventional power plants and the assessment of ocean energy in establishing offshore wind farms. In face of the limited observational data available coastDat was used in many of installation of offshore wind farms (from Wiese 2008: Auswirkungen der Offshore-Windenergie auf den Betrieb von

  8. DOE Awards 265 Million Hours of Supercomputing Time to Advance...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    National Institute of Standards and Technology; the Max-Planck Institute for Quantum Optics in Germany; CERFACS, the European Center for Research and Advanced Training in...

  9. ORIGINAL RESEARCH ARTICLE published: 22 June 2012

    E-Print Network [OSTI]

    Saxe, Rebecca

    Department of Human Perception, Cognition, and Action, Max Planck Institute for Biological Cybernetics, Tuebingen, Germany 3 Department of Brain and Cognitive Sciences, Massachusetts Institute of Technology

  10. LOWER BOUNDS ON MAGNETIC FIELDS IN INTERGALACTIC VOIDS FROM LONG...

    Office of Scientific and Technical Information (OSTI)

    (Japan) Max-Planck-Institut fuer Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg (Germany) Theory Center, Institute of Particle and Nuclear Studies, KEK, 1-1, Oho, Tsukuba...

  11. Opacity of iron, nickel, and copper plasmas in the x-ray wavelength...

    Office of Scientific and Technical Information (OSTI)

    2 more ; Max-Planck-Institut fuer Quantenoptik, D-85748 Garching 3 ; Institute of Nuclear Fusion, Universidad Politecnica de Madrid, Spain and Laboratoire d'Optique...

  12. Max Tech and Beyond Design Competition

    Broader source: Energy.gov [DOE]

    The Max Tech and Beyond Design Competition is an annual competition run by the Department of Energy (DOE) and the Lawrence Berkeley National Laboratory (LBNL) that challenges students to design...

  13. Desensitizing Inflation from the Planck Scale

    E-Print Network [OSTI]

    Daniel Baumann; Daniel Green

    2010-04-21

    A new mechanism to control Planck-scale corrections to the inflationary eta parameter is proposed. A common approach to the eta problem is to impose a shift symmetry on the inflaton field. However, this symmetry has to remain unbroken by Planck-scale effects, which is a rather strong requirement on possible ultraviolet completions of the theory. In this paper, we show that the breaking of the shift symmetry by Planck-scale corrections can be systematically suppressed if the inflaton field interacts with a conformal sector. The inflaton then receives an anomalous dimension in the conformal field theory, which leads to sequestering of all dangerous high-energy corrections. We analyze a number of models where the mechanism can be seen in action. In our most detailed example we compute the exact anomalous dimensions via a-maximization and show that the eta problem can be solved using only weakly-coupled physics.

  14. Planck's Radiation Law in the Quantized Universe

    E-Print Network [OSTI]

    Rainer Collier

    2014-09-15

    Physical research looks for clues to quantum properties of the gravitational field. On the basis of the common Schr\\"odinger theory, a simple model of the quantization of a Friedmann universe comprising dust and radiation is investigated. With regard to energy quantization, the result suggests a universal limitation of the energy spacing between neighbouring quantum states by the Planck energy. Applied to black-body radiation, a modified Planck radiation law follows. If this could be verified in the laboratory, it would provide a direct hint at quantum properties of the space-time manifold.

  15. Massive Gauge Fields and the Planck Scale

    E-Print Network [OSTI]

    Acosta, G D

    2004-01-01

    The present work is devoted to massive gauge fields in special relativity with two fundamental constants-the velocity of light, and the Planck length, so called doubly special relativity (DSR). The two invariant scales are accounted for by properly modified boost parameters. Within above framework we construct the vector potential as the (1/2,0)x(0,1/2) direct product, build the associated field strength tensor together with the Dirac spinors and use them to calculate various observables as functions of the Planck length.

  16. Massive Gauge Fields and the Planck Scale

    E-Print Network [OSTI]

    G. D. Acosta; M. Kirchbach

    2004-11-09

    The present work is devoted to massive gauge fields in special relativity with two fundamental constants-the velocity of light, and the Planck length, so called doubly special relativity (DSR). The two invariant scales are accounted for by properly modified boost parameters. Within above framework we construct the vector potential as the (1/2,0)x(0,1/2) direct product, build the associated field strength tensor together with the Dirac spinors and use them to calculate various observables as functions of the Planck length.

  17. Axion hot dark matter bounds after Planck

    SciTech Connect (OSTI)

    Archidiacono, Maria; Hannestad, Steen; Mirizzi, Alessandro; Raffelt, Georg; Wong, Yvonne Y.Y. E-mail: sth@phys.au.dk E-mail: raffelt@mpp.mpg.de

    2013-10-01

    We use cosmological observations in the post-Planck era to derive limits on thermally produced cosmological axions. In the early universe such axions contribute to the radiation density and later to the hot dark matter fraction. We find an upper limit m{sub a} < 0.67 eV at 95% C.L. after marginalising over the unknown neutrino masses, using CMB temperature and polarisation data from Planck and WMAP respectively, the halo matter power spectrum extracted from SDSS-DR7, and the local Hubble expansion rate H{sub 0} released by the Carnegie Hubble Program based on a recalibration of the Hubble Space Telescope Key Project sample. Leaving out the local H{sub 0} measurement relaxes the limit somewhat to 0.86 eV, while Planck+WMAP alone constrain the axion mass to 1.01 eV, the first time an upper limit on m{sub a} has been obtained from CMB data alone. Our axion limit is therefore not very sensitive to the tension between the Planck-inferred H{sub 0} and the locally measured value. This is in contrast with the upper limit on the neutrino mass sum, which we find here to range from ? m{sub ?} < 0.27 eV at 95% C.L. combining all of the aforementioned observations, to 0.84 eV from CMB data alone.

  18. Entanglement induced Sub-Planck structures

    E-Print Network [OSTI]

    Jitesh R. Bhatt; Prasanta K. Panigrahi; Manan Vyas

    2007-08-31

    We study Wigner function of a system describing entanglement of two cat-states. Quantum interferece arising due to entanglement is shown to produce sub-Planck structures in the phase-space plots of the Wigner function. Origin of these structures in our case depends on entanglement unlike those in Zurek \\cite{Zurek}. It is argued that the entangled cat-states are better suited for carrying out precision measurements.

  19. Research Life Cycle Max J. Egenhofer

    E-Print Network [OSTI]

    Egenhofer, Max J.

    Research Life Cycle Max J. Egenhofer #12;Five Phases Research Orientation Phase Research Startup Phase Research Proposal Preparation Phase Active Research Phase Harvest #12;Research Orientation Phase Identify the field in which you want to do research Do some selected reading · Identify key concepts

  20. Introduction to Graduate Research Max J. Egenhofer

    E-Print Network [OSTI]

    Egenhofer, Max J.

    a graduate degree A researcher's credentials (CV, publication list) Types of research Literature search SpeedSIE 501 Introduction to Graduate Research Max J. Egenhofer #12;Pragmatics 1-credit course · First;Topics Covered Measures of research success Goals of academic research Research life cycle How to get

  1. Planck 2015 results. V. LFI calibration

    E-Print Network [OSTI]

    Ade, P A R; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaglia, P; Battaner, E; Benabed, K; Benoît, A; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bock, J J; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Catalano, A; Chamballu, A; Christensen, P R; Colombi, S; Colombo, L P L; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Dickinson, C; Diego, J M; Dole, H; Donzelli, S; Doré, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Giard, M; Giraud-Héraud, Y; Gjerløw, E; González-Nuevo, J; Górski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versillé, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, T S; Knoche, J; Krachmalnicoff, N; Kunz, M; Kurki-Suonio, H; Lagache, G; Lähteenmäki, A; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leahy, J P; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vørnle, M; López-Caniego, M; Lubin, P M; Macías-Pérez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, P G; Martínez-González, E; Masi, S; Matarrese, S; McGehee, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nørgaard-Nielsen, H U; Novikov, D; Novikov, I; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Partridge, B; Pasian, F; Patanchon, G; Pearson, T J; Peel, M; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Pierpaoli, E; Pietrobon, D; Pointecouteau, E; Polenta, G; Pratt, G W; Prézeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rebolo, R; Reinecke, M; Remazeilles, M; Renzi, A; Rocha, G; Romelli, E; Rosset, C; Rossetti, M; Roudier, G; Rubiño-Martín, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Türler, M; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vassallo, T; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Watson, R; Wehus, I K; Wilkinson, A; Yvon, D; Zacchei, A; Zonca, A

    2015-01-01

    We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. Our 2015 LFI analysis provides an independent Solar dipole estimate in excellent agreement with that of HFI and within $1\\sigma$ (0.3 % in amplitude) of the WMAP value. This 0.3 % shift in the peak-to-peak dipole temperature from WMAP and a global overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45 % (30 GHz), 0.64 % (44 GHz), and 0.82 % (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is at the level of 0.20 % for the 70 GHz map, 0.26 % for the 44 GHz...

  2. Towards Heavy Fermions in Europium Intermetallic Compounds

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Yu. Kucherenko (Technische Universitt Dresden, and National Academy of Sciences of Ukraine); N. Caroca-Canales, C. Krellner, and C. Geibel (Max-Planck-Institut fr Chemische...

  3. DOE's Office of Science Awards 95 Million Hours of Supercomputing...

    Office of Environmental Management (EM)

    Oceanographic and Atmospheric Administration and the Max-Planck Institute for Quantum Optics in Germany. The Council on Competitiveness is the only non-governmental group of...

  4. GALPROP Explanatory Supplement Andrew W. Strong

    E-Print Network [OSTI]

    Strong, Andrew W.

    GALPROP Explanatory Supplement Andrew W. Strong Max-Planck-Institut f¨ur extraterrestrische Physik Supplement . . . . . . . . . . . . . . . . . . . . . . . 5 2 General Principles 5 2.1 Transport equation

  5. Giant Protease TPP II's Structure, Mechanism Uncovered

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Lab, the University of California, Berkeley, and the Max Planck Institute of Biochemistry combined single-particle cryo-electron microscopy and x-ray crystallography at ALS...

  6. Light Induced Superconductivity | Stanford Synchrotron Radiation...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Light Induced Superconductivity Wednesday, August 5, 2015 - 3:00pm SLAC, Redtail Hawk Conference Room 108A Speaker: Daniele Nicoletti, Max Planck Institute for the Structure and...

  7. Duke Mathematical Journal 125 2004, 329-349.

    E-Print Network [OSTI]

    Penkov, Ivan

    subalgebras, 1Work supported in part by an NSF GIG grant, by the Max-Planck-Institute for Mathematics in Bonn

  8. Experience Matters: Information Acquisition Optimizes Probability Gain

    E-Print Network [OSTI]

    Cottrell, Garrison W.

    ,2,3, Craig R.M. McKenzie2, Garrison W. Cottrell2, and Terrence J. Sejnowski2,3,4 1Max Planck Institute

  9. EXTRAGALACTIC BACKGROUND LIGHT FROM HIERARCHICAL GALAXY FORMATION...

    Office of Scientific and Technical Information (OSTI)

    States) Max-Planck-Institut fuer Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg (Germany) Research Center for Space and Cosmic Evolution, Ehime University, Bunkyo-cho,...

  10. Metagenomic and Metaproteomic Analyses of Symbioses between Bacteria and Gutless Marine Worms (2014 DOE JGI Genomics of Energy & Environment Meeting)

    SciTech Connect (OSTI)

    Dubilier, Nicole

    2014-03-19

    Nicole Dubilier of the Max Planck Institute speaks at the 9th Annual Genomics of Energy & Environment Meeting on March 20, 2014 in Walnut Creek, Calif.

  11. Der Band ist als Beitrag des Berliner Ar-chivs der Max-Planck-Gesellschaft zu den

    E-Print Network [OSTI]

    Falge, Eva

    . Interessante Presseartikel ­ vor allem aus der Zeit zwischen 1930 und 1937 ­ hat Bernd Hoffmann ausgewählt. Der aussterben und daß die heranwachsende Generation von vornherein mit der Wahr- heit vertraut gemacht wird

  12. 42 MaxPlanckForschung 2 | 11 Wir Menschen sprechen nicht nur gerne und viel, wir tun

    E-Print Network [OSTI]

    Falge, Eva

    beeinflusst. Im Hypothalamus unterdrückt Insulin den Forschern zufolge bei fettreicher Ernäh- rung das Hypothalamus überstimmen. Dies er- klärt möglicherweise, warum wir bei entsprechender Metabolism, 7. Juni 2011; Nature Neuro- science, 5. Juni 2011) Insulin im Mittelhirn und im Hypothalamus

  13. 4 | 10 MaxPlanckForschung 3 seit ich Anfang der 1970er-Jahre in einem orangefarbe-

    E-Print Network [OSTI]

    Thema Indien nachlesen können, erforscht die Gruppe die Ursachen der Luftverschmutzung und unter- sucht

  14. The best inflationary models after Planck

    SciTech Connect (OSTI)

    Martin, Jérôme; Vennin, Vincent; Ringeval, Christophe; Trotta, Roberto E-mail: christophe.ringeval@uclouvain.be E-mail: vennin@iap.fr

    2014-03-01

    We compute the Bayesian evidence and complexity of 193 slow-roll single-field models of inflation using the Planck 2013 Cosmic Microwave Background data, with the aim of establishing which models are favoured from a Bayesian perspective. Our calculations employ a new numerical pipeline interfacing an inflationary effective likelihood with the slow-roll library ASPIC and the nested sampling algorithm MultiNest. The models considered represent a complete and systematic scan of the entire landscape of inflationary scenarios proposed so far. Our analysis singles out the most probable models (from an Occam's razor point of view) that are compatible with Planck data, while ruling out with very strong evidence 34% of the models considered. We identify 26% of the models that are favoured by the Bayesian evidence, corresponding to 15 different potential shapes. If the Bayesian complexity is included in the analysis, only 9% of the models are preferred, corresponding to only 9 different potential shapes. These shapes are all of the plateau type.

  15. Neurton Damage and MAX Phase Ternary Compounds

    SciTech Connect (OSTI)

    Barsoum, Michael; Hoffman, Elizabeth; Sindelar, Robert; Garcua-Duaz, Brenda; Kohse, Gordon

    2014-06-17

    The Demands of Gen IV nuclear power plants for long service life under neutron radiation at high temperature are severe. Advanced materials that would withstand high temperatures (up to 1000+ C) to high doses in a neutron field would be ideal for reactor internal structures and would add to the long service life and reliability of the reactors. The objective of this work is to investigate the resonse of a new class of machinable, conductive, layered, ternary transition metal carbides and nitrides - the so-called MAX phases - to low and moderate neutron dose levels.

  16. MaxPower Inc | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History View NewTexas:Montezuma,InformationIllinois:Martin,OpenMatthews,Maverick County,MaxPower Inc

  17. Bernhard E. Riecke bernhard.riecke@tuebingen.mpg.de

    E-Print Network [OSTI]

    Bernhard E. Riecke bernhard.riecke@tuebingen.mpg.de Max Planck Institute for Biological Cybernetics Soesterberg The Netherlands AG Heinrich H. Bu¨ lthoff Max Planck Institute for Biological Cybernetics Presence, Vol. 11, No. 5, October 2002, 443­ 473 © 2002 by the Massachusetts Institute of Technology Visual

  18. ForPeerReview Atypical brain activation patterns during a face-to-face joint

    E-Print Network [OSTI]

    Saxe, Rebecca

    for Biological Cybernetics, 72076 Tuebingen, Germany 5. Massachusetts Institute of Technology, Cambridge, MA; Massachusetts Institute of Technology, Brain and Cognitive Sciences Kleiner, Mario; Max Planck Institute for Biological Cybernetics, Human Perception, Cognition, and Action Pearrow, Mark; Massachusetts Institute

  19. Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates

    E-Print Network [OSTI]

    ,

    2015-01-01

    The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources on the sky, including distant objects in the high-redshift Universe traced by their dust emission. A novel method, based on a component-separation procedure using a combination of Planck and IRAS data, has been applied to select the most luminous cold submm sources with spectral energy distributions peaking between 353 and 857GHz at 5' resolution. A total of 2151 Planck high-z source candidates (the PHZ) have been detected in the cleanest 26% of the sky, with flux density at 545GHz above 500mJy. Embedded in the cosmic infrared background close to the confusion limit, these high-z candidates exhibit colder colours than their surroundings, consistent with redshifts z>2, assuming a dust temperature of 35K and a spectral index of 1.5. First follow-up observations obtained from optical to submm have confirmed that this list consists of tw...

  20. AVTA: 2013 Ford C-MAX HEV Testing Results

    Broader source: Energy.gov [DOE]

    VTO's National Laboratories have tested and collected both dynamometer and fleet data for the Ford C-MAX HEV (a hybrid electric vehicle).

  1. A New Basis for Interpretation of the Planck Length

    E-Print Network [OSTI]

    C. L. Herzenberg

    2006-10-17

    A critical length has recently been identified that appears to provide a fundamental limit distinguishing quantum behavior from classical behavior. Because of the unique association between critical length and mass, it appears that we can correlate the mass of an object with the size over which its quantum behavior is manifested. When the expression for the critical length is set equal to the Planck length, we find an associated mass value that in magnitude corresponds to an approximation of the mass of the visible universe. This would appear to suggest that the quantum behavior associated with the universe as a whole would be manifested at distances comparable to or smaller than the Planck length. Accordingly, it would appear that all position measurements would be subject to uncertainties at the limit of the Planck length, so that the Planck length sets a fundamental limit on position determination.

  2. On Quanti ed Weighted MAX-SAT Amol Dattatraya Mali

    E-Print Network [OSTI]

    Mali, Amol D.

    On Quanti#12;ed Weighted MAX-SAT Amol Dattatraya Mali Dept. of Electrical Engg. & Computer Science, University of Wisconsin, Milwaukee, WI 53211, mali@miller.cs.uwm.edu, Phone: 1-414-229-6762, Fax: 1-414-229-2769, http://www.cs.uwm.edu/faculty/mali Abstract In this paper we introduce quanti#12;ed weighted MAX-SAT (Q

  3. Planck Intermediate Results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes in the Canary Islands Observatories

    E-Print Network [OSTI]

    Ade, P A R; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Barrena, R; Bartolo, N; Battaner, E; Benabed, K; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bikmaev, I; Böhringer, H; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Burenin, R; Burigana, C; Calabrese, E; Cardoso, J -F; Catalano, A; Chamballu, A; Chary, R -R; Chiang, H C; Chon, G; Christensen, P R; Clements, D L; Colombo, L P L; Combet, C; Comis, B; Crill, B P; Curto, A; Cuttaia, F; Dahle, H; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Diego, J M; Dole, H; Donzelli, S; Doré, O; Douspis, M; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Ferragamo, A; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Fromenteau, S; Galeotta, S; Galli, S; Ganga, K; Génova-Santos, R T; Giard, M; Gjerløw, E; González-Nuevo, J; Górski, K M; Gruppuso, A; Hansen, F K; Harrison, D L; Hempel, A; Hernández-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, T R; Keihänen, E; Keskitalo, R; Khamitov, I; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; León-Tavares, J; Levrier, F; Lietzen, H; Liguori, M; Lilje, P B; Linden-Vørnle, M; López-Caniego, M; Lubin, P M; Macías-Pérez, J F; Maffei, B; Maino, D; Mandolesi, N; Maris, M; Martin, P G; Martínez-González, E; Masi, S; Matarrese, S; McGehee, P; Melchiorri, A; Mennella, A; Migliaccio, M; Miville-Deschênes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Novikov, D; Novikov, I; Oxborrow, C A; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Perdereau, O; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Plaszczynski, S; Pointecouteau, E; Polenta, G; Pratt, G W; Prunet, S; Puget, J -L; Rachen, J P; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubiño-Martín, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Stolyarov, V; Streblyanska, A; Sudiwala, R; Sunyaev, R; Suur-Uski, A -S; Sygnet, J -F; Terenzi, L; Toffolatti, L; Tomasi, M; Tramonte, D; Tristram, M; Tucci, M; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; Yvon, D; Zacchei, A; Zonca, A

    2015-01-01

    We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories, as part of the general optical follow-up programme undertaken by the Planck collaboration. In total, 78 SZ sources are discussed. Deep imaging observations were obtained for most of those sources; spectroscopic observations in either in long-slit or multi-object modes were obtained for many. We found optical counterparts for 73 of the 78 candidates. This sample includes 53 spectroscopic redshifts determinations, 20 of them obtained with a multi-object spectroscopic mode. The sample contains new redshifts for 27 Planck clusters that were not included in the first Planck SZ source catalogue (PSZ1).

  4. Begoa Daz Menndez CURRICULUM VITAE

    E-Print Network [OSTI]

    Verschure, Paul

    : Spanish Government travel grant to visit the F.C. Donders Center for Cognitive Neuroimaging, Nijmegen, The Netherlands. 2006: Spanish Government travel grant to visit the Max Planck Institute for Physcholinguistics, Nijmegen, The Netherlands. 2005: Spanish Government travel grant to visit Max Planck Institute for Human

  5. 2 / 2 0 0 7 M A X P L A N C K R E S E A R C H 27 THE WORLD IN OUR HEADS

    E-Print Network [OSTI]

    Chaos reigns. I am on my way to the Max Planck Institute for Biologi- cal Cybernetics in Tübingen, where Processes at the MAX PLANCK INSTITUTE FOR BIOLOGICAL CYBERNETICS in Tübingen are trying to answer. Led researcher studied mathematics and theoretical physics at the Swiss Federal Insti- tute of Technology (ETH

  6. Multi-loop Pilot Behaviour Identification in Response to Simultaneous Visual and Haptic Stimuli

    E-Print Network [OSTI]

    Cybernetics, T¨ubingen, Germany Delft University of Technology, Delft, The Netherlands Heinrich H. B Mario Olivari Max Planck Institute for Biological Cybernetics, T¨ubingen, Germany University of Pisa¨ulthoff§ Max Planck Institute for Biological Cybernetics, T¨ubingen, Germany Department of Brain and Cognitive

  7. First Evaluation of A Novel Tactile Display Exerting Shear Force via Lateral Displacement

    E-Print Network [OSTI]

    DREWING Max Planck Institute for Biological Cybernetics MICHAEL FRITSCHI Technische Universit¨at M¨unchen REGINE ZOPF, and MARC O. ERNST Max Planck Institute for Biological Cybernetics and MARTIN BUSS Technische psychophysical knowledge based on this new technology will in return be used to improve the design of the display

  8. Gauge-flation confronted with Planck

    SciTech Connect (OSTI)

    Namba, Ryo; Dimastrogiovanni, Emanuela; Peloso, Marco E-mail: ema@physics.umn.edu

    2013-11-01

    Gauge-flation is a recently proposed model in which inflation is driven solely by a non-Abelian gauge field thanks to a specific higher order derivative operator. The nature of the operator is such that it does not introduce ghosts. We compute the cosmological scalar and tensor perturbations for this model, improving over an existing computation. We then confront these results with the Planck data. The model is characterized by the quantity ? ? g{sup 2}Q{sup 2}/H{sup 2} (where g is the gauge coupling constant, Q the vector vev, and H the Hubble rate). For ? < 2, the scalar perturbations show a strong tachyonic instability. In the stable region, the scalar power spectrum n{sub s} is too low at small ?, while the tensor-to-scalar ratio r is too high at large ?. No value of ? leads to acceptable values for n{sub s} and r, and so the model is ruled out by the CMB data. The same behavior with ? was obtained in Chromo-natural inflation, a model in which inflation is driven by a pseudo-scalar coupled to a non-Abelian gauge field. When the pseudo-scalar can be integrated out, one recovers the model of Gauge-flation plus corrections. It was shown that this identification is very accurate at the background level, but differences emerged in the literature concerning the perturbations of the two models. On the contrary, our results show that the analogy between the two models continues to be accurate also at the perturbative level.

  9. Impacts of dark energy on weighing neutrinos after Planck 2015

    E-Print Network [OSTI]

    Zhang, Xin

    2015-01-01

    We investigate how dark energy properties impact the cosmological limits on the total mass of active neutrinos. We consider two typical, simple dark energy models (that have only one more additional parameter than $\\Lambda$CDM), i.e., the $w$CDM model and the holographic dark energy (HDE) model, as examples, to make an analysis. In the cosmological fits, we use the Planck 2015 temperature and polarization data, in combination with other low-redshift observations, including the baryon acoustic oscillations, type Ia supernovae, and Hubble constant measurement, as well as the Planck lensing measurements. We find that, once dynamical dark energy is considered, the degeneracy between $\\sum m_\

  10. LINEAR-PROGRAMMING DESIGN AND ANALYSIS OF FAST ALGORITHMS FOR MAX 2-CSP

    E-Print Network [OSTI]

    Scott, Alexander Alexander

    LINEAR-PROGRAMMING DESIGN AND ANALYSIS OF FAST ALGORITHMS FOR MAX 2-CSP ALEXANDER D. SCOTT AND GREGORY B. SORKIN Abstract. The class Max (r, 2)-CSP (or simply Max 2-CSP) consists of constraint(G) (13/75 + o(1))m, which gives a faster Max 2-CSP algorithm that uses exponential space: running in time

  11. PLANCK'S FORMULA IN CLASSICAL MECHANICS Andrea CARATI, Luigi GALGANI

    E-Print Network [OSTI]

    .e. by considering processes involving continuous variations of energy. A particular effort in this direction), the expected energy distribution is apparently frozen about the initial one, with the addition of a ``thermal of classical mechanics. We prove that the expected energy distribution of the oscillators obeys Planck

  12. 2012, . 26, . 1?? IF ENERGY IS NOT PRESERVED, THEN PLANCK'S

    E-Print Network [OSTI]

    Kreinovich, Vladik

    are consistent with the original theory or with an alternative theory. In particular, to check whether energy 2012, . 26, . 1­?? 000.000 IF ENERGY IS NOT PRESERVED, THEN PLANCK'S CONSTANT IS NO LONGER, we need to for- mulate an alternative theory and check whether the experimental results

  13. Howard E. Haber Santa Cruz Institute for Particle Physics (SCIPP)

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    Physics, H.E. Haber and A.E. Nelson, editors (World Scientific, Singapore, 2004). 3. Proceedings of the 5, H.E. Haber, and J. Siegrist, editors (World Scientific, Singapore, 1996). 5. From the Planck Scale Institute in Elementary Particle Physics, vols. I and II, H.E. Haber, editor, (World Scientific, Singapore

  14. Planck's Dusty GEMS: Gravitationally lensed high-redshift galaxies discovered with the Planck survey

    E-Print Network [OSTI]

    Canameras, R; Guery, D; McKenzie, T; Koenig, S; Petitpas, G; Dole, H; Frye, B; Flores-Cacho, I; Montier, L; Negrello, M; Beelen, A; Boone, F; Dicken, D; Lagache, G; Floch, E Le; Altieri, B; Bethermin, M; Chary, R; De Zotti, G; Giard, M; Kneissl, R; Krips, M; Malhotra, S; Martinache, C; Omont, A; Pointecouteau, E; Puget, J -L; Scott, D; Soucail, G; Valtchanov, I; Welikala, N; Yan, L

    2015-01-01

    We present an analysis of 11 bright far-IR/submm sources discovered through a combination of the Planck survey and follow-up Herschel-SPIRE imaging. Each source has a redshift z=2.2-3.6 obtained through a blind redshift search with EMIR at the IRAM 30-m telescope. Interferometry obtained at IRAM and the SMA, and optical/near-infrared imaging obtained at the CFHT and the VLT reveal morphologies consistent with strongly gravitationally lensed sources. Additional photometry was obtained with JCMT/SCUBA-2 and IRAM/GISMO at 850 um and 2 mm, respectively. All objects are bright, isolated point sources in the 18 arcsec beam of SPIRE at 250 um, with spectral energy distributions peaking either near the 350 um or the 500 um bands of SPIRE, and with apparent far-infrared luminosities of up to 3x10^14 L_sun. Their morphologies and sizes, CO line widths and luminosities, dust temperatures, and far-infrared luminosities provide additional empirical evidence that these are strongly gravitationally lensed high-redshift gala...

  15. arXiv:astro-ph/0609503v118Sep2006 Observations Supporting the Role of Magnetoconvection in

    E-Print Network [OSTI]

    Lin, Gang

    Supply to the Quiescent Solar Atmosphere Scott W. McIntosh, Alisdair R. Davey, Donald M. Hassler USA Werner Curdt, Klaus Wilhelm Max Planck Institute for Solar System Research, Max-Planck-Str. 2 mechanisms behind the production and suste- nance of the quiescent solar corona and solar wind poses two

  16. Curriculum Vitae Personal Information

    E-Print Network [OSTI]

    Pérez-Cruz, Fernando

    .perezcruz@gmail.com Web page : http://www.tsc.uc3m.es/fernando Academics · Ph.D. in Telecommunication Engineering, Dec 2000. · B.Sc. & M.Sc. in Telecommunication Engineering (Electrical and Electronic Engineering. Biological Cybernetics, Max Planck Institute in T¨ubingen. Oct 2005. 3. Biological Cybernetics, Max Planck

  17. Adolfo, Poma Computational Physics Group

    E-Print Network [OSTI]

    Roma "La Sapienza", Università di

    , Poster Session, Regensburg, Germany. Sep. 2009 Physics of biopolymers: Theory and simulation, Istanbul,Turkey, Max Planck Institute for Polymer Research, Germany. - Major in Physics, Cum laude -- Phd Thesis title.A.U.S.T. Scholarship, Italy. 2009-2011 DAAD Scholarship, Germany. 2008­2009 International Max Planck Research School

  18. CURRICULUM VITAE PhD in Materials Science and Technology, February 2005 July 2008

    E-Print Network [OSTI]

    Gizeli, Electra

    -Planck Institute for Polymer Research, Mainz, Germany Materials Science and Technology Department, University.10.2006 For: `Analytical Methods in the Development of Science and Technology of Polymers' Max PlanckCURRICULUM VITAE EDUCATION PhD in Materials Science and Technology, February 2005 ­ July 2008 Max

  19. Ruddle, R. A., Volkova, E., & Blthoff, H. H. (in press). Learning to walk in virtual reality. ACM Transactions on Applied Perception.

    E-Print Network [OSTI]

    Institute for Biological Cybernetics, Tübingen, Germany 3 Department of Brain and Cognitive Engineering Research Foundation of Korea funded by the Ministry of Education, Science and Technology (R31 Volkova, Max Planck Institute for Biological Cybernetics, Spemannstrasse 38, 72076 Tübingen, Germany

  20. System Identification and Signal Processing for PID Control of B0 Shim Systems in Ultra-High Field Magnetic Resonance Applications

    E-Print Network [OSTI]

    for Biological Cybernetics, Tübingen, Germany Institute for Biomedical Engineering, University and ETH Zurich for Biological Cybernetics, Tübingen, Germany. Graduate School of Neural & Behavioural Sciences, University Cybernetics, Tübingen, Germany. (e-mail: nikolai.avdievitch@tuebingen.mpg.de) ***Max Planck Institute

  1. Planetary and Space Science 55 (2007) 13981413 The BepiColombo Laser Altimeter (BELA): Concept and

    E-Print Network [OSTI]

    Wieczorek, Mark

    2007-01-01

    a Physikalisches Institut, Sidlerstr. 5, University of Bern, CH-3012 Bern, Switzerland b Deutsches Zentrum fu. 5, University of Bern, CH-3012 Bern, Switzerland e Max-Planck-Institut fuer Sonnensystemforschung

  2. Distance Priors from \\emph{Planck} 2015 data

    E-Print Network [OSTI]

    Qing-Guo Huang; Ke Wang; Sai Wang

    2015-09-03

    We update the distance priors by adopting $Planck~ \\textrm{TT,TE,EE}+\\textrm{lowP}$ data released in 2015, and our results impose at least $30\\%$ tighter constraints than those from $Planck~ \\textrm{TT}+\\textrm{lowP}$. Combining the distance priors with the combination of supernova Union~2.1 compilation of 580 SNe (Union~2.1) and low redshift Baryon Acoustic Oscillation (BAO) data, we constrain the cosmological parameters in the freely binned dark energy (FBDE) and FBDE$+\\Omega_k$ models respectively, and find that the equations of state of dark energy in both models are consistent with $w=-1$. Furthermore, we show that the tension with the BAO data at $z=2.34$ from Ly$\\alpha$ forest (Ly$\\alpha$F) auto-correlation and Combined Ly$\\alpha$F cannot be relaxed in the FBDE and FBDE$+\\Omega_k$ models.

  3. Statistical Measures of Planck Scale Signal Correlations in Interferometers

    E-Print Network [OSTI]

    Hogan, Craig J

    2015-01-01

    A model-independent statistical framework is presented to interpret data from systems where the mean time derivative of positional cross correlation between world lines, a measure of spreading in a quantum geometrical wave function, is measured with a precision smaller than the Planck time. The framework provides a general way to constrain possible departures from perfect independence of classical world lines, associated with Planck scale bounds on positional information. A parametrized candidate set of possible correlation functions is shown to be consistent with the known causal structure of the classical geometry measured by an apparatus, and the holographic scaling of information suggested by gravity. Frequency-domain power spectra are derived that can be compared with interferometer data. Simple projections of sensitivity for specific experimental set-ups suggests that measurements will directly yield constraints on a universal time derivative of the correlation function, and thereby confirm or rule out ...

  4. Water Quality for Livestock Max Irsik DVM, MAB

    E-Print Network [OSTI]

    Watson, Craig A.

    Water Quality for Livestock Max Irsik DVM, MAB Beef Cattle Extension Veterinarian University of Florida College of Veterinary Medicine Water is an essential nutrient for humans and livestock and drinking water is the primary source of water for most cattle. The most important aspect of water

  5. Molecular motors interacting with their own tracks Max N. Artyomov

    E-Print Network [OSTI]

    Molecular motors interacting with their own tracks Max N. Artyomov Department of Chemistry; published 17 April 2008 Dynamics of molecular motors that move along linear lattices and interact with them exactly solvable discrete-state "burnt- bridge" models. Molecular motors are viewed as diffusing particles

  6. Quantum Algorithms for Evaluating MIN-MAX Trees

    E-Print Network [OSTI]

    Richard Cleve; Dmitry Gavinsky; David L. Yeung

    2007-10-31

    We present a bounded-error quantum algorithm for evaluating Min-Max trees. For a tree of size N our algorithm makes N^{1/2+o(1)} comparison queries, which is close to the optimal complexity for this problem.

  7. SINGLE-ZONE STACK-DOMINATED INFILTRATION MODELING Max Sherman

    E-Print Network [OSTI]

    dominates and total ventilation can be calculated by treating other effects (i.e., wind and small fansSINGLE-ZONE STACK-DOMINATED INFILTRATION MODELING Max Sherman Energy Performance of Buildings Group Energy, Office of Buildings and Community Systems Building Systems Division of the U.S. Department

  8. Naive Geography Max J. Egenhofer and David M. Mark

    E-Print Network [OSTI]

    California at Santa Barbara, University of

    Naive Geography by Max J. Egenhofer and David M. Mark National Center for Geographic Information;1 Abstract This paper defines the notion and concepts of Naive Geography, the field of study that is concerned with formal models of the common-sense geographic world. Naive Geography is the body of knowledge

  9. On an Improvement of the Planck radiation Energy Distribution

    E-Print Network [OSTI]

    Diego Saa

    2006-07-18

    The probability distribution function for thermodynamics and econophysics is obtained by solving an equilibrium equation. This approach is different from the common one of optimizing the entropy of the system or obtaining the state of maximum probability, which usually obtains as a result the Boltzmann distribution. The Gamma distribution is proposed as a better equation to describe the blackbody radiation in substitution of Planck's radiation equation. Also, a new form of entropy is proposed, that maintains the correct relation with the Clausius' formula.

  10. Precision measurements of the Planck and Avogadro constants

    E-Print Network [OSTI]

    Bettin, Horst; Man, John; Mana, Giovanni; Massa, Enrico; Picard, Alain

    2013-01-01

    Precision measurements of the fundamental constants are tour de force of basic metrology, where the useful information is usually beyond the last digit of the measured value. They challenge theoretical models and measurement technologies and set a network of measurement equations on which a universal system of units can be built, which stems from the most basic concepts of physics. Because of their connection with the mass unit, the Avogadro and Planck constants are on the spotlight.

  11. Orbit-averaged guiding-center Fokker-Planck operator

    SciTech Connect (OSTI)

    Brizard, A. J. [Department of Chemistry and Physics, Saint Michael's College, Colchester, Vermont 05439 (United States); Decker, J.; Peysson, Y.; Duthoit, F.-X. [CEA, IRFM, Saint-Paul-lez-Durance F-13108 (France)

    2009-10-15

    A general orbit-averaged guiding-center Fokker-Planck operator suitable for the numerical analysis of transport processes in axisymmetric magnetized plasmas is presented. The orbit-averaged guiding-center operator describes transport processes in a three-dimensional guiding-center invariant space: the orbit-averaged magnetic-flux invariant {psi}, the minimum-B pitch-angle coordinate {xi}{sub 0}, and the momentum magnitude p.

  12. SETI at Planck Energy: When Particle Physicists Become Cosmic Engineers

    E-Print Network [OSTI]

    Lacki, Brian C

    2015-01-01

    What is the meaning of the Fermi Paradox -- are we alone or is starfaring rare? Can general relativity be united with quantum mechanics? The searches for answers to these questions could intersect. It is known that an accelerator capable of energizing particles to the Planck scale requires cosmic proportions. The energy required to run a Planck accelerator is also cosmic, of order 100 M_sun c^2 for a hadron collider, because the natural cross section for Planck physics is so tiny. If aliens are interested in fundamental physics, they could resort to cosmic engineering for their experiments. These colliders are detectable through the vast amount of "pollution" they produce, motivating a YeV SETI program. I investigate what kinds of radiation they would emit in a fireball scenario, and the feasibility of detecting YeV radiation at Earth, particularly YeV neutrinos. Although current limits on YeV neutrinos are weak, Kardashev 3 YeV neutrino sources appear to be at least 30--100 Mpc apart on average, if they are ...

  13. max walltime for "low" queue is increased to 24 hrs on Hopper

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    max walltime for low queue is increased to 24 hrs on Hopper max walltime for low queue is increased to 24 hrs on Hopper May 31, 2012 by Helen He (0 Comments) We have increased the...

  14. WPPI GreenMax-Scheller Residence: Near Zero Energy Monitoring Summary

    SciTech Connect (OSTI)

    2010-11-19

    This report describes results of GreenMax 2 monitoring project referred to as the GreenMax Net Zero Home, a demonstration home that can provide a wealth of information for the building community.

  15. Sugar++: A SAT-Based MAX-CSP/COP Solver Tomoya Tanjo1

    E-Print Network [OSTI]

    Banbara, Mutsunori

    Sugar++: A SAT-Based MAX-CSP/COP Solver Tomoya Tanjo1 , Naoyuki Tamura2 , and Mutsunori Banbara2 1 describes some features of Sugar++, a SAT-based MAX- CSP/COP solver entering the Third International CSP Solver Competition. In our approach, a MAX-CSP is translated into a Constraint Optimization Problem (COP

  16. Financial Institutions

    Broader source: Energy.gov [DOE]

    A lending program begins with a financial institution that procures the funds they lend from a number of other sources.

  17. SETI at Planck Energy: When Particle Physicists Become Cosmic Engineers

    E-Print Network [OSTI]

    Brian C. Lacki

    2015-03-05

    What is the meaning of the Fermi Paradox -- are we alone or is starfaring rare? Can general relativity be united with quantum mechanics? The searches for answers to these questions could intersect. It is known that an accelerator capable of energizing particles to the Planck scale requires cosmic proportions. The energy required to run a Planck accelerator is also cosmic, of order 100 M_sun c^2 for a hadron collider, because the natural cross section for Planck physics is so tiny. If aliens are interested in fundamental physics, they could resort to cosmic engineering for their experiments. These colliders are detectable through the vast amount of "pollution" they produce, motivating a YeV SETI program. I investigate what kinds of radiation they would emit in a fireball scenario, and the feasibility of detecting YeV radiation at Earth, particularly YeV neutrinos. Although current limits on YeV neutrinos are weak, Kardashev 3 YeV neutrino sources appear to be at least 30--100 Mpc apart on average, if they are long-lived and emit isotropically. I consider the feasibility of much larger YeV neutrino detectors, including an acoustic detection experiment that spans all of Earth's oceans, and instrumenting the entire Kuiper Belt. Any detection of YeV neutrinos implies an extraordinary phenomenon at work, whether artificial and natural. Searches for YeV neutrinos from any source are naturally commensal, so a YeV neutrino SETI program has value beyond SETI itself, particularly in limiting topological defects. I note that the Universe is very faint in all kinds of nonthermal radiation, indicating that cosmic engineering is extremely rare.

  18. 42 MaxPlanckForschung 4 | 13 Turbulence is omnipresent: it plays an important role during planet formation, mixes fuel and air

    E-Print Network [OSTI]

    Falge, Eva

    formation, mixes fuel and air in the cylinder of an engine, but also increases the energy needed for pumps vortices also stir in the weather factory of our atmosphere. "Fluid turbulence is probably the most efficient without the thorough turbu- lent mixing of the injected fuel. And when we stir milk into our

  19. The observational status of Galileon gravity after Planck

    SciTech Connect (OSTI)

    Barreira, Alexandre; Li, Baojiu; Baugh, Carlton M.; Pascoli, Silvia E-mail: baojiu.li@durham.ac.uk E-mail: silvia.pascoli@durham.ac.uk

    2014-08-01

    We use the latest CMB data from Planck, together with BAO measurements, to constrain the full parameter space of Galileon gravity. We constrain separately the three main branches of the theory known as the Cubic, Quartic and Quintic models, and find that all yield a very good fit to these data. Unlike in ?CDM, the Galileon model constraints are compatible with local determinations of the Hubble parameter and predict nonzero neutrino masses at over 5? significance. We also identify that the low l part of the CMB lensing spectrum may be able to distinguish between ?CDM and Galileon models. In the Cubic model, the lensing potential deepens at late times on sub-horizon scales, which is at odds with the current observational suggestion of a positive ISW effect. Compared to ?CDM, the Quartic and Quintic models predict less ISW power in the low l region of the CMB temperature spectrum, and as such are slightly preferred by the Planck data. We illustrate that residual local modifications to gravity in the Quartic and Quintic models may render the Cubic model as the only branch of Galileon gravity that passes Solar System tests.

  20. Joint Planck and WMAP Assessment of Low CMB Multipoles

    E-Print Network [OSTI]

    Iqbal, Asif; Souradeep, Tarun; Malik, Manzoor A

    2015-01-01

    The remarkable progress in cosmic microwave background (CMB) studies over past decade has led to the era of precision cosmology in striking agreement with the $\\Lambda$CDM model. However, the lack of power in the CMB temperature anisotropies at large angular scales (low-$\\ell$), as has been confirmed by the recent Planck data also (up to $\\ell=40$), is still an open problem. One can avoid to seek an explanation for this problem by attributing the lack of power to cosmic variance or can look for explanations i.e., different inflationary potentials or initial conditions for inflation to begin with, non-trivial topology, ISW effect etc. Features in the primordial power spectrum (PPS) motivated by the early universe physics has been the most common solution to address this problem. In the present work we also follow this approach and consider a set of PPS which have features and constrain the parameters of those using WMAP 9 year and Planck data employing Markov-Chain Monte Carlo (MCMC) analysis. The prominent fe...

  1. DBI Galileon inflation in the light of Planck 2015

    E-Print Network [OSTI]

    K. Sravan Kumar; Celia Escamilla-Rivera; Juan C. Bueno Sanchez; Paulo Vargas Moniz; Joao Marto

    2015-07-14

    In this work we consider a DBI Galileon (DBIG) inflationary model and constrain its parameter space with the Planck 2015 and BICEP2/Keck array and Planck (BKP) joint analysis data by means of a potential independent analysis. We focus our attention on inflationary solutions characterized by a constant or varying sound speed as well as warp factor. We impose bounds on stringy aspects of the model, such as the warp factor $\\left(f\\right)$ and the induced gravity parameter $\\left(\\tilde{m}\\right)$. We find that inflation happens at the GUT scale with $r=\\mathcal{O}\\left(10^{-3}\\right)$. In addition, we obtain the tilt of the tensor power spectrum and test the standard inflationary consistency relation $\\left(r\\simeq-8n_{t}\\right)$ against the latest bounds from the combined results of BKP+Laser Interferometer Gravitational-Waves Observatory (LIGO), and find that DBIG inflation predicts a red spectral index for the tensor power spectrum.

  2. Planck and the local Universe: quantifying the tension

    E-Print Network [OSTI]

    Licia Verde; Pavlos Protopapas; Raul Jimenez

    2013-06-28

    We use the latest Planck constraints, and in particular constraints on the derived parameters (Hubble constant and age of the Universe) for the local universe and compare them with local measurements of the same quantities. We propose a way to quantify whether cosmological parameters constraints from two different experiments are in tension or not. Our statistic, T, is an evidence ratio and therefore can be interpreted with the widely used Jeffrey's scale. We find that in the framework of the LCDM model, the Planck inferred two dimensional, joint, posterior distribution for the Hubble constant and age of the Universe is in "strong" tension with the local measurements; the odds being ~ 1:50. We explore several possibilities for explaining this tension and examine the consequences both in terms of unknown errors and deviations from the LCDM model. In some one-parameter LCDM model extensions, tension is reduced whereas in other extensions, tension is instead increased. In particular, small total neutrino masses are favored and a total neutrino mass above 0.15 eV makes the tension "highly significant" (odds ~ 1:150). A consequence of accepting this interpretation of the tension is that the degenerate neutrino hierarchy is highly disfavoured by cosmological data and the direct hierarchy is slightly favored over the inverse.

  3. Nonlinear transforms of momenta and Planck scale limit

    E-Print Network [OSTI]

    A. Chakrabarti

    2003-01-13

    Starting with the generators of the Poincar\\'e group for arbitrary mass (m) and spin (s) a nonunitary transformation is implemented to obtain momenta with an absolute Planck scale limit. In the rest frame (for $m>0$) the transformed energy coincides with the standard one, both being $m$. As the latter tends to infinity under Lorentz transformations the former tends to a finite upper limit $m\\coth(lm) = l^{-1}+ O(l)$ where $l$ is the Planck length and the mass-dependent nonleading terms vanish exactly for zero rest mass.The invariant $m^{2}$ is conserved for the transformed momenta. The speed of light continues to be the absolute scale for velocities. We study various aspects of the kinematics in which two absolute scales have been introduced in this specific fashion. Precession of polarization and transformed position operators are among them. A deformation of the Poincar\\'e algebra to the SO(4,1) deSitter one permits the implementation of our transformation in the latter case. A supersymmetric extension of the Poincar\\'e algebra is also studied in this context.

  4. A Natural Mass Unit Hidden in the Planck Action Quantum Bernd Binder

    E-Print Network [OSTI]

    Binder, Bernd

    A Natural Mass Unit Hidden in the Planck Action Quantum Bernd Binder binder@quanics.com c 2003 baryon mass a natural mass unit µ can be identified by extrapolating dimensionless Planck units h = c = 1 to the System of Units (SI). Similar to quantum measurements that determine h it is only necessary to relate

  5. A Natural Mass Unit Hidden in the Planck Action Quantum Bernd Binder

    E-Print Network [OSTI]

    Binder, Bernd

    A Natural Mass Unit Hidden in the Planck Action Quantum Bernd Binder binder@quanics.com c #2003 baryon mass a natural mass unit µ can be identified by extrapolating dimensionless Planck units h = c = 1 to the System of Units (SI). Similar to quantum measurements that determine h it is only necessary to relate

  6. Transient finite element analysis of electric double layer using Nernst-Planck-Poisson equations with a modified stern layer 

    E-Print Network [OSTI]

    Lim, Jong Il

    2007-04-25

    Finite element analysis of electric double layer capacitors using a transient nonlinear Nernst-Planck-Poisson (NPP) model and Nernst-Planck-Poisson-modified Stern layer (NPPMS) model are presented in 1D and 2D. The NPP ...

  7. Property:Incentive/MaxInc | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 Jump to: navigation, searchContDiv Jump to:FundSrc Jump to:MaxInc Jump to:

  8. Property:Incentive/PVPbiFitMaxKW | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 Jump to: navigation, searchContDiv Jump to:FundSrc JumpPVPbiFitMaxKW Jump

  9. MaxWest Environmental Systems | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource HistoryScenariosMarysville Mt GeothermalMauna Loa Northeast RiftMaxWest

  10. The Influence of Motion System Characteristics on Pilot Control Behaviour

    E-Print Network [OSTI]

    Planck Institute for Biological Cybernetics, T¨ubingen, Germany Delft University of Technology, Delft, The Netherlands M. Mulder, M. M. van Paassen, Delft University of Technology, Delft, The Netherlands and H. H. B¨ulthoff§ Max Planck Institute for Biological Cybernetics, T¨ubingen, Germany Department of Brain and Cognitive

  11. Combining Real-Time Brain-Computer Interfacing and Robot Control for Stroke Rehabilitation

    E-Print Network [OSTI]

    Planck Institute for Biological Cybernetics, 2 Stanford University, 3 Wadsworth Center, 4 Werner at the Max Planck Institute for Biologi- cal Cybernetics and the University of T¨ubingen, and discuss there is no empirical evidence for a positive impact of BCI-technology on functional recovery. One reason for this may

  12. Cluster at the Bow Shock: Introduction A. Balogh1, S. J. Schwartz2 3, S. D. Bale4, M. A. Balikhin5,

    E-Print Network [OSTI]

    California at Berkeley, University of

    , University of New Hampshire, Durham, New Hampshire, USA 8CETP/IPSL, Velizy, France 9Also Department of Physics, University of New Hampshire, Durham, New Hampshire, USA 10Max-Planck-Institut f

  13. 10 optolines No. 2 | 2. Quartal 2004 MPI fr biophysikalische Chemie, Gttingen

    E-Print Network [OSTI]

    Hell, Stefan W.

    10 optolines No. 2 | 2. Quartal 2004 STARTUP MPI für biophysikalische Chemie, Göttingen Lichtblicke Direktor am Max-Planck-Institut für biophysikalische Chemie und Leiter der Abteilung ,,NanoBio- photonik

  14. Bayesian Experimental Design of Magnetic Resonance Imaging Sequences

    E-Print Network [OSTI]

    Seeger, Matthias

    Nickisch, Rolf Pohmann and Bernhard Sch¨olkopf Max Planck Institute for Biological Cybernetics research of the brain. Without applying any harmful ioniz- ing radiation, this technique stands out by its

  15. INFRARED PROPERTIES OF SOLID TITANIUM OXIDES: EXPLORING POTENTIAL PRIMARY DUST CONDENSATES

    E-Print Network [OSTI]

    Kerschbaum, Franz

    , Hardenbergstrae 36, D-10623 Berlin, Germany and Th. Henning Max-Planck-Institut fu¨r Astronomie (MPIA), Ko et al. (Jeong, Winters, & Sedlmayr 1999; Jeong et al. 2003) predicted TiO2 to be the most promising

  16. Sub-coloring and Hypo-coloring Interval Graphs Rajiv Gandhi1, Bradford Greening, Jr.1, Sriram Pemmaraju2, and Rajiv Raman3

    E-Print Network [OSTI]

    Gandhi, Rajiv C.

    Sub-coloring and Hypo-coloring Interval Graphs Rajiv Gandhi1, Bradford Greening, Jr.1, Sriram, Iowa 52242. E-mail: sriram@cs.uiowa.edu. 3 Max-Planck Institute for Informatik, Saarbr¨ucken, Germany

  17. ISSN 0021-3640, JETP Letters, 2006, Vol. 84, No. 12, pp. 650655. Pleiades Publishing, Inc., 2006. 1. The diverse physical properties of the cobaltate

    E-Print Network [OSTI]

    Eremin, Ilya

    , Ural Division, Russian Academy of Sciences, Yekaterinburg GSP-170, 620041 Russia Received October 30 Division, Russian Academy of Sciences, Krasnoyarsk, 660036 Russia b Max-Planck-Institut für Physik

  18. ISSN 0021-3640, JETP Letters, 2006, Vol. 84, No. 12, pp. 650655. Pleiades Publishing, Inc., 2006. 1. The diverse physical properties of the cobaltate

    E-Print Network [OSTI]

    Eremin, Ilya

    , Ural Division. Russian Academy of Sciences, Yekaterinburg GSP-170, 620041 Russia Received October 30 Division, Russian Academy of Sciences, Krasnoyarsk, 660036 Russia b Max-Planck-Institut für Physik

  19. Influence of Motion Cueing on Helicopter Stabilization

    E-Print Network [OSTI]

    Influence of Motion Cueing on Helicopter Stabilization Daniel R. Berger, Cengiz Terzibas, and Heinrich H. Bülthoff Max Planck Institute for Biological Cybernetics, Tübingen, Germany Helicopters vestibular and somatosensory cues. To test this hypothesis, we measured helicopter hovering performance

  20. experiment, collaboration

    E-Print Network [OSTI]

    Complutense, E-28040Madrid, Spain Max-Planck-Institut fuer Physik, D-80805Muenchen CIEMAT Almeria, Sierra Nevada, southern spain, 505 m a.s.l. " Spanish CIEMAT research centre for solar energy

  1. From corrosion to batteries: Electrochemical interface studies...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    From corrosion to batteries: Electrochemical interface studies Thursday, October 18, 2012 - 11:00am SSRL, Bldg. 137, Rm 226 Dr. Frank Uwe Renner Max-Planck-Institut fr...

  2. Cognitive Engineering Group Contact group leader: Cristobal.Curio@tuebingen.mpg.de

    E-Print Network [OSTI]

    Cognitive Engineering Group Contact group leader: Cristobal.Curio@tuebingen.mpg.de Research Max Planck Institute for Biological Cybernetics Goal: To develop reliable, non-intrusive, Human paper awards In the Cognitive Engineering group computer scientists, psychologists, mathematicians

  3. Engineering and Probing Topological Bloch Bands in Optical Lattices

    E-Print Network [OSTI]

    Dalibard, Jean

    Braun, Philipp Ronzheimer, Michael Schreiber,Tim Rom, Sean Hodgman Ulrich Schneider, Monika Schleier Buchheim, Zhenkai Lu Max-Planck-Institut für Quantenoptik Ludwig-Maximilians Universität funding by MPG

  4. List of Registrants Fermi National Accelerator Laboratory -Batavia, Illinois -USA

    E-Print Network [OSTI]

    Fermilab Experiment E831

    Andricek lca@hll.mpg.deMax-Planck Institut für Physik, Halbleiterlabor7. Steven Aplin aplin. Stewart Boogert stewart.boogert@rhul.ac.ukRoyal Holloway f 37. Tim Botlon tbolton@ksu.eduKansas State

  5. Biogeosciences, 6, 113127, 2009 www.biogeosciences.net/6/113/2009/

    E-Print Network [OSTI]

    ) and surface energy budget parametrizations, and the explicit resolution of local to re- gional wind 6Max Planck Institute for Biogeochemistry, Hans-Knoell-Str. 10, 07745 Jena, Germany 7INRA, B. P. 81

  6. Next-Generation Genetics in Plants: Evolutionary Trade-off, Immunity and Speciation (2010 JGI User Meeting)

    ScienceCinema (OSTI)

    Wiegel, Detlef

    2011-04-25

    Detlef Wiegel from the Max Planck Institute for Developmental Biology on "Next-generation genetics in plants: Evolutionary tradeoffs, immunity and speciation" on March 25, 2010 at the 5th Annual DOE JGI User Meeting

  7. On the Einstein-Cartan cosmology vs. Planck data

    E-Print Network [OSTI]

    Palle, Davor

    2014-01-01

    The first comprehensive analyses of Planck data reveal that the cosmological model with dark energy and cold dark matter can satisfactorily explain the essential physical features of the expanding Universe. However, the inability to simultaneously fit large and small scale TT power spectrum, scalar power index smaller than one and the observations of the violation of the isotropy found by few statistical indicators of the CMB, urge theorists to search for explanations. We show that the model of the Einstein-Cartan cosmology with clustered dark matter halos and their corresponding clustered angular momenta coupled to torsion, can account for small scale - large scale discrepancy and larger peculiar velocities (bulk flows) for galaxy clusters. The nonvanishing total angular momentum (torsion) of the Universe enters as a negative effective density term in the Einstein-Cartan equations causing partial cancellation of the mass density. The integrated Sachs-Wolfe contribution of the Einstein-Cartan model is negativ...

  8. Primordial non-Gaussianities after Planck 2015: an introductory review

    E-Print Network [OSTI]

    Sébastien Renaux-Petel

    2015-08-27

    Deviations from Gaussian statistics of the cosmological density fluctuations, so-called primordial non-Gaussianities (NG), are one of the most informative fingerprints of the origin of structures in the universe. Indeed, they can probe physics at energy scales inaccessible to laboratory experiments, and are sensitive to the interactions of the field(s) that generated the primordial fluctuations, contrary to the Gaussian linear theory. As a result, they can discriminate between inflationary models that are otherwise almost indistinguishable. In this short review, we explain how to compute the non-Gaussian properties in any inflationary scenario. We review the theoretical predictions of several important classes of models. We then describe the ways NG can be probed observationally, and we highlight the recent constraints from the Planck mission, as well as their implications. We finally identify well motivated theoretical targets for future experiments and discuss observational prospects.

  9. Primordial non-Gaussianities after Planck 2015: an introductory review

    E-Print Network [OSTI]

    Renaux-Petel, Sébastien

    2015-01-01

    Deviations from Gaussian statistics of the cosmological density fluctuations, so-called primordial non-Gaussianities (NG), are one of the most informative fingerprints of the origin of structures in the universe. Indeed, they can probe physics at energy scales inaccessible to laboratory experiments, and are sensitive to the interactions of the field(s) that generated the primordial fluctuations, contrary to the Gaussian linear theory. As a result, they can discriminate between inflationary models that are otherwise almost indistinguishable. In this short review, we explain how to compute the non-Gaussian properties in any inflationary scenario. We review the theoretical predictions of several important classes of models. We then describe the ways NG can be probed observationally, and we highlight the recent constraints from the Planck mission, as well as their implications. We finally identify well motivated theoretical targets for future experiments and discuss observational prospects.

  10. Planck 2015 results. XII. Full Focal Plane simulations

    E-Print Network [OSTI]

    Ade, P A R; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartlett, J G; Bartolo, N; Battaner, E; Benabed, K; Beno\\^\\it, A; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bock, J J; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Castex, G; Catalano, A; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Clements, D L; Colombi, S; Colombo, L P L; Combet, C; Couchot, F; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Désert, F -X; Dickinson, C; Diego, J M; Dolag, K; Dole, H; Donzelli, S; Doré, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Giraud-Héraud, Y; Gjerløw, E; González-Nuevo, J; Górski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versillé, S; Hernández-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Karakci, A; Keihänen, E; Keskitalo, R; Kiiveri, K; Kisner, T S; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vørnle, M; Lindholm, V; López-Caniego, M; Lubin, P M; Mac\\'\\ias-Pérez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, P G; Mart\\'\\inez-González, E; Masi, S; Matarrese, S; McGehee, P; Meinhold, P R; Melchiorri, A; Melin, J -B; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschênes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nørgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Pratt, G W; Prézeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Roman, M; Rosset, C; Rossetti, M; Roudier, G; Rubiño-Martín, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; Welikala, N; Yvon, D; Zacchei, A; Zonca, A

    2015-01-01

    We present the 8th Full Focal Plane simulation set (FFP8), deployed in support of the Planck 2015 results. FFP8 consists of 10 fiducial mission realizations reduced to 18144 maps, together with the most massive suite of Monte Carlo realizations of instrument noise and CMB ever generated, comprising $10^4$ mission realizations reduced to about $10^6$ maps. The resulting maps incorporate the dominant instrumental, scanning, and data analysis effects; remaining subdominant effects will be included in future updates. Generated at a cost of some 25 million CPU-hours spread across multiple high-performance-computing (HPC) platforms, FFP8 is used for the validation and verification of analysis algorithms, as well as their implementations, and for removing biases from and quantifying uncertainties in the results of analyses of the real data.

  11. Strong Planck constraints on braneworld and non-commutative inflation

    SciTech Connect (OSTI)

    Calcagni, Gianluca [Instituto de Estructura de la Materia, CSIC, Serrano 121, 28006 Madrid (Spain); Kuroyanagi, Sachiko; Ohashi, Junko; Tsujikawa, Shinji, E-mail: calcagni@iem.cfmac.csic.es, E-mail: skuro@rs.tus.ac.jp, E-mail: j1211703@ed.tus.ac.jp, E-mail: shinji@rs.kagu.tus.ac.jp [Department of Physics, Faculty of Science, Tokyo University of Science, 1-3, Kagurazaka, Shinjuku-ku, Tokyo 162-8601 (Japan)

    2014-03-01

    We place observational likelihood constraints on braneworld and non-commutative inflation for a number of inflaton potentials, using Planck, WMAP polarization and BAO data. Both braneworld and non-commutative scenarios of the kind considered here are limited by the most recent data even more severely than standard general-relativity models. At more than 95 % confidence level, the monomial potential V(?)??{sup p} is ruled out for p ? 2 in the Randall-Sundrum (RS) braneworld cosmology and, for p > 0, also in the high-curvature limit of the Gauss-Bonnet (GB) braneworld and in the infrared limit of non-commutative inflation, due to a large scalar spectral index. Some parameter values for natural inflation, small-varying inflaton models and Starobinsky inflation are allowed in all scenarios, although some tuning is required for natural inflation in a non-commutative spacetime.

  12. Standard big bang nucleosynthesis and primordial CNO abundances after Planck

    SciTech Connect (OSTI)

    Coc, Alain [Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), CNRS/IN2P3, Université Paris Sud 11, UMR 8609, Bâtiment 104, F–91405 Orsay Campus (France); Uzan, Jean-Philippe; Vangioni, Elisabeth, E-mail: coc@csnsm.in2p3.fr, E-mail: uzan@iap.fr, E-mail: vangioni@iap.fr [Institut d'Astrophysique de Paris, UMR-7095 du CNRS, Université Pierre et Marie Curie, 98 bis bd Arago, 75014 Paris (France)

    2014-10-01

    Primordial or big bang nucleosynthesis (BBN) is one of the three historical strong evidences for the big bang model. The recent results by the Planck satellite mission have slightly changed the estimate of the baryonic density compared to the previous WMAP analysis. This article updates the BBN predictions for the light elements using the cosmological parameters determined by Planck, as well as an improvement of the nuclear network and new spectroscopic observations. There is a slight lowering of the primordial Li/H abundance, however, this lithium value still remains typically 3 times larger than its observed spectroscopic abundance in halo stars of the Galaxy. According to the importance of this ''lithium problem{sup ,} we trace the small changes in its BBN calculated abundance following updates of the baryonic density, neutron lifetime and networks. In addition, for the first time, we provide confidence limits for the production of {sup 6}Li, {sup 9}Be, {sup 11}B and CNO, resulting from our extensive Monte Carlo calculation with our extended network. A specific focus is cast on CNO primordial production. Considering uncertainties on the nuclear rates around the CNO formation, we obtain CNO/H ? (5-30)×10{sup -15}. We further improve this estimate by analyzing correlations between yields and reaction rates and identified new influential reaction rates. These uncertain rates, if simultaneously varied could lead to a significant increase of CNO production: CNO/H?10{sup -13}. This result is important for the study of population III star formation during the dark ages.

  13. Inflationary Magnetogenesis in $R^{2}$-Inflation after Planck 2015

    E-Print Network [OSTI]

    Anwar Saleh AlMuhammad

    2015-05-19

    We study the primordial magnetic field generated by the simple model $f^2 FF$ in Starobinsky, $R^2$-inflationary, model. The scale invariant PMF is achieved at relatively high power index of the coupling function, $\\left| \\alpha \\right| \\approx 7.44$. This model does not suffer from the backreaction problem as long as, the rate of inflationary expansion, $H$, is in the order of or less than the upper bound reported by Planck ($\\le 3.6 \\times 10^{-5} M_\\rm{Pl}$) in both de Sitter and power law expansion, which show similar results. We calculate the lower limit of the reheating parameter, $R_\\rm{rad} > 6.888$ in $R^2$-inflation. Based on the upper limit obtained from CMB, we find that the upper limits of magnetic field and reheating energy density as, $\\left(\\rho_{B_\\rm{end}} \\right)_\\rm{CMB} right)_\\rm{CMB} energy density for all possible values of $w _\\rm{reh}$ are respectively constrained as, $T_\\rm{reh} < 4.32 \\times 10^{13} \\rm{GeV}$ and $\\rho_\\rm{reh} < 3.259 \\times 10^{-18} M_\\rm{Pl}^4$ at $n_\\rm{s} \\approx 0.9674$. This value of spectral index is well consistent with Planck, 2015 results. Adopting $T_\\rm{reh}$, enables us to constrain the reheating e-folds number, $N_\\rm{reh}$ on the range $1 < N_\\rm{reh} < 8.3$, for $- 1/3 < w_\\rm{reh} < 1$. By using the scale invariant PMF generated by $f^2 FF$, we find that the upper limit of present magnetic field, $B_0 < 8.058 \\times 10^{-9} \\rm{G}$.

  14. Vor 100 Jahren ffnete in Berlin-Dahlem das Kaiser-Wilhelm-Institut fr Chemie seine Pforten. Schon drei Jahre spter konnte es mit dem ersten Nobelpreistrger aufwarten: Richard Willsttter

    E-Print Network [OSTI]

    Falge, Eva

    Vor 100 Jahren öffnete in Berlin-Dahlem das Kaiser-Wilhelm-Institut für Chemie seine Pforten. Schon-Planck-Institut für Chemie in Mainz hervorging, durch die Entdeckung der Kernspaltung. TEXT ELKE MAIER Ein Ort Politik versammelt. Man erwartete hohen Besuch: Der Kaiser persönlich sollte das Institut für Chemie

  15. The use and misuse of Vc,max in Earth System Models Alistair Rogers

    E-Print Network [OSTI]

    Rogers, Alistair

    REVIEW The use and misuse of Vc,max in Earth System Models Alistair Rogers Received: 18 November Dordrecht (outside the USA) 2013 Abstract Earth System Models (ESMs) aim to project global change. Central Á Vc,max Á Leaf nitrogen Á Earth System Models Introduction The primary goal of Earth System Models

  16. Andreas Sundelf, Valerio Bartolino, Max Cardinale Aqua reports 2013:15

    E-Print Network [OSTI]

    Andreas Sundelöf, Valerio Bartolino, Max Cardinale Aqua reports 2013:15 Waking the Deads Final report #12;Waking the Deads Final report Andreas Sundelöf, Valerio Bartolino, Max Cardinale Address SLU 2013 SLU, Department of Aquatic Resources Aqua reports 2013:15 ISBN: 978-91-576-9177-4 (elektronisk

  17. Holographic Noise in Michelson Interferometers: A Direct Experimental Probe of Unification at the Planck Scale

    ScienceCinema (OSTI)

    Hogan, Craig

    2010-01-08

    Classical spacetime and quantum mass-energy form the basis of all of physics. They become inconsistent at the Planck scale, 5.4 times 10^{-44} seconds, which may signify a need for reconciliation in a unified theory. Although proposals for unified theories exist, a direct experimental probe of this scale, 16 orders of magnitude above Tevatron energy, has seemed hopelessly out of reach. However in a particular interpretation of holographic unified theories, derived from black hole evaporation physics, a world assembled out of Planck-scale waves displays effects of unification with a new kind of uncertainty in position at the Planck diffraction scale, the geometric mean of the Planck length and the apparatus size. In this case a new phenomenon may measurable, an indeterminacy of spacetime position that appears as noise in interferometers. The colloquium will discuss the theory of the effect, and our plans to build a holographic interferometer at Fermilab to measure it.

  18. On the Einstein-Cartan cosmology vs. Planck data

    E-Print Network [OSTI]

    Davor Palle

    2014-05-14

    The first comprehensive analyses of Planck data reveal that the cosmological model with dark energy and cold dark matter can satisfactorily explain the essential physical features of the expanding Universe. However, the inability to simultaneously fit large and small scale TT power spectrum, scalar power index smaller than one and the observations of the violation of the isotropy found by few statistical indicators of the CMB, urge theorists to search for explanations. We show that the model of the Einstein-Cartan cosmology with clustered dark matter halos and their corresponding clustered angular momenta coupled to torsion, can account for small scale - large scale discrepancy and larger peculiar velocities (bulk flows) for galaxy clusters. The nonvanishing total angular momentum (torsion) of the Universe enters as a negative effective density term in the Einstein-Cartan equations causing partial cancellation of the mass density. The integrated Sachs-Wolfe contribution of the Einstein-Cartan model is negative, thus it can provide partial cancellation of the large scale power of the TT CMB spectrum. The observed violation of the isotropy appears as a natural ingredient of the Einstein-Cartan model caused by the spin densities of light Majorana neutrinos in the early stage of the evolution of the Universe and bound to the lepton CP violation and matter-antimatter asymmetry.

  19. The Effective Planck Mass and the Scale of Inflation

    E-Print Network [OSTI]

    Ignatios Antoniadis; Subodh P. Patil

    2015-04-23

    Observable quantities in cosmology are dimensionless, and therefore independent of the units in which they are measured. This is true of all physical quantities associated with the primordial perturbations that source cosmic microwave background anisotropies such as their amplitude and spectral properties. However, if one were to try and infer an absolute energy scale for inflation-- a priori, one of the more immediate corollaries of detecting primordial tensor modes-- one necessarily makes reference to a particular choice of units, the natural choice for which is Planck units. In this note, we discuss various aspects of how inferring the energy scale of inflation is complicated by the fact that the effective strength of gravity as seen by inflationary quanta necessarily differs from that seen by gravitational experiments at presently accessible scales. The uncertainty in the former relative to the latter has to do with the unknown spectrum of universally coupled particles between laboratory scales and the putative scale of inflation. These intermediate particles could be in hidden as well as visible sectors or could also be associated with Kaluza-Klein resonances associated with a compactification scale below the scale of inflation. We discuss various implications for cosmological observables.

  20. Cellular Networks as Models for Planck-Scale Physics

    E-Print Network [OSTI]

    Manfred Requardt

    1998-06-17

    Starting from the working hypothesis that both physics and the corresponding mathematics have to be described by means of discrete concepts on the Planck scale, one of the many problems one has to face in this enterprise is to find the discrete protoforms of the building blocks of our ordinary continuum physics and mathematics. We base our own approach on what we call `cellular networks', consisting of cells (nodes) interacting with each other via bonds (figuring as elementary interactions) according to a certain `local law'. Geometrically our dynamical networks are living on graphs. Hence a substantial amount of the investigation is devoted to the developement of various versions of discrete (functional) analysis and geometry on such (almost random) webs. Another important topic we address is a suitable concept of intrinsic (fractal) dimension on erratic structures of this kind. In the course of the investigation we make comments concerning both different and related approaches to quantum gravity as, say, the spin network framework. It may perhaps be said that certain parts of our programme seem to be a realisation of ideas sketched by Smolin some time ago (see the introduction).

  1. Planck Early Results: The High Frequency Instrument data processing

    E-Print Network [OSTI]

    Ade, P A R; Ansari, R; Arnaud, M; Ashdown, M; Aumont, J; Banday, A J; Bartelmann, M; Bartlett, J G; Battaner, E; Benabed, K; Benoît, A; Bernard, J -P; Bersanelli, M; Bock, J J; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bradshaw, T; Bucher, M; Cardoso, J -F; Castex, G; Catalano, A; Challinor, A; Chamballu, A; Chary, R -R; Chen, X; Chiang, C; Church, S; Clements, D L; Colley, J -M; Colombi, S; Couchot, F; Coulais, A; Cressiot, C; Crill, B P; Crook, M; de Bernardis, P; Delabrouille, J; Delouis, J -M; Désert, F -X; Dolag, K; Dole, H; Doré, O; Douspis, M; Dunkley, J; Efstathiou, G; Filliard, C; Forni, O; Fosalba, P; Ganga, K; Giard, M; Girard, D; Giraud-Héraud, Y; Gispert, R; Górski, K M; Gratton, S; Griffin, M; Guyot, G; Haissinski, J; Harrison, D; Helou, G; Henrot-Versillé, S; Hernández-Monteagudo, C; Hildebrandt, S R; Hills, R; Hivon, E; Hobson, M; Holmes, W A; Huffenberger, K M; Jaffe, A H; Jones, W C; Kaplan, J; Kneissl, R; Knox, L; Kunz, M; Lagache, G; Lamarre, J -M; Lange, A E; Lasenby, A; Lavabre, A; Lawrence, C R; Jeune, M Le; Leroy, C; Lesgourgues, J; Lewis, A; Macías-Pérez, J F; MacTavish, C J; Maffei, B; Mandolesi, N; Mann, R; Marleau, F; Marshall, D J; Masi, S; Matsumura, T; McAuley, I; McGehee, P; Melin, J -B; Mercier, C; Mitra, S; Miville-Deschênes, M -A; Moneti, A; Montier, L; Mortlock, D; Murphy, A; Nati, F; Netterfield, C B; N\\orgaard-Nielsen, H U; North, C; Noviello, F; Novikov, D; Osborne, S; Pajot, F; Patanchon, G; Peacocke, T; Pearson, T J; Perdereau, O; Perotto, L; Piacentini, F; Piat, M; Plaszczynski, S; Pointecouteau, E; Ponthieu, N; Prézeau, G; Prunet, S; Puget, J -L; Reach, W T; Remazeilles, M; Renault, C; Riazuelo, A; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rowan-Robinson, M; Rusholme, B; Saha, R; Santos, D; Savini, G; Schaefer, B M; Shellard, P; Spencer, L; Starck, J -L; Stolyarov, V; Stompor, R; Sudiwala, R; Sunyaev, R; Sutton, D; Sygnet, J -F; Tauber, J A; Thum, C; Torre, J -P; Touze, F; Tristram, M; Van Leeuwen, F; Vibert, L; Vibert, D; Wandelt, B D; White, S D M; Wiesemeyer, H; Woodcraft, A; Yurchenko, V; Yvon, D; Zacchei, A

    2011-01-01

    We describe the processing of the 334 billion raw data samples from the High Frequency Instrument (hereafter HFI) which we performed to produce six temperature maps from the first 295 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143, 217, 353, 545 and 857GHz with an angular resolution ranging from 9.9 to 4.4 arcmin. The white noise level is around 1.5 microK.degree or less in the 3 main CMB channels (100-217GHz). The photometric accuracy is better than 2% at frequencies lower or equal to 353GHz, and around 7% at the two highest frequencies. The maps created by the HFI Data Processing Centre reach our goals in terms of sensitivity, resolution, and photometric accuracy. They are already sufficiently accurate and well-characterised to allow scientific analyses which are presented in an accompanying series of early papers. At this stage, HFI data appears to be of high quality and we expect that with further refinements of the data processing we should be abl...

  2. Negative running of the spectral index, hemispherical asymmetry and the consistency of Planck with large r

    SciTech Connect (OSTI)

    McDonald, John

    2014-11-01

    Planck favours a negative running of the spectral index, with the likelihood being dominated by low multipoles l ?< 50 and no preference for running at higher l. A negative spectral index is also necessary for the 2- Planck upper bound on the tensor-to-scalar ratio r to be consistent with values significantly larger than 0.1. Planck has also observed a hemispherical asymmetry of the CMB power spectrum, again mostly at low multipoles. Here we consider whether the physics responsible for the hemispherical asymmetry could also account for the negative running of the spectral index and the consistency of Planck with a large value of r. A negative running of the spectral index can be generated if the hemispherical asymmetry is due to a scale- and space-dependent modulation which suppresses the CMB power spectrum at low multipoles. We show that the observed hemispherical asymmetry at low l can be generated while satisfying constraints on the asymmetry at higher l and generating a negative spectral index of the right magnitude to account for the Planck observation and to allow Planck to be consistent with a large value of r.

  3. A Connectionist model of Planning via Back-chaining Search Max Garagnani

    E-Print Network [OSTI]

    Shastri, Lokendra

    A Connectionist model of Planning via Back-chaining Search Max Garagnani Department of Computing+1 World state ObservableEpisodic Memory ECALL Figure 1: A block diagram showing the basic compo

  4. Max-Min characterization of the mountain pass energy level for a class of variational problems

    E-Print Network [OSTI]

    Jacopo Bellazzini; Nicola Visciglia

    2009-09-01

    We provide a max-min characterization of the mountain pass energy level for a family of variational problems. As a consequence we deduce the mountain pass structure of solutions to suitable PDEs, whose existence follows from classical minimization argument.

  5. Max Tech Appliance Design: Potential for Maximizing U.S. Energy Savings through Standards

    E-Print Network [OSTI]

    Garbesi, Karina

    2011-01-01

    savings. Annual Reduction in Primary Energy Use for Best-on-Product Annual Reduction in Primary Energy Use for Max Tech30-year Baseline Primary Energy Use (quads) Annual Primary

  6. Max Tech and Beyond: Maximizing Appliance and Equipment Efficiency by Design

    E-Print Network [OSTI]

    Desroches, Louis-Benoit

    2012-01-01

    from moving to best-on- market designs) is realized for thefor most best-on-market products, design information isboth best-on-market and max tech designs (e.g. , best

  7. On the "counter-example" in the article "Max -controlled siphons for liveness of S3

    E-Print Network [OSTI]

    Reveliotis, Spiridon "Spyros"

    On the "counter-example" in the article "Max -controlled siphons for liveness of S3 PGR2 characterization of the S3PGR2 nets by means of the structural object of deadly marked siphon, are correct

  8. The introduction of symmetry constraints within MaxEnt Jaynes's methodology

    E-Print Network [OSTI]

    F. Holik; C. Massri; A. Plastino

    2014-12-31

    We provide a generalization of the approach to geometric probability advanced by the great mathematician Gian Carlo Rota, in order to apply it to generalized probabilistic physical theories. In particular, we use this generalization to provide an improvement of the Jaynes' MaxEnt method. The improvement consists in providing a framework for the introduction of symmetry constrains. This allows us to include group theory within MaxEnt. Some examples are provided.

  9. Advanced Studies Institute

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Engineering Institute Advanced Studies Institute Contact Institute Director Charles Farrar (505) 663-5330 Email UCSD EI Director Michael Todd (858) 534-5951 Professional Staff...

  10. Principal component analysis of the reionization history from Planck 2015 data

    E-Print Network [OSTI]

    Dai, Wei-Ming; Cai, Rong-Gen

    2015-01-01

    The simple assumption of an instantaneous reionization of the Universe may bias estimates of cosmological parameters. In this paper a model-independent principal component method for the reionization history is applied to give constraints on the cosmological parameters from recent Planck 2015 data. We find that the Universe are not completely reionized at redshifts $z \\ge 8.5$ at 95% CL. Both the reionization optical depth and the matter fluctuation amplitude are higher than but consistent with those obtained in the standard instantaneous reionization scheme. The high estimated value of the matter fluctuation amplitude strengthens the tension between Planck CMB observations and some astrophysical data, such as cluster counts and weak lensing. The tension can significantly be relieved if the neutrino masses are allowed to vary. Thanks to a high scalar spectral index, the low-scale spontaneously broken SUSY inflationary model can fit the data well, which is marginally disfavored at 95% CL in the Planck analysis...

  11. Cosmological constant in SUGRA models with Planck scale SUSY breaking and degenerate vacua

    E-Print Network [OSTI]

    C. D. Froggatt; R. Nevzorov; H. B. Nielsen; A. W. Thomas

    2014-10-08

    The empirical mass of the Higgs boson suggests small to vanishing values of the quartic Higgs self--coupling and the corresponding beta function at the Planck scale, leading to degenerate vacua. This leads us to suggest that the measured value of the cosmological constant can originate from supergravity (SUGRA) models with degenerate vacua. This scenario is realised if there are at least three exactly degenerate vacua. In the first vacuum, associated with the physical one, local supersymmetry (SUSY) is broken near the Planck scale while the breakdown of the SU(2)_W\\times U(1)_Y symmetry takes place at the electroweak (EW) scale. In the second vacuum local SUSY breaking is induced by gaugino condensation at a scale which is just slightly lower than \\Lambda_{QCD} in the physical vacuum. Finally, in the third vacuum local SUSY and EW symmetry are broken near the Planck scale.

  12. Possible Evidence for Planck-Scale Resonant Particle Production during Inflation from the CMB Power Spectrum

    E-Print Network [OSTI]

    Mathews, G J; Ichiki, K; Kajino, T

    2015-01-01

    The power spectrum of the cosmic microwave background from both the Planck and WMAP data exhibits a slight dip in for multipoles in the range of l=10-30. We show that such a dip could be the result of resonant creation of a massive particle that couples to the inflaton field. For our best-fit models, epochs of resonant particle creation reenters the horizon at wave numbers of k* ~ 0.00011 (h/Mpc). The amplitude and location of these features correspond to the creation of a number of degenerate fermion species of mass ~ 15 times the planck mass during inflation with a coupling constant between the inflaton field and the created fermion species of near unity. Although the evidence is marginal, if this interpretation is correct, this could be one of the first observational hints of new physics at the Planck scale.

  13. The Wigner-Fokker-Planck equation: Stationary states and large-time behavior

    E-Print Network [OSTI]

    Anton Arnold; Irene M. Gamba; Maria Pia Gualdani; Stephane Mischler; Clement Mouhot; Christof Sparber

    2012-01-20

    We consider the linear Wigner-Fokker-Planck equation subject to confining potentials which are smooth perturbations of the harmonic oscillator potential. For a certain class of perturbations we prove that the equation admits a unique stationary solution in a weighted Sobolev space. A key ingredient of the proof is a new result on the existence of spectral gaps for Fokker-Planck type operators in certain weighted $L^2$-spaces. In addition we show that the steady state corresponds to a positive density matrix operator with unit trace and that the solutions of the time-dependent problem converge towards the steady state with an exponential rate.

  14. THE JOURNAL OF CHEMICAL PHYSICS 135, 084103 (2011) How accurate are the nonlinear chemical Fokker-Planck and chemical

    E-Print Network [OSTI]

    Straube, Arthur V.

    2011-01-01

    THE JOURNAL OF CHEMICAL PHYSICS 135, 084103 (2011) How accurate are the nonlinear chemical Fokker-Planck and chemical Langevin equations? Ramon Grima,1,a) Philipp Thomas,1,2 and Arthur V. Straube2 1 School August 2011) The chemical Fokker-Planck equation and the corresponding chemical Langevin equation are com

  15. Entropy production in irreversible systems described by a Fokker-Planck equation Tnia Tom and Mrio J. de Oliveira

    E-Print Network [OSTI]

    de Oliveira, Mário José

    Entropy production in irreversible systems described by a Fokker-Planck equation Tânia Tomé and the entropy production in nonequilibrium interacting particle systems described by a Fokker-Planck equation for the entropy production is deduced from a general definition, which is related to the probability

  16. FREE ENERGY AND SOLUTIONS OF THE VLASOV-POISSON-FOKKER-PLANCK SYSTEM : EXTERNAL POTENTIAL AND CONFINEMENT

    E-Print Network [OSTI]

    Dolbeault, Jean

    FREE ENERGY AND SOLUTIONS OF THE VLASOV-POISSON-FOKKER-PLANCK SYSTEM : EXTERNAL POTENTIAL-mail: dolbeault@ceremade.dauphine.fr June 20, 1997 Introduction I. The free energy 1. Jensen's inequality and related topics 2. Applications to the free energy 2.1. The linear case 2.2. The self-consistent case 3

  17. North-South non-Gaussian asymmetry in Planck CMB maps

    SciTech Connect (OSTI)

    Bernui, A.; Oliveira, A.F.; Pereira, T.S. E-mail: adhimar@unifei.edu.br

    2014-10-01

    We report the results of a statistical analysis performed with the four foreground-cleaned Planck maps by means of a suitably defined local-variance estimator. Our analysis shows a clear dipolar structure in Planck's variance map pointing in the direction (l,b) ? (220°,-32°), thus consistent with the North-South asymmetry phenomenon. Surprisingly, and contrary to previous findings, removing the CMB quadrupole and octopole makes the asymmetry stronger. Our results show a maximal statistical significance, of 98.1% CL, in the scales ranging from ?=4 to ?=500. Additionally, through exhaustive analyses of the four foreground-cleaned and individual frequency Planck maps, we find unlikely that residual foregrounds could be causing this dipole variance asymmetry. Moreover, we find that the dipole gets lower amplitudes for larger masks, evidencing that most of the contribution to the variance dipole comes from a region near the galactic plane. Finally, our results are robust against different foreground cleaning procedures, different Planck masks, pixelization parameters, and the addition of inhomogeneous real noise.

  18. Green function of the double fractional Fokker-Planck equation: Path integral and stochastic differential equations

    E-Print Network [OSTI]

    H. Kleinert; V. Zatloukal

    2015-03-05

    The statistics of rare events, the so-called black-swan events, is governed by non-Gaussian distributions with heavy power-like tails. We calculate the Green functions of the associated Fokker-Planck equations and solve the related stochastic differential equations. We also discuss the subject in the framework of path integration.

  19. Ground states of 2d J Ising spin glasses via stationary FokkerPlanck sampling

    E-Print Network [OSTI]

    Peinke, Joachim

    of the individual variables that enter the cost function. Moreover, the influence of the cost function on the search disciplines [1, 2]. Among those, stochastic search strategies like e.g. simulated annealing [3, 4], parallel function. Langevin dynamics can also be cast in terms of a Fokker­Planck equation as evolution equation

  20. Aging correlation functions of the interrupted fractional Fokker-Planck propagator

    E-Print Network [OSTI]

    Cao, Jianshu

    Aging correlation functions of the interrupted fractional Fokker-Planck propagator James B The authors explore aging in a general semi-Markov process with arbitrary waiting time distributions coordination, but one can generalize the construction to incorporate cutoffs in the aging of the system, i

  1. Planck CMB anomalies: astrophysical and cosmological secondary effects and the curse of masking

    SciTech Connect (OSTI)

    Rassat, A.; Starck, J.-L.; Paykari, P.; Sureau, F.; Bobin, J. E-mail: jstarck@cea.fr E-mail: florent.sureau@cea.fr

    2014-08-01

    Large-scale anomalies have been reported in CMB data with both WMAP and Planck data. These could be due to foreground residuals and or systematic effects, though their confirmation with Planck data suggests they are not due to a problem in the WMAP or Planck pipelines. If these anomalies are in fact primordial, then understanding their origin is fundamental to either validate the standard model of cosmology or to explore new physics. We investigate three other possible issues: 1) the trade-off between minimising systematics due to foreground contamination (with a conservative mask) and minimising systematics due to masking, 2) astrophysical secondary effects (the kinetic Doppler quadrupole and kinetic Sunyaev-Zel'dovich effect), and 3) secondary cosmological signals (the integrated Sachs-Wolfe effect). We address the masking issue by considering new procedures that use both WMAP and Planck to produce higher quality full-sky maps using the sparsity methodology (LGMCA maps). We show the impact of masking is dominant over that of residual foregrounds, and the LGMCA full-sky maps can be used without further processing to study anomalies. We consider four official Planck PR1 and two LGMCA CMB maps. Analysis of the observed CMB maps shows that only the low quadrupole and quadrupole-octopole alignment seem significant, but that the planar octopole, Axis of Evil, mirror parity and cold spot are not significant in nearly all maps considered. After subtraction of astrophysical and cosmological secondary effects, only the low quadrupole may still be considered anomalous, meaning the significance of only one anomaly is affected by secondary effect subtraction out of six anomalies considered. In the spirit of reproducible research all reconstructed maps and codes will be made available for download here http://www.cosmostat.org/anomaliesCMB.html.

  2. TOKYO INSTITUTE OF TECHNOLOGY

    E-Print Network [OSTI]

    TOKYO INSTITUTE OF TECHNOLOGY 2005 TOKYO INSTITUTE OF TECHNOLOGY 152-8550 2 12 1 E3-3 2005 8 TEL. 03 5734 2975 URL. http://www.titech.ac.jp/ PROFILE #12;TOKYO INSTITUTE OF TECHNOLOGY 0201 CONTENTS 03 06 06 08 09 10 15 17 25 31 33 37 41 0201 #12;TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE

  3. National Institutes of Health Current National Institute

    E-Print Network [OSTI]

    Rau, Don C.

    Library of Medicine John E. Fogarty International Center for Advanced Study in National Center National Institute of Nursing Research National Library of Medicine John E. Fogarty International CenterNational Institutes of Health Current National Institute of Arthritis and Musculoskeletal and Skin

  4. Environmental Change Institute Environmental Change Institute

    E-Print Network [OSTI]

    Oxford, University of

    Environmental Change Institute 2012/13 eci Environmental Change Institute #12;ii Environmental 06 Educating environmental leaders 08 Centre for interdisciplinary doctoral training 10 A thriving, Dumfriesshire (ECI) #12;1 The Environmental Change Institute has 21 years' experience in helping governments

  5. Supplement of Atmos. Chem. Phys., 14, 89058915, 2014 http://www.atmos-chem-phys.net/14/8905/2014/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    considered representative, while periods (hourly data) of off-shore winds observed at Iraklion were rejected in the Environment, Brno, Czech Republic b Helmholtz Research Centre Jülich, Institute for Energy & Climate Research, Jülich, Germany c CNR, Institute for Atmospheric Pollution Research, Rende, Italy d Max Planck Institute

  6. Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

    E-Print Network [OSTI]

    Aghanim, N; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartlett, J G; Bartolo, N; Battaner, E; Benabed, K; Benoît, A; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bock, J J; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Catalano, A; Challinor, A; Chiang, H C; Christensen, P R; Clements, D L; Colombo, L P L; Combet, C; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Désert, F -X; Di Valentino, E; Dickinson, C; Diego, J M; Dolag, K; Dole, H; Donzelli, S; Doré, O; Douspis, M; Ducout, A; Dunkley, J; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Gauthier, C; Gerbino, M; Giard, M; Gjerløw, E; González-Nuevo, J; Górski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Hamann, J; Hansen, F K; Harrison, D L; Helou, G; Henrot-Versillé, S; Hernández-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Holmes, W A; Hornstrup, A; Huffenberger, K M; Hurier, G; Jaffe, A H; Jones, W C; Juvela, M; Keihänen, E; Keskitalo, R; Kiiveri, K; Knoche, J; Knox, L; Kunz, M; Kurki-Suonio, H; Lagache, G; Lähteenmäki, A; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Jeune, M Le; Leonardi, R; Lesgourgues, J; Levrier, F; Lewis, A; Liguori, M; Lilje, P B; Lilley, M; Linden-Vørnle, M; Lindholm, V; López-Caniego, M; Macías-Pérez, J F; Maffei, B; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, P G; Martínez-González, E; Masi, S; Matarrese, S; Meinhold, P R; Melchiorri, A; Migliaccio, M; Millea, M; Miville-Deschênes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J A; Narimani, A; Naselsky, P; Nati, F; Natoli, P; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Partridge, B; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Pratt, G W; Prunet, S; Puget, J -L; Rachen, J P; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rossetti, M; Roudier, G; d'Orfeuil, B Rouillé; Rubiño-Martín, J A; Rusholme, B; Salvati, L; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Serra, P; Spencer, L D; Spinelli, M; Stolyarov, V; Stompor, R; Sunyaev, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Trombetti, T; Tucci, M; Tuovinen, J; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; Yvon, D; Zacchei, A; Zonca, A

    2015-01-01

    This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of CMB temperature and polarization. They use the hybrid approach employed previously: pixel-based at low multipoles, $\\ell$, and a Gaussian approximation to the distribution of cross-power spectra at higher $\\ell$. The main improvements are the use of more and better processed data and of Planck polarization data, and more detailed foreground and instrumental models. More than doubling the data allows further checks and enhanced immunity to systematics. Progress in foreground modelling enables a larger sky fraction, contributing to enhanced precision. Improvements in processing and instrumental models further reduce uncertainties. Extensive tests establish robustness and accuracy, from temperature, from polarization, and from their combination, and show that the {\\Lambda}CDM model continues to offer a very good fit. We further validate the likelihood against specific extensions to this baseline, suc...

  7. Orbit-averaged guiding-center Fokker-Planck operator for numerical applications

    SciTech Connect (OSTI)

    Decker, J.; Peysson, Y.; Duthoit, F.-X. [IRFM, CEA, F-13108 Saint-Paul-lez-Durance (France); Brizard, A. J. [Department of Chemistry and Physics, Saint Michael's College, Colchester, Vermont 05439 (United States)

    2010-11-15

    A guiding-center Fokker-Planck operator is derived in a coordinate system that is well suited for the implementation in a numerical code. This differential operator is transformed such that it can commute with the orbit-averaging operation. Thus, in the low-collisionality approximation, a three-dimensional Fokker-Planck evolution equation for the orbit-averaged distribution function in a space of invariants is obtained. This transformation is applied to a collision operator with nonuniform isotropic field particles. Explicit neoclassical collisional transport diffusion and convection coefficients are derived, and analytical expressions are obtained in the thin orbit approximation. To illustrate this formalism and validate our results, the bootstrap current is analytically calculated in the Lorentz limit.

  8. The present and future of the most favoured inflationary models after $Planck$ 2015

    E-Print Network [OSTI]

    Escudero, Miguel; Boubekeur, Lotfi; Giusarma, Elena; Mena, Olga

    2015-01-01

    The value of the tensor-to-scalar ratio $r$ in the region allowed by the latest $Planck$ 2015 measurements can be associated to a large variety of inflationary models. We discuss here the potential of future Cosmic Microwave Background cosmological observations in disentangling among the possible theoretical scenarios allowed by our analyses of current $Planck$ temperature and polarization data. Rather than focusing only on $r$, we focus as well on the running of the primordial power spectrum, $\\alpha_s$ and the running of thereof, $\\beta_s$. Our Fisher matrix method benefits from a detailed and realistic appraisal of the expected foregrounds. Future cosmological probes, as the COrE mission, may be able to reach an unprecedented accuracy in the extraction of $\\beta_s$ and rule out the most favoured inflationary models.

  9. A Power-Law Formulation of Laminar Flow in Short Pipes Max Sherman

    E-Print Network [OSTI]

    A Power-Law Formulation of Laminar Flow in Short Pipes Max Sherman Indoor Environment Program ABSTRACT This report develops a theoretical description of the hydrodynamic relationship based on a power pipes can be described with a simple power law dependence on pressure, but that the exponent

  10. Improved Approximation Algorithms for the Min-max Tree Cover and Bounded Tree Cover Problems

    E-Print Network [OSTI]

    Salavatipour, Mohammad R.

    ). In this paper we consider Min-Max k-Tree Cover Problem (MMkTC) and Bounded Tree Cover Problem (BTC) defined of the largest tree in the cover is minimized. In the Bounded Tree Cover problem (BTC), we are given the weight G

  11. Computing Reliability Distributions of Windowed Max-log-map (MLM) Detectors : ISI Channels

    E-Print Network [OSTI]

    Kavcic, Aleksandar

    Computing Reliability Distributions of Windowed Max-log-map (MLM) Detectors : ISI Channels Fabian-log-map (MLM) detector has well-known appli- cations to the intersymbol interefence (ISI) channel [1, · · · , is trans- mitted across the ISI channel. Let the following random This work was performed when F. Lim

  12. A Variable Leaky LMS Adaptive Algorithm Max Kamenetsky and Bernard Widrow

    E-Print Network [OSTI]

    Widrow, Bernard

    A Variable Leaky LMS Adaptive Algorithm Max Kamenetsky and Bernard Widrow ISL, Department (650) 723-4769 fax: +1 (650) 723-8473 Abstract--The LMS algorithm has found wide application in many ar- eas of adaptive signal processing and control. We introduce a variable leaky LMS algorithm, designed

  13. Cost-Optimal Planning using Weighted MaxSAT Nathan Robinson

    E-Print Network [OSTI]

    Gretton, Charles

    -benefit plan- ning in fixed-horizon problems. In this setting actions have costs and goal utilities canCost-Optimal Planning using Weighted MaxSAT Nathan Robinson , Charles Gretton , Duc-Nghia Pham the problem of computing optimal plans for propositional planning problems with action costs. In the spirit

  14. Large-Scale Patent Classification with Min-Max Modular Support Vector Machines

    E-Print Network [OSTI]

    Lu, Bao-Liang

    Large-Scale Patent Classification with Min-Max Modular Support Vector Machines Xiao-Lei Chu, Chao Ma, Jing Li, Bao-Liang Lu Senior Member, IEEE, Masao Utiyama, and Hitoshi Isahara Abstract-- Patent-world patent classification typically exceeds one million, and this number increases every year. An effective

  15. A Centralized Associative Behavioral Robotic System Rolando Panez Max Makeev A. Antonio Arroyo Eric Schwartz

    E-Print Network [OSTI]

    Schwartz, Eric M.

    A Centralized Associative Behavioral Robotic System Rolando Panez Max Makeev A. Antonio Arroyo Eric Laboratory University of Florida Abstract The implementation of swarm robotics is still in early stages of simplified swarm intelligence, between robots using the master/slave concept. This paper will give a brief

  16. Advanced Android Motion Detection App Number of teams you can accommodate: max 6

    E-Print Network [OSTI]

    Reed, Nancy E.

    Advanced Android Motion Detection App Number of teams you can accommodate: max 6 Number of students per team: 3-4 Industry Challenge Background The rapid rise of Android and iOS devices has made mobile to grow, many in the defense industry have started viewing Android-based devices as viable low

  17. AmbiMax: Autonomous Energy Harvesting Platform for Multi-Supply Wireless Sensor Nodes

    E-Print Network [OSTI]

    Shinozuka, Masanobu

    AmbiMax: Autonomous Energy Harvesting Platform for Multi-Supply Wireless Sensor Nodes Chulsung Park and a supercapacitor based energy storage system for wireless sensor nodes (WSN). Previous WSNs attempt to harvest of multiple energy harvesting sources including solar, wind, thermal, and vibration, each with a different

  18. On Quanti ed Weighted MAX-SAT Amol D. Mali 1

    E-Print Network [OSTI]

    Mali, Amol D.

    On Quanti#12;ed Weighted MAX-SAT Amol D. Mali 1 Abstract Propositional satis#12;ability (SAT Science, University of Wisconsin, Milwaukee, WI 53211, mali@miller.cs.uwm.edu, Phone: 1-414-229-6762, Fax: 1-414-229-2769, http://www.cs.uwm.edu/faculty/mali. This technical report is an extended version

  19. An Algorithm for Pruning Redundant Modules in Min-Max Modular Network

    E-Print Network [OSTI]

    Lu, Bao-Liang

    of the trained M3 network associated with training data to find out the redundant modules by means of `back, all trained network modules can be integreted into a M3 network automatically according to two moduleAn Algorithm for Pruning Redundant Modules in Min-Max Modular Network Hui-Cheng Lian and Bao

  20. HEAT RECOVERY IN BUILDING ENVELOPES Max H. Sherman and Iain S. Walker

    E-Print Network [OSTI]

    1 LBNL 47329 HEAT RECOVERY IN BUILDING ENVELOPES Max H. Sherman and Iain S. Walker Energy formula may produce an unreasonably high contribution because of heat recovery within the building physical model has been developed and used to predict the infiltration heat recovery based on the Peclet

  1. Airborne MAX-DOAS measurements over California: Testing the NASA OMI tropospheric NO2 product

    E-Print Network [OSTI]

    Airborne MAX-DOAS measurements over California: Testing the NASA OMI tropospheric NO2 product Hilke] Airborne Multi-AXis Differential Optical Absorption Spectroscopy (AMAX-DOAS) measurements of NO2 are compared to the NASA Ozone Monitoring Instrument (OMI) tropospheric vertical columns (data product v2

  2. Salmonella and tomatoes: Q & A for consumers1 Max Teplitski, Keith Schneider and Michelle Danyluk2

    E-Print Network [OSTI]

    Burns, Jacqueline K.

    SL263 Salmonella and tomatoes: Q & A for consumers1 Max Teplitski, Keith Schneider and Michelle sick. Typically, at least several thousand cells of Salmonella are required to cause salmonellosis in healthy adults (although one outbreak of salmonellosis resulted from consuming as few as four Salmonella

  3. Phosphatidic acid activates a wound-activated MAPK in Glycine max

    E-Print Network [OSTI]

    Hirt, Heribert

    the alfalfa MAPK, SIMK. When PA production is inhibited with n-butanol, an inhibitor of phospholipase DPhosphatidic acid activates a wound-activated MAPK in Glycine max Sumin Lee1 , Heribert Hirt2 a systemic increase in phosphatidic acid (PA) levels after being wounded (Lee et al., 1997). To understand

  4. Compatibility of Planck and BICEP2 in the Light of Inflation

    E-Print Network [OSTI]

    Jerome Martin; Christophe Ringeval; Roberto Trotta; Vincent Vennin

    2014-10-29

    We investigate the implications for inflation of the detection of B-modes polarization in the Cosmic Microwave Background (CMB) by BICEP2. We show that the hypothesis of primordial origin of the measurement is only favored by the first four bandpowers, while the others would prefer unreasonably large values of the tensor-to-scalar ratio. Using only those four bandpowers, we carry out a complete analysis in the cosmological and inflationary slow-roll parameter space using the BICEP2 polarization measurements alone and extract the Bayesian evidences and complexities for all the Encyclopaedia Inflationaris models. This allows us to determine the most probable and simplest BICEP2 inflationary scenarios. Although this list contains the simplest monomial potentials, it also includes many other scenarios, suggesting that focusing model building efforts on large field models only is unjustified at this stage. We demonstrate that the sets of inflationary models preferred by Planck alone and BICEP2 alone are almost disjoint, indicating a clear tension between the two data sets. We address this tension with a Bayesian measure of compatibility between BICEP2 and Planck. We find that for models favored by Planck the two data sets tend to be incompatible, whereas there is a moderate evidence of compatibility for the BICEP2 preferred models. As a result, it would be premature to draw any conclusion on the best Planck models, such as Starobinsky and/or Kahler moduli inflation. For the subset of scenarios not exhibiting data sets incompatibility, we update the evidences and complexities using both data sets together.

  5. The Planck energy-mass source as an alternative to the Big Bang

    E-Print Network [OSTI]

    Timashev, Serge F

    2008-01-01

    The general theory of relativity is used to show that the total energy-mass of the visible Universe could be produced by an energy-mass source with the Planck power. The source was supposedly born at the phase of cosmic inflation and acts continuously throughout the lifetime of our Universe. The model allows one to treat dark energy as a real form of energy without using the hypothesis of anti-gravity.

  6. Current dependence of spin torque switching rate based on Fokker-Planck approach

    SciTech Connect (OSTI)

    Taniguchi, Tomohiro Imamura, Hiroshi

    2014-05-07

    The spin torque switching rate of an in-plane magnetized system in the presence of an applied field is derived by solving the Fokker-Planck equation. It is found that three scaling currents are necessary to describe the current dependence of the switching rate in the low-current limit. The dependences of these scaling currents on the applied field strength are also studied.

  7. The Planck energy-mass source as an alternative to the Big Bang

    E-Print Network [OSTI]

    Serge F. Timashev

    2008-04-17

    The general theory of relativity is used to show that the total energy-mass of the visible Universe could be produced by an energy-mass source with the Planck power. The source was supposedly born at the phase of cosmic inflation and acts continuously throughout the lifetime of our Universe. The model allows one to treat dark energy as a real form of energy without using the hypothesis of anti-gravity.

  8. Could Planck level physics be driving classical macroscopic physics through a random walk?

    E-Print Network [OSTI]

    C. L. Herzenberg

    2011-11-28

    We examine a very simple conceptual model of stochastic behavior based on a random walk process in velocity space. For objects engaged in classical non-relativistic velocities, this leads under asymmetric conditions to acceleration processes that resemble the behavior of objects subject to Newton's second law, and in three dimensional space, acceleration dependent on an inverse square law emerges. Thus, a non-relativistic random walk would appear to be capable of describing certain prominent features of classical physics; however, this classical behavior appears to be able to take place only for objects with mass exceeding a threshold value which we identify with the Planck mass. Under these circumstances, stochastic space-time displacements would be smaller than the Planck length and the Planck time so that such classically behaved objects would be effectively localized. Lower mass objects exhibit more rapid diffusion and less localization, and a relativistic random walk would seem to be required of objects having masses comparable to and smaller than the threshold mass value. Results suggest the possibility of an intrinsic quantum-classical transition in the microgram mass range.

  9. Petroleum Institute Scholarly Publications

    E-Print Network [OSTI]

    Abu Dhabi The Petroleum Institute Scholarly Publications 2010 #12;#12;The Petroleum Institute Belhaj Petroleum Engineering Sadoon Morad Petroleum Geosciences Sivakumar Sivasubramaniam College of Arts departments within the Petroleum Institute. Names in bold show Petroleum Institute faculty who are attached

  10. Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator

    SciTech Connect (OSTI)

    Novaes, C.P.; Wuensche, C.A. [Divisão de Astrofísica, Instituto Nacional de Pesquisas Espaciais, Av. dos Astronautas 1758, São José dos Campos 12227-010, SP (Brazil); Bernui, A. [Observatório Nacional, Rua General José Cristino 77, São Cristóvão, 20921-400, Rio de Janeiro, RJ (Brazil); Ferreira, I.S., E-mail: camilapnovaes@gmail.com, E-mail: bernui@on.br, E-mail: ivan@fis.unb.br, E-mail: ca.wuensche@inpe.br [Instituto de Física, Universidade de Brasília, Campus Universitário Darcy Ribeiro, Asa Norte, 70919-970, Brasília, DF (Brazil)

    2014-01-01

    The extensive search for deviations from Gaussianity in cosmic microwave background radiation (CMB) data is very important due to the information about the very early moments of the universe encoded there. Recent analyses from Planck CMB data do not exclude the presence of non-Gaussianity of small amplitude, although they are consistent with the Gaussian hypothesis. The use of different techniques is essential to provide information about types and amplitudes of non-Gaussianities in the CMB data. In particular, we find interesting to construct an estimator based upon the combination of two powerful statistical tools that appears to be sensitive enough to detect tiny deviations from Gaussianity in CMB maps. This estimator combines the Minkowski functionals with a Neural Network, maximizing a tool widely used to study non-Gaussian signals with a reinforcement of another tool designed to identify patterns in a data set. We test our estimator by analyzing simulated CMB maps contaminated with different amounts of local primordial non-Gaussianity quantified by the dimensionless parameter f{sub  NL}. We apply it to these sets of CMB maps and find ?> 98% of chance of positive detection, even for small intensity local non-Gaussianity like f{sub  NL} = 38±18, the current limit from Planck data for large angular scales. Additionally, we test the suitability to distinguish between primary and secondary non-Gaussianities: first we train the Neural Network with two sets, one of nearly Gaussian CMB maps (|f{sub  NL}| ? 10) but contaminated with realistic inhomogeneous Planck noise (i.e., secondary non-Gaussianity) and the other of non-Gaussian CMB maps, that is, maps endowed with weak primordial non-Gaussianity (28 ? f{sub  NL} ? 48); after that we test an ensemble composed of CMB maps either with one of these non-Gaussian contaminations, and find out that our method successfully classifies ? 95% of the tested maps as being CMB maps containing primordial or secondary non-Gaussianity. Furthermore, we analyze the foreground-cleaned Planck maps obtaining constraints for non-Gaussianity at large-angles that are in good agreement with recent constraints. Finally, we also test the robustness of our estimator including cut-sky masks and realistic noise maps measured by Planck, obtaining successful results as well.

  11. A joint analysis of Planck and BICEP2 B modes including dust polarization uncertainty

    SciTech Connect (OSTI)

    Mortonson, Michael J.; Seljak, Uroš E-mail: useljak@berkeley.edu

    2014-10-01

    We analyze BICEP2 and Planck data using a model that includes CMB lensing, gravity waves, and polarized dust. Recently published Planck dust polarization maps have highlighted the difficulty of estimating the amount of dust polarization in low intensity regions, suggesting that the polarization fractions have considerable uncertainties and may be significantly higher than previous predictions. In this paper, we start by assuming nothing about the dust polarization except for the power spectrum shape, which we take to be C{sub l}{sup BB,dust} ? l{sup -2.42}. The resulting joint BICEP2+Planck analysis favors solutions without gravity waves, and the upper limit on the tensor-to-scalar ratio is r<0.11, a slight improvement relative to the Planck analysis alone which gives r<0.13 (95% c.l.). The estimated amplitude of the dust polarization power spectrum agrees with expectations for this field based on both HI column density and Planck polarization measurements at 353 GHz in the BICEP2 field. Including the latter constraint on the dust spectrum amplitude in our analysis improves the limit further to r < 0.09, placing strong constraints on theories of inflation (e.g., models with r>0.14 are excluded with 99.5% confidence). We address the cross-correlation analysis of BICEP2 at 150 GHz with BICEP1 at 100 GHz as a test of foreground contamination. We find that the null hypothesis of dust and lensing with 0r= gives ? ?{sup 2} < 2 relative to the hypothesis of no dust, so the frequency analysis does not strongly favor either model over the other. We also discuss how more accurate dust polarization maps may improve our constraints. If the dust polarization is measured perfectly, the limit can reach r < 0.05 (or the corresponding detection significance if the observed dust signal plus the expected lensing signal is below the BICEP2 observations), but this degrades quickly to almost no improvement if the dust calibration error is 20% or larger or if the dust maps are not processed through the BICEP2 pipeline, inducing sampling variance noise.

  12. INSTITUTIONAL MEMBERS CURRENT SCIENCE ASSOCIATION

    E-Print Network [OSTI]

    Giri, Ranjit K.

    , Guwahati 40. Indian Institute of Technology, Hyderabad 41. Indian Institute of Technology, Indore 42

  13. Determination of Dark Energy and Dark Matter from the values of Redshift for the present time, Planck and Trans-Planck epochs of the Big-Bang model

    E-Print Network [OSTI]

    Asger G. Gasanalizade; Ramin A. Hasanalizade

    2015-02-20

    As an alternative to the Standard cosmology model we have developed a new modified Freundlich's (quantum relativity) redshift (MFRS) mechanisms, which provide a precise solutions of the Dark Energy and Dark Matter problems. We apply the joint solution of three MFRS equations for concordances quantize bounce Planck hierarchy steps. Simultaneous scaling solutions of MFRS equations in logarithmic scale appropriate to three cosmological epoch's, yields a currently testable predictions regarding the Dark Matter {\\Omega}_{DM} = 0.25, and Dark Energy {\\Omega}_{DE} = 0.75. These predictions coincides with the recent observational data from WMAP and other a key supernovae SNe Ia findings. Thus, the presence of Dark Matter and Dark Energy had already been not only detected observationally, but also confirmed theoretically with the very compelling accuracy. From the WMAP7 and our predicted ages we find a value of the Hubble constant H_0 = 65.6 km * s^{-1} Mpc^{-1} which is excellent agreement with the Planck 2013 results XVI. Compared with the "holographic scenario" results, we find an important coincidence between our new and "holographic" parameters. We discuss the connection hierarchy between the multiverse masses and examine the status of the cosmic acceleration. The product of the age of the Universe into the cosmic acceleration in each cosmological epochs --including present day are constant and precisely corresponds to an possible observable-geophysical parameter g_U = 9.50005264_{265} (exact) * (m/s^2). For the derived by WMAP7 age of the Universe t_{W7} = 13.75(13) * 10^9 yr, we find the relevant acceleration a_{W7} = 6.91(65) * 10^{-10} m/s^2. The predicted value of t_0 = 9.0264_9(51) * 10^2 Gyr is consistent with the background acceleration. a_0 = 1.05246_4(61) * 10^{-11} m/s^2.

  14. Weizmann Institute 76100 Rehovot,

    E-Print Network [OSTI]

    Prior, Yehiam

    , Weizmann Institute 2006 - Alternative Energy Research Initiative (WIS), Steering Committee 2006 - Dean by the international diamond processing community, and sold hundreds of machines world wide. 1988 - 1990 Bell Foundation Israel Diamond Institute MAGNET program (LESHED, diode pumped lasers consortium) Minerva

  15. On the significance of power asymmetries in Planck CMB data at all scales

    SciTech Connect (OSTI)

    Quartin, Miguel [Instituto de Física, Universidade Federal do Rio de Janeiro, 21941-972, Rio de Janeiro, RJ (Brazil); Notari, Alessio, E-mail: mquartin@if.ufrj.br, E-mail: notari@ffn.ub.es [Departament de Física Fondamental i Institut de Ciéncies del Cosmos, Universitat de Barcelona, Martí i Franqués 1, E-08028 Barcelona (Spain)

    2015-01-01

    We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if there is any significant deviation from cosmological isotropy. We look for differences in the spectrum between two opposite hemispheres and also for dipolar modulations. We propose a new way to avoid biases due to partial-sky coverage by producing a mask symmetrized in antipodal directions, in addition to the standard smoothing procedure. We also properly take into account both Doppler and aberration effects due to our peculiar velocity and the anisotropy of the noise, since these effects induce a significant hemispherical asymmetry. We are thus able to probe scales all the way to ? = 2000. After such treatment we find no evidence for significant hemispherical anomalies along any of the analyzed directions (i.e. deviations are less than 1.5? when summing over all scales). Although among the larger scales there are sometimes higher discrepancies, these are always less than 3?. We also find results on a dipolar modulation of the power spectrum. Along the hemispheres aligned with the most asymmetric direction for 2 ? ? ? 2000 we find a 3.3? discrepancy when comparing to simulations. However, if we do not restrict ourselves to Planck's maximal asymmetry axis, which can only be known a posteriori, and compare Planck data with the modulation of simulations along their respective maximal asymmetry directions, the discrepancy goes down to less than 1? (with, again, almost 3? discrepancies in some low-? modes). We thus conclude that no significant power asymmetries seem to be present in the full data set. Interestingly, without proper removal of Doppler and aberration effects one would find spurious anomalies at high ?, between 3? and 5?. Even when considering only ? < 600 we find that the boost is non-negligible and alleviates the discrepancy by roughly half-?.

  16. A Joint Analysis of BICEP2/Keck Array and Planck Data

    E-Print Network [OSTI]

    BICEP2/Keck; Planck Collaborations; :; P. A. R. Ade; N. Aghanim; Z. Ahmed; R. W. Aikin; K. D. Alexander; M. Arnaud; J. Aumont; C. Baccigalupi; A. J. Banday; D. Barkats; R. B. Barreiro; J. G. Bartlett; N. Bartolo; E. Battaner; K. Benabed; A. Benoît; A. Benoit-Lévy; S. J. Benton; J. -P. Bernard; M. Bersanelli; P. Bielewicz; C. A. Bischoff; J. J. Bock; A. Bonaldi; L. Bonavera; J. R. Bond; J. Borrill; F. R. Bouchet; F. Boulanger; J. A. Brevik; M. Bucher; I. Buder; E. Bullock; C. Burigana; R. C. Butler; V. Buza; E. Calabrese; J. -F. Cardoso; A. Catalano; A. Challinor; R. -R. Chary; H. C. Chiang; P. R. Christensen; L. P. L. Colombo; C. Combet; J. Connors; F. Couchot; A. Coulais; B. P. Crill; A. Curto; F. Cuttaia; L. Danese; R. D. Davies; R. J. Davis; P. de Bernardis; A. de Rosa; G. de Zotti; J. Delabrouille; J. -M. Delouis; F. -X. Désert; C. Dickinson; J. M. Diego; H. Dole; S. Donzelli; O. Doré; M. Douspis; C. D. Dowell; L. Duband; A. Ducout; J. Dunkley; X. Dupac; C. Dvorkin; G. Efstathiou; F. Elsner; T. A. Enßlin; H. K. Eriksen; E. Falgarone; J. P. Filippini; F. Finelli; S. Fliescher; O. Forni; M. Frailis; A. A. Fraisse; E. Franceschi; A. Frejsel; S. Galeotta; S. Galli; K. Ganga; T. Ghosh; M. Giard; E. Gjerløw; S. R. Golwala; J. González-Nuevo; K. M. Górski; S. Gratton; A. Gregorio; A. Gruppuso; J. E. Gudmundsson; M. Halpern; F. K. Hansen; D. Hanson; D. L. Harrison; M. Hasselfield; G. Helou; S. Henrot-Versillé; D. Herranz; S. R. Hildebrandt; G. C. Hilton; E. Hivon; M. Hobson; W. A. Holmes; W. Hovest; V. V. Hristov; K. M. Huffenberger; H. Hui; G. Hurier; K. D. Irwin; A. H. Jaffe; T. R. Jaffe; J. Jewell; W. C. Jones; M. Juvela; A. Karakci; K. S. Karkare; J. P. Kaufman; B. G. Keating; S. Kefeli; E. Keihänen; S. A. Kernasovskiy; R. Keskitalo; T. S. Kisner; R. Kneissl; J. Knoche; L. Knox; J. M. Kovac; N. Krachmalnicoff; M. Kunz; C. L. Kuo; H. Kurki-Suonio; G. Lagache; A. Lähteenmäki; J. -M. Lamarre; A. Lasenby; M. Lattanzi; C. R. Lawrence; E. M. Leitch; R. Leonardi; F. Levrier; A. Lewis; M. Liguori; P. B. Lilje; M. Linden-Vørnle; M. López-Caniego; P. M. Lubin; M. Lueker; J. F. Macías-Pérez; B. Maffei; D. Maino; N. Mandolesi; A. Mangilli; M. Maris; P. G. Martin; E. Martínez-González; S. Masi; P. Mason; S. Matarrese; K. G. Megerian; P. R. Meinhold; A. Melchiorri; L. Mendes; A. Mennella; M. Migliaccio; S. Mitra; M. -A. Miville-Deschênes; A. Moneti; L. Montier; G. Morgante; D. Mortlock; A. Moss; D. Munshi; J. A. Murphy; P. Naselsky; F. Nati; P. Natoli; C. B. Netterfield; H. T. Nguyen; H. U. Nørgaard-Nielsen; F. Noviello; D. Novikov; I. Novikov; R. O'Brient; R. W. Ogburn IV; A. Orlando; L. Pagano; F. Pajot; R. Paladini; D. Paoletti; B. Partridge; F. Pasian; G. Patanchon; T. J. Pearson; O. Perdereau; L. Perotto; V. Pettorino; F. Piacentini; M. Piat; D. Pietrobon; S. Plaszczynski; E. Pointecouteau; G. Polenta; N. Ponthieu; G. W. Pratt; S. Prunet; C. Pryke; J. -L. Puget; J. P. Rachen; W. T. Reach; R. Rebolo; M. Reinecke; M. Remazeilles; C. Renault; A. Renzi; S. Richter; I. Ristorcelli; G. Rocha; M. Rossetti; G. Roudier; M. Rowan-Robinson; J. A. Rubiño-Martín; B. Rusholme; M. Sandri; D. Santos; M. Savelainen; G. Savini; R. Schwarz; D. Scott; M. D. Seiffert; C. D. Sheehy; L. D. Spencer; Z. K. Staniszewski; V. Stolyarov; R. Sudiwala; R. Sunyaev; D. Sutton; A. -S. Suur-Uski; J. -F. Sygnet; J. A. Tauber; G. P. Teply; L. Terenzi; K. L. Thompson; L. Toffolatti; J. E. Tolan; M. Tomasi; M. Tristram; M. Tucci; A. D. Turner; L. Valenziano; J. Valiviita; B. Van Tent; L. Vibert; P. Vielva; A. G. Vieregg; F. Villa; L. A. Wade; B. D. Wandelt; R. Watson; A. C. Weber; I. K. Wehus; M. White; S. D. M. White; J. Willmert; C. L. Wong; K. W. Yoon; D. Yvon; A. Zacchei; A. Zonca

    2015-04-14

    We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg$^2$ patch of sky centered on RA 0h, Dec. $-57.5\\deg$. The combined maps reach a depth of 57 nK deg in Stokes $Q$ and $U$ in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven frequencies from 30 to 353 GHz, but much less deeply in any given region (1.2 $\\mu$K deg in $Q$ and $U$ at 143 GHz). We detect 150$\\times$353 cross-correlation in $B$-modes at high significance. We fit the single- and cross-frequency power spectra at frequencies $\\geq 150$ GHz to a lensed-$\\Lambda$CDM model that includes dust and a possible contribution from inflationary gravitational waves (as parameterized by the tensor-to-scalar ratio $r$), using a prior on the frequency spectral behavior of polarized dust emission from previous \\planck\\ analysis of other regions of the sky. We find strong evidence for dust and no statistically significant evidence for tensor modes. We probe various model variations and extensions, including adding a synchrotron component in combination with lower frequency data, and find that these make little difference to the $r$ constraint. Finally we present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for $r$, and yields an upper limit $r_{0.05}<0.12$ at 95% confidence. Marginalizing over dust and $r$, lensing $B$-modes are detected at $7.0\\,\\sigma$ significance.

  17. OIL & GAS INSTITUTE Introduction

    E-Print Network [OSTI]

    Strathclyde, University of

    OIL & GAS INSTITUTE CONTENTS Introduction Asset Integrity Underpinning Capabilities 2 4 4 6 8 9 10 COMPETITIVENESS UNIVERSITY of STRATHCLYDE OIL & GAS INSTITUTE OIL & GAS EXPERTISE AND PARTNERSHIPS #12;1 The launch of the Strathclyde Oil & Gas Institute represents an important step forward for the University

  18. The National Cancer Institute,

    E-Print Network [OSTI]

    The National Cancer Institute, International Cancer Information Center Bldg. 82, Rm 123 Bethesda, MD 20892 The National Cancer Institute (NCI) is part of the Federal Government. NCI coordinates the government's cancer research program. It is the largest of the 17 biomedical research institutes and centers

  19. The Morphology of the Anomalous Microwave Emission in the Planck 2015 data release

    E-Print Network [OSTI]

    von Hausegger, Sebastian

    2015-01-01

    We calculate weighted mosaic correlations between the recently published Planck 2015 foreground maps - both anomalous microwave emission (AME) maps, free-free emission, synchrotron radiation and thermal dust emission. The weighting coefficients are constructed taking account of the signal-to-error ratio given by the data product. Positive correlation is found for AME compared with thermal dust emission as well as synchrotron radiation. We find AME and free-free emission tending to be anti-correlated, however, when investigating different scales, their relationship appears to be more complex. We argue that dust particles responsible for AME are pushed out of hot zones in the interstellar medium (ISM).

  20. Queue length asymptotics for generalized max-weight scheduling in the presence of heavy-tailed traffic

    E-Print Network [OSTI]

    Jagannathan, Krishna Prasanna

    We investigate the asymptotic behavior of the steady-state queue length distribution under generalized max-weight scheduling in the presence of heavy-tailed traffic. We consider a system consisting of two parallel queues, ...

  1. National Science Library, CAS Expert Review Meeting

    E-Print Network [OSTI]

    Wang, Wei Hua

    (Institute Directors) 9.800 Scientists and scholarship holders 80 Max Planck Institutes MPG Budget 1,4 bn 8 and registry services für MPG (e.g. PubMan) Support with data publications and related visualization (e semantic full text search. Bibliometric indicators (for research evaluation) and calculation

  2. THE ASTROPHYSICAL JOURNAL, 509:212228, 1998 December 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(

    E-Print Network [OSTI]

    Moskalenko, Igor V.

    for the calculation of Galactic cosmic-ray propagation has been developed, building on the approach described- 1 Max-Planck-Institut fu r extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany; aws=mpe.mpg.de; imos=mpe.mpg.de. 2 Institute for Nuclear Physics, M. V. Lomonosov Moscow State Uni- versity, 119 899

  3. 1036 VOLUME 34J O U R N A L O F P H Y S I C A L O C E A N O G R A P H Y 2004 American Meteorological Society

    E-Print Network [OSTI]

    Drijfhout, Sybren

    energy. This increase in the energy conversion is absent in the wind-driven case, indicating an important Meteorological Society Remote Wind-Driven Overturning in the Absence of the Drake Passage Effect BARRY A. KLINGER Max Planck Institute for Meteorology, Hamburg, Germany JEFFERY R. SCOTT Massachusetts Institute

  4. Manuscript prepared for Atmos. Chem. Phys. with version 3.0 of the LATEX class copernicus.cls.

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    , China 2 Institute for Energy- and Climate Research (IEK-8), Forschungszentrum J¨ulich, J¨ulich, Germany 3 Max-Planck-Institut for Chemistry, Mainz, Germany Correspondence to: T. Brauers (th from the OMI observations. 4 #12;Fig. S6. Time series of wind speed in the 9 cloud-free days during

  5. Geophysical Research Abstracts Vol. 13, EGU2011-7998, 2011

    E-Print Network [OSTI]

    Ulich, Thomas

    ), and Thomas Ulich (4) (1) University of Bern, Institute of Applied Physics, Microwave, Bern, Switzerland, Germany, (3) Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4) Sodankylä microwave radiometers measured middle atmospheric water vapor profiles, one in Andenes, Norway (69.3 N, 16 E

  6. AcceptedArticle 2013 American Geophysical Union. All Rights Reserved.

    E-Print Network [OSTI]

    Department of Energy, Washington, DC, USA. 11 Max Planck Institute, Hamburg, Germany. 12 University of Tokyo, Washington, USA. 9 Deutsches Zentrum für Luft- und Raumfahrt Oberpfaffenhofen, Wessling, Germany. 10 US Forschungszentrum Jülich GmbH, Jülich, Germany. 15 Norwegian Meteorological Institute, Oslo, Norway. 16 Indian

  7. 3rd Survey on the Situation of PhD Students in the Max Planck Society Open from the 25th of May until the 21th of June

    E-Print Network [OSTI]

    insurance I don't have such an insurance other insurance G8 Are you male or female? Variables: G8 1 Female 2

  8. An efficient particle Fokker–Planck algorithm for rarefied gas flows

    SciTech Connect (OSTI)

    Gorji, M. Hossein; Jenny, Patrick

    2014-04-01

    This paper is devoted to the algorithmic improvement and careful analysis of the Fokker–Planck kinetic model derived by Jenny et al. [1] and Gorji et al. [2]. The motivation behind the Fokker–Planck based particle methods is to gain efficiency in low Knudsen rarefied gas flow simulations, where conventional direct simulation Monte Carlo (DSMC) becomes expensive. This can be achieved due to the fact that the resulting model equations are continuous stochastic differential equations in velocity space. Accordingly, the computational particles evolve along independent stochastic paths and thus no collision needs to be calculated. Therefore the computational cost of the solution algorithm becomes independent of the Knudsen number. In the present study, different computational improvements were persuaded in order to augment the method, including an accurate time integration scheme, local time stepping and noise reduction. For assessment of the performance, gas flow around a cylinder and lid driven cavity flow were studied. Convergence rates, accuracy and computational costs were compared with respect to DSMC for a range of Knudsen numbers (from hydrodynamic regime up to above one). In all the considered cases, the model together with the proposed scheme give rise to very efficient yet accurate solution algorithms.

  9. Bohr - Planck quantum theory, (Tesla) magnetic monopoles and fine structure constant

    E-Print Network [OSTI]

    Vladan Pankovic; Darko V. Kapor; Stevica Djurovic; Miodrag Krmar

    2014-10-17

    In this work we apply Bohr-Planck (Old quantum atomic and radiation) theory, i.e. and quasi-classical methods for analysis of the magnetic monopoles and other problems. We reproduce exactly some basic elements of the Dirac magnetic monopoles theory, especially Dirac electric/magnetic charge quantization condition. Also, we suggest a new, effective, simply called Tesla model (for analogy with positions of the solenoids by Tesla inductive motor) of the magnetic monopole instead of usual effective Dirac model (half-infinite, very tinny solenoid) of the magnetic monopole. In our, i.e. Tesla model we use three equivalent tiny solenoids connected in series with a voltage source. One end of any solenoid is placed at the circumference of a circle and solenoids are directed radial toward circle center. Length of any solenoid is a bit smaller than finite circle radius so that other end of any solenoid is very close to the circle center. Angles between neighboring solenoids equal $120^{\\circ}$. All this implies that, practically, there is no magnetic field, or, magnetic pole, e.g. $S$, in the circle center, and that whole system holds only other, $N$ magnetic pole, at the ends of the solenoids at circle circumference. Finally, we reproduce relatively satisfactory value of the fine structure constant using Planck, i.e. Bose-Einstein statistics and Wien displacement law.

  10. Self-unitarization of New Higgs Inflation and compatibility with Planck and BICEP2 data

    E-Print Network [OSTI]

    Cristiano Germani; Yuki Watanabe; Nico Wintergerst

    2014-12-09

    In this paper we show that the Germani-Kehagias model of Higgs inflation (or New Higgs Inflation), where the Higgs boson is kinetically non-minimally coupled to the Einstein tensor is in perfect compatibility with the latest Planck and BICEP2 data. Moreover, we show that the tension between the Planck and BICEP2 data can be relieved within the New Higgs inflation scenario by a negative running of the spectral index. Regarding the unitarity of the model, we argue that it is unitary throughout the evolution of the Universe. Weak couplings in the Higgs-Higgs and Higgs-graviton sectors are provided by a large background dependent cut-off scale during inflation. In the same regime, the W and Z gauge bosons acquire a very large mass, thus decouple. On the other hand, if they are also non-minimally coupled to the Higgs boson, their effective masses can be enormously reduced. In this case, the W and Z bosons are no longer decoupled. After inflation, the New Higgs model is well approximated by a quartic Galileon with a renormalizable potential. We argue that this can unitarily create the right conditions for inflation to eventually start.

  11. Self-unitarization of New Higgs Inflation and compatibility with Planck and BICEP2 data

    SciTech Connect (OSTI)

    Germani, Cristiano; Wintergerst, Nico; Watanabe, Yuki E-mail: watanabe@resceu.s.u-tokyo.ac.jp

    2014-12-01

    In this paper we show that the Germani-Kehagias model of Higgs inflation (or New Higgs Inflation), where the Higgs boson is kinetically non-minimally coupled to the Einstein tensor is in perfect compatibility with the latest Planck and BICEP2 data. Moreover, we show that the tension between the Planck and BICEP2 data can be relieved within the New Higgs inflation scenario by a negative running of the spectral index. Regarding the unitarity of the model, we argue that it is unitary throughout the evolution of the Universe. Weak couplings in the Higgs-Higgs and Higgs-graviton sectors are provided by a large background dependent cut-off scale during inflation. In the same regime, the W and Z gauge bosons acquire a very large mass, thus decouple. On the other hand, if they are also non-minimally coupled to the Higgs boson, their effective masses can be enormously reduced. In this case, the W and Z bosons are no longer decoupled. After inflation, the New Higgs model is well approximated by a quartic Galileon with a renormalizable potential. We argue that this can unitarily create the right conditions for inflation to eventually start.

  12. ~max0006

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorkingLosThe 26thI D- 6 0 4 2 rz machine |NNSA0202(2).pdf More

  13. Max Schulze

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room NewsInformationJesse BergkampCentermillion toMSDSMaterialsMathematicalWalther

  14. Max Schulze

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on dark matter By Sarah Schlieder *8Matthew Tirrell

  15. Indian Institute of Technology Bombay INDIAN INSTITUTE OF TECHNOLOGY BOMBAY

    E-Print Network [OSTI]

    Narayanan, H.

    Indian Institute of Technology Bombay INDIAN INSTITUTE OF TECHNOLOGY BOMBAY INVITATION Description of work Estimated cost (1) (2) (3) 1 Construction of Institutional/Residential buildings, external development, HVAC, Elevators etc. for Indian Institute of Technology Bombay, at the campus

  16. On the detection of point sources in Planck LFI 70 GHz CMB maps based on cleaned K-map

    E-Print Network [OSTI]

    Khachatryan, H G; Poghosyan, E; Yegoryan, G

    2015-01-01

    We use the Planck LFI 70GHz data to further probe point source detection technique in the sky maps of the cosmic microwave background (CMB) radiation. The method developed by Tegmark et al. for foreground reduced maps and the Kolmogorov parameter as the descriptor are adopted for the analysis of Planck satellite CMB temperature data. Most of the detected points coincide with point sources already revealed by other methods. However, we have also found 9 source candidates for which still no counterparts are known.

  17. Institutional Research & Development Reports | National Nuclear...

    National Nuclear Security Administration (NNSA)

    Advanced Simulation and Computing and Institutional R&D Programs Institutional Research & Development Institutional Research & Development Reports Institutional Research &...

  18. Determine Institutional Change Sustainability Goals | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change Determine Institutional Change Sustainability Goals Determine Institutional Change Sustainability Goals Institutional Change Continuous Improvement Cycle...

  19. Institutional Change for Sustainability Contacts | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change Institutional Change for Sustainability Contacts Institutional Change for Sustainability Contacts For more information about institutional change for...

  20. UNCLASSIFIED Institute for Materials ...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Antonia Antoniou Georgia Institute of Technology, Atlanta, Georgia Mechanical Behavior of Hierarchical Nanoporous Metals Thursday, August 27, 2015 1:30 - 2:30pm MSL Auditorium...

  1. Edison Electric Institute Update

    Broader source: Energy.gov [DOE]

    Presentation—given at the Fall 2011 Federal Utility Partnership Working Group (FUPWG) meeting—discusses the Edison Electric Institute (EEI) and the current electricity landscape.

  2. UNCLASSIFIED Institute for Materials ...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Gabriel Aeppli Head of the Synchrotron and Nanotechnology Department Paul Scherrer Institute, Switzerland Accelerator-based Light Sources for the Future Wednesday, August 12, 2015...

  3. UNCLASSIFIED Institute for Materials ...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Dr. Jol Mesot Director, Paul Scherrer Institute, Switzerland Probing Excitations in Strongly Correlated Electron Systems: Recent Highlights Obtained at the Large-Scale Facilities...

  4. UNCLASSIFIED Institute for Materials ...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Head of the Synchrotron and Nanotechnology Department Paul Scherrer Institute, Switzerland Accelerator-based Light Sources for the Future Wednesday, August 12, 2015 2:00 to...

  5. Max Tech and Beyond: Maximizing Appliance and Equipment Efficiency by Design

    SciTech Connect (OSTI)

    Desroches, Louis-Benoit; Garbesi, Karina

    2011-07-20

    It is well established that energy efficiency is most often the lowest cost approach to reducing national energy use and minimizing carbon emissions. National investments in energy efficiency to date have been highly cost-effective. The cumulative impacts (out to 2050) of residential energy efficiency standards are expected to have a benefit-to-cost ratio of 2.71:1. This project examined energy end-uses in the residential, commercial, and in some cases the industrial sectors. The scope is limited to appliances and equipment, and does not include building materials, building envelopes, and system designs. This scope is consistent with the scope of DOE's appliance standards program, although many products considered here are not currently subject to energy efficiency standards. How much energy could the United States save if the most efficient design options currently feasible were adopted universally? What design features could produce those savings? How would the savings from various technologies compare? With an eye toward identifying promising candidates and strategies for potential energy efficiency standards, the Max Tech and Beyond project aims to answer these questions. The analysis attempts to consolidate, in one document, the energy savings potential and design characteristics of best-on-market products, best-engineered products (i.e., hypothetical products produced using best-on-market components and technologies), and emerging technologies in research & development. As defined here, emerging technologies are fundamentally new and are as yet unproven in the market, although laboratory studies and/or emerging niche applications offer persuasive evidence of major energy-savings potential. The term 'max tech' is used to describe both best-engineered and emerging technologies (whichever appears to offer larger savings). Few best-on-market products currently qualify as max tech, since few apply all available best practices and components. The three primary analyses presented in this report are: Nevertheless, it is important to analyze best-on-market products, since data on truly max tech technologies are limited. (1) an analysis of the cross-cutting strategies most promising for reducing appliance and equipment energy use in the U.S.; (2) a macro-analysis of the U.S. energy-saving potential inherent in promising ultra-efficient appliance technologies; and (3) a product-level analysis of the energy-saving potential.

  6. Property:OpenEI/UtilityRate/DemandRateStructure/Tier1Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDate Jump to:Information Tier1Max Jump to: navigation,

  7. Property:OpenEI/UtilityRate/DemandRateStructure/Tier2Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDate Jump to:Information Tier1Max Jump

  8. Property:OpenEI/UtilityRate/DemandRateStructure/Tier3Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDate Jump to:Information Tier1MaxInformation

  9. Property:OpenEI/UtilityRate/EnergyRateStructure/Tier3Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDate JumpEnergyInformation SellInformation Max Jump

  10. Property:OpenEI/UtilityRate/EnergyRateStructure/Tier5Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDateInformation Max Jump to: navigation, search This is

  11. Property:OpenEI/UtilityRate/EnergyRateStructure/Tier6Max | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo,AltFuelVehicle2 JumpPublicationDateInformation Max Jump to: navigation,

  12. text in "Max kWh" fields | OpenEI Community

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop IncIowa (UtilityMichigan)data bookresult formats Homestormtext in "Max

  13. Claire E. Max, 2004 | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorkingLosThe 26thI D- 6 0GrantsTheBurtonCertifiedChicago OfficeClaire E. Max,

  14. Planck is Europe's first mission to study the relic radiation from the Big Bang. Ever since the detection of small fluctuations in the temperature of this radiation, announced in late 1992,

    E-Print Network [OSTI]

    the Nobel Prize in 1918. Planck will map the structure of the Cosmic Microwave Background radiationPlanck Planck is Europe's first mission to study the relic radiation from the Big Bang. Ever since the detection of small fluctuations in the temperature of this radiation, announced in late 1992, astronomers

  15. Universittsarchiv Mainz Physiologisches Institut

    E-Print Network [OSTI]

    ;Vorwort II Vorwort Das Physiologische Institut wurde 1946 mit der Berufung von Prof. Hans Schriever (1898-1979) einge- richtet. Der 1898 in Düsseldorf geborene Schriever promovierte 1921 in Bonn zum Dr. med. und 1922 wurde er 1939 zum ordentlichen Professor ernannt. Prof. Schriever leitete das Mainzer Institut bis zu

  16. Inflationary generalized Chaplygin gas and dark energy in the light of the Planck and BICEP2 experiments

    E-Print Network [OSTI]

    Bikash R Dinda; Sumit Kumar; Anjan A. Sen

    2014-10-21

    In this work, we study an inflationary scenario in the presence of Generalized Chaplygin Gas (GCG). We show that in Einstein gravity, GCG is not a suitable candidate for inflation; but in a five dimensional brane world scenario, it can work as a viable inflationary model. We calculate the relevant quantities such as $n_{s}$, $r$ and $A_{s}$ related to the primordial scalar and tensor fluctuations, and using their recent bounds from Planck and BICEP2, we constrain the model parameters as well as the five-dimensional Planck mass. But as a slow-roll inflationary model with a power-law type scalar primordial power spectrum, GCG as an inflationary model can not resolve the tension between results from BICEP2 and Planck with a concordance $\\Lambda$CDM Universe. We show that going beyond the concordance $\\Lambda$CDM model and incorporating more general dark energy behaviour, this tension may be eased. We also obtain the constraints on the $n_{s}$ and $r$ and the GCG model parameters using Planck+WP+BICEP2 data considering the CPL dark energy behaviour.

  17. Low-energy expansion formula for one-dimensional Fokker-Planck and Schrödinger equations with periodic potentials

    E-Print Network [OSTI]

    Toru Miyazawa

    2011-12-26

    We study the low-energy behavior of the Green function for one-dimensional Fokker-Planck and Schr\\"odinger equations with periodic potentials. We derive a formula for the power series expansion of reflection coefficients in terms of the wave number, and apply it to the low-energy expansion of the Green function.

  18. Low-energy expansion formula for one-dimensional Fokker-Planck and Schrödinger equations with asymptotically periodic potentials

    E-Print Network [OSTI]

    Toru Miyazawa

    2011-12-26

    We consider one-dimensional Fokker-Planck and Schr\\"odinger equations with a potential which approaches a periodic function at spatial infinity. We extend the low-energy expansion method, which was introduced in previous papers, to be applicable to such asymptotically periodic cases. Using this method, we study the low-energy behavior of the Green function.

  19. TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY

    E-Print Network [OSTI]

    #12;06 06 TOKYO INSTITUTE OF TECHNOLOGY 0201 CONTENTS 03 08 09 10 15 17 25 31 33 37 41 0201 08 23 TokyoTech #12;TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY 0403 20 1 5 11 #12;TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY 0605 4 3 2 5 5 4 3 #12;TOKYO INSTITUTE OF TECHNOLOGY

  20. Deterministic proton transport solving a one dimensional Fokker-Planck equation

    SciTech Connect (OSTI)

    Marr, D.; Prael, R.; Adams, K.; Alcouffe, R.

    1997-10-01

    The transport of protons through matter is characterized by many interactions which cause small deflections and slight energy losses. The few which are catastrophic or cause large angle scattering can be viewed as extinction for many applications. The transport of protons at this level of approximation can be described by a Fokker Planck Equation. This equation is solved using a deterministic multigroup differencing scheme with a highly resolved set of discrete ordinates centered around the beam direction which is adequate to properly account for deflections and energy losses due to multiple Coulomb scattering. Comparisons with LAHET for a large variety of problems ranging from 800 MeV protons on a copper step wedge to 10 GeV protons on a sandwich of material are presented. The good agreement with the Monte Carlo code shows that the solution method is robust and useful for approximate solutions of selected proton transport problems.

  1. A High-Order Finite-Volume Algorithm for Fokker-Planck Collisions in Magnetized Plasmas

    SciTech Connect (OSTI)

    Xiong, Z; Cohen, R H; Rognlien, T D; Xu, X Q

    2007-04-18

    A high-order finite volume algorithm is developed for the Fokker-Planck Operator (FPO) describing Coulomb collisions in strongly magnetized plasmas. The algorithm is based on a general fourth-order reconstruction scheme for an unstructured grid in the velocity space spanned by parallel velocity and magnetic moment. The method provides density conservation and high-order-accurate evaluation of the FPO independent of the choice of the velocity coordinates. As an example, a linearized FPO in constant-of-motion coordinates, i.e. the total energy and the magnetic moment, is developed using the present algorithm combined with a cut-cell merging procedure. Numerical tests include the Spitzer thermalization problem and the return to isotropy for distributions initialized with velocity space loss cones. Utilization of the method for a nonlinear FPO is straightforward but requires evaluation of the Rosenbluth potentials.

  2. Ion Fokker-Planck simulation of D-{sup 3}He gas target implosions

    SciTech Connect (OSTI)

    Larroche, O. [CEA DIF, Bruyeres le Chatel, 91297 Arpajon Cedex (France)

    2012-12-15

    Recently performed inertial confinement fusion implosion experiments involving D-{sup 3}He gas-filled microballoons have shown discrepancies between expected and measured nuclear fusion yields as the relative abundances of D and {sup 3}He are varied. The latter have been tentatively attributed to a sedimentation, or stratification phenomenon occurring in the target core. This work investigates the possibility of ion species sedimentation in a detailed way through multi-species ion-kinetic Vlasov-Fokker-Planck simulations of the implosion process. A noticeable amount of sedimentation is found to build up during the main shock propagation to the target center, but then disappears as the implosion proceeds. As a result, only the yield of the first burst of neutrons, associated with shock convergence, is appreciably modified, leaving the main neutron production phase during fuel compression and stagnation unaffected. The sedimentation of fuel ion species found, thus, cannot explain the experimental discrepancies.

  3. Monte Carlo implementation of a guiding-center Fokker-Planck kinetic equation

    SciTech Connect (OSTI)

    Hirvijoki, E.; Snicker, A.; Kurki-Suonio, T. [Department of Applied Physics, Aalto University, FI-00076 Aalto (Finland)] [Department of Applied Physics, Aalto University, FI-00076 Aalto (Finland); Brizard, A. [Department of Physics, Saint Michael's College, Colchester, Vermont 05439 (United States)] [Department of Physics, Saint Michael's College, Colchester, Vermont 05439 (United States)

    2013-09-15

    A Monte Carlo method for the collisional guiding-center Fokker-Planck kinetic equation is derived in the five-dimensional guiding-center phase space, where the effects of magnetic drifts due to the background magnetic field nonuniformity are included. It is shown that, in the limit of a homogeneous magnetic field, our guiding-center Monte Carlo collision operator reduces to the guiding-center Monte Carlo Coulomb operator previously derived by Xu and Rosenbluth [Phys. Fluids B 3, 627 (1991)]. Applications of the present work will focus on the collisional transport of energetic ions in complex nonuniform magnetized plasmas in the large mean-free-path (collisionless) limit, where magnetic drifts must be retained.

  4. Max Phase Materials And Coatings For High Temperature Heat Transfer Applications

    SciTech Connect (OSTI)

    Martinez-Rodriguez, M.; Garcia-Diaz, B.; Olson, L.; Fuentes, R.; Sindelar, R.

    2015-10-19

    Molten salts have been used as heat transfer fluids in a variety of applications within proposed Gen IV nuclear designs and in advanced power system such as Concentrating Solar Power (CSP). However, operating at elevated temperatures can cause corrosion in many materials. This work developed coating technologies for MAX phase materials on Haynes-230 and characterized the corrosion of the coatings in the presence of commercial MgCl2-KCl molten salt. Cold spraying of Ti2AlC and physical vapor deposition (PVD) of Ti2AlC or Zr2AlC were tested to determine the most effective form of coating MAX phases on structural substrates. Corrosion testing at 850°C for 100 hrs showed that 3.9 ?m Ti2AlC by PVD was slightly protective while 117 ?m Ti2AlC by cold spray and 3.6 ?m Zr2AlC by PVD were completely protective. None of the tests showed decomposition of the coating (Ti or Zr) into the salt

  5. SRF Institute | Jefferson Lab

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Lab Jefferson Lab's SRF Institute designs, manufactures, assembles and tests SRF technology, such as these niobium cavities, for facilities worldwide. A D D I T I O N A L...

  6. Massachusetts Institute of Technology

    E-Print Network [OSTI]

    ChemE Massachusetts Institute of Technology Department of Chemical Engineering Undergraduate technology, chemical engineers play a role in almost every industry and they collaborate with all types, creating and improving pharmaceuticals, fuels, polymers, plastics, cosmetics, cereals and more." Klavs

  7. Petroleum Institute Scholarly Publications

    E-Print Network [OSTI]

    Abu Dhabi The Petroleum Institute Scholarly Publications 2009 #12 Mechanical Engineering HHaaddii BBeellhhaajj Petroleum Engineering SSaaddoooonn MMoorraadd Petroleum LLaannggiillllee Advanced University Placement Editors' notes: Names in bold in citations indicate Petroleum

  8. Critical Materials Institute

    ScienceCinema (OSTI)

    Alex King

    2013-06-05

    Ames Laboratory Director Alex King talks about the goals of the Critical Materials Institute in diversifying the supply of critical materials, developing substitute materials, developing tools and techniques for recycling critical materials, and forecasting materials needs to avoid future shortages.

  9. INSTITUTE COLLOQUIA AND SEMINARS

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    2-March 31, 2003 2002 April 2 Dr. Bency John, Cyclotron Institute, Texas A&M University Isoscalar Giant Resonances in 12 C April 9 Professor J. Rapaport, Ohio University, Athens,...

  10. PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE

    E-Print Network [OSTI]

    Heller, Barbara

    PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE AND ENGINEERING Strategic Plan Summary #12;Pritzker Institute for Biomedical Science and Engineering for Strategic Plan Summary | 1 PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE AND ENGINEERING STRATEGIC PLAN SUMMARY 1. Grow the student body · Provide financial

  11. American Institute of Aeronautics Astronautics

    E-Print Network [OSTI]

    American Institute of Aeronautics Astronautics Study Cylindrical Thruster Low Power Space scaling of magnetic circuit leaves almost no magnetic Copyright American Institute Aeronautics; American Institute of Aeronautics Astronautics ability coaxial thrusters achieve performance moderate power

  12. Min-max control design for large angle maneuvers of flexible spacecraft 

    E-Print Network [OSTI]

    Kim, Cheolho

    1991-01-01

    ( ber) gP Shankar P. Bhattacharyy (Member) Srinivas R. Vadali (Member) /Ye~- gc'g Walter E. Haisler (Head of Department) December 1991 ABSTRACT Min-Max Control Design for Large Angle Maneuvers of Flexible Spacecraft(December 1991) Cheolho I...] ? S] C2 6, (2, 1. 10) 03 C]S2C3 + S3S] C]S2S] + C3S] C]C2 63 where C, = cos8, and S, = sin8, . Hence, o] = d];6, = (C2C3)61+ ( ? C2S3)62+ (S3)63 (2, 1. 11) For the convenience of notation, the permutation symbol e03 is used. 1 e;ic = 0 ? 1...

  13. Boride-based nano-laminates with MAX-phase-like behaviour

    SciTech Connect (OSTI)

    Telle, Rainer . E-mail: telle@ghi.rwth-aachen.de; Momozawa, Ai; Music, Denis; Schneider, Jochen M.

    2006-09-15

    MAX-phases being usually composed of transition metals, group A elements and carbon/nitrogen are considered interesting materials for many applications because of their tremendous bulk modulus, 'reversible' plasticity, and machinability. This is mainly due to their unique kind of bonding comprising covalent, ionic as well as metallic bonds providing 'easy' planes of rupture and deformability due to the layered crystal structures. In transition metal boride systems, similar types of bonding are available. In particular the W{sub 2}B{sub 5}-structure type and its stacking variations allow the synthesis of strongly layered crystal structures exhibiting unique delamination phenomena. The paper presents ab initio calculations showing the similarities of bonding between the ternary carbides and the corresponding ternary or quaternary borides. Formation of boride-based nano-laminates from auxiliary liquid phases, from the melt as well as during sintering and precipitation from supersaturated solid solutions will be discussed by means of SEM and TEM studies. The role of impurities weakening the interlayer bonding will be addressed in particular. The pronounced cleavage parallel to the basal plane gives rise for crack deflection and pull-out mechanisms if the laminates are dispersed in brittle matrices such as boron carbide, silicon carbide or other transition metal borides. - Graphical abstract: Some transition metal borides crystallise in a layered structure of alternating stacks of metal and boron atoms giving rise for strongly anisotropic properties. Their preferred cleavage parallel and the deformability perpendicular to the basal plan are similar to the peculiar mechanical behaviour recently described for MAX-phases. Ab initio calculations of the crystal structure prove the weak bonds between the layers for a variety of borides which can be used to reinforce ceramic materials on a nano-scale level.

  14. Strategies for Achieving Institutional Change

    Broader source: Energy.gov [DOE]

    Many strategies—including those derived from Institutional Change Principles–may be used to effect institutional change in support of energy and sustainability objectives.

  15. Los Alamos National Laboratory Institutes

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Consortium consists of the University of New Mexico, New Mexico State University, and New Mexico Tech. The Engineering Institute Information Science and Technology Institute...

  16. Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

    E-Print Network [OSTI]

    Ade, P A R; Alves, M I R; Arnaud, M; Arzoumanian, D; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benoît, A; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bock, J J; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bracco, A; Burigana, C; Calabrese, E; Cardoso, J -F; Catalano, A; Chiang, H C; Christensen, P R; Colombo, L P L; Combet, C; Couchot, F; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Dickinson, C; Diego, J M; Dole, H; Donzelli, S; Doré, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Falgarone, E; Ferrière, K; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Gjerløw, E; González-Nuevo, J; Górski, K M; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Guillet, V; Harrison, D L; Helou, G; Henrot-Versillé, S; Hernández-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Holmes, W A; Hornstrup, A; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; Levrier, F; Liguori, M; Lilje, P B; Linden-Vørnle, M; López-Caniego, M; Lubin, P M; Macías-Pérez, J F; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, P G; Martínez-González, E; Masi, S; Matarrese, S; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Miville-Deschênes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Netterfield, C B; Noviello, F; Novikov, D; Novikov, I; Oppermann, N; Oxborrow, C A; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Perotto, L; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Pratt, G W; Prunet, S; Puget, J -L; Rachen, J P; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rossetti, M; Roudier, G; Rubiño-Martín, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Soler, J D; Stolyarov, V; Sudiwala, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; Ysard, N; Yvon, D; Zonca, A

    2015-01-01

    Within ten nearby (d projected on the plane of sky, inferred from the polarized thermal emission of Galactic dust observed by Planck at 353 GHz, and the gas column density structures, quantified by the gradient of the column density, $N_H$. The relative orientation is evaluated pixel by pixel and analyzed in bins of column density using the novel statistical tool Histogram of Relative Orientations. Within most clouds we find that the relative orientation changes progressively with increasing $N_H$ from preferentially parallel or no preferred orientation to preferentially perpendicular. In simulations of magnetohydrodynamic turbulence in molecular clouds this trend in relative orientation is a signature of Alfv\\'enic or sub-Alfv\\'enic turbulence, implying that the magnetic field is significant for the gas dynamics at the scales probed by Planck. We compare the deduced magnetic field strength w...

  17. Head Tracking for the Oculus Rift Steven M. LaValle1 Anna Yershova1 Max Katsev1 Michael Antonov

    E-Print Network [OSTI]

    LaValle, Steven M.

    maintaining human head orientation using low-cost MEMS sensors. We particularly address gyroscope integrationHead Tracking for the Oculus Rift Steven M. LaValle1 Anna Yershova1 Max Katsev1 Michael Antonov tracking head movement in the Oculus Rift Development Kit, which is the most widely used virtual reality

  18. 5782 IEEE TRANSACTIONS ON SIGNAL PROCESSING, VOL. 55, NO. 12, DECEMBER 2007 Max-SINR ISI/ICI-Shaping Multicarrier

    E-Print Network [OSTI]

    Schniter, Philip

    5782 IEEE TRANSACTIONS ON SIGNAL PROCESSING, VOL. 55, NO. 12, DECEMBER 2007 Max-SINR ISI-symbol/inter-car- rier interference (ISI/ICI) subject to orthogonal or biorthogonal constraints. In doubly dispersive channels, however, complete sup- pression of ISI/ICI is impossible, and the ISI/ICI pattern gener- ated

  19. ITALY DAILY, WEDNESDAY, JULY 25, 2001 PAGE 3 temp min c/f max c/f

    E-Print Network [OSTI]

    Frischer, Bernard

    Hunting for Horace's Humble Home Did the Poet Live as Modestly as He Said He Did? An Archaeological TeamDISCOVER ITALY DAILY, WEDNESDAY, JULY 25, 2001 PAGE 3 Weather temp min c/f max c/f SUNNY PARTLY in his writing than many of his contemporaries, he left clues as to where he made his home. He wrote

  20. In-Depth Look at Ground Source Heat Pumps and Other Electric Loads in Two GreenMax Homes

    SciTech Connect (OSTI)

    Puttagunta, S.; Shapiro, C.

    2012-04-01

    CARB partnered with WPPI Energy to answer key research questions on in-field performance of ground-source heat pumps and LAMELs through extensive field monitoring at two WPPI GreenMax demonstration homes in Wisconsin. These two test home evaluations provided valuable data on the true in-field performance of various building mechanical systems and lighting, appliances, and miscellaneous loads (LAMELs).

  1. DETECTION OF HAIRLINE MANDIBULAR FRACTURE USING MAX-FLOW MIN-CUT AND KOLMOGOROV-SMIRNOV DISTANCE

    E-Print Network [OSTI]

    Bhandarkar, Suchendra "Suchi" M.

    DETECTION OF HAIRLINE MANDIBULAR FRACTURE USING MAX-FLOW MIN-CUT AND KOLMOGOROV-SMIRNOV DISTANCE. ABSTRACT The paper addresses a clinically challenging problem of hairline mandibular fracture detection from Computed Tomography (CT) images. A hairline fracture that has critical clinical importance, can

  2. High-energy asymptotic expansion of the Green function for one-dimensional Fokker-Planck and Schrödinger equations

    E-Print Network [OSTI]

    Toru Miyazawa

    2011-12-26

    A new formalism is presented for high-energy analysis of the Green function for Fokker-Planck and Schr\\"odinger equations in one dimension. Formulas for the asymptotic expansion in powers of the inverse wave number are derived, and conditions for the validity of the expansion are studied through the analysis of the remainder term. The short-time expansion of the Green function is also discussed.

  3. Low-energy asymptotic expansion of the Green function for one-dimensional Fokker-Planck and Schrödinger equations

    E-Print Network [OSTI]

    Toru Miyazawa

    2011-12-26

    We consider Schr\\"odinger equations and Fokker-Planck equations in one dimension, and study the low-energy asymptotic behavior of the Green function using a new method. In this method, the coefficient of the expansion in powers of the wave number can be systematically calculated to arbitrary order, and the behavior of the remainder term can be analyzed on the basis of an expression in terms of transmission and reflection coefficients.

  4. 05 teChnoLogIetranSFer teChnoLogY tranSFer

    E-Print Network [OSTI]

    Falge, Eva

    a central access point to the expertise and patented innovations of the various research institutions and filing patents, as well as in setting up businesses based on technol- ogy developed at a Max Planck einer Patent- anmeldung führt. Seit 1979 wurden ca. 3.600 Erfindungen begleitet und rund 2

  5. Breakthrough Technologies AGRONOMICS1: A New Resource for Arabidopsis

    E-Print Network [OSTI]

    Gent, Universiteit

    Center, ETH Zurich, CH­8092 Zurich, Switzerland (W.G., H.S., L.H.); Department of Molecular Biology, Max Planck Institute for Developmental Biology, D­72076 Tuebingen, Germany (S.R.H., S.L., D.W., G][OA] Hubert Rehrauer, Catharine Aquino, Wilhelm Gruissem, Stefan R. Henz, Pierre Hilson, Sascha Laubinger

  6. Comparative Microbial Genomics group CenterforBiologicalSequenceanalysisDepartmentofSystemsBiology,TechnicalUniversityofDenmark

    E-Print Network [OSTI]

    Ussery, David W.

    Comparative Microbial Genomics group CenterforBiologicalSequenceanalysisDepartmentofSystemsBiology,TechnicalUniversityofDenmark Burkholderia Pan-genomics Dave Ussery Max Planck Institut fur Terrestrial Microbiology Marburg, Germany 26 May, 2008 - or - What can we learn from more than 50 sequenced genomes? #12;Comparative Microbial Genomics

  7. JT-60 Modification Plan for Long Pulse Advanced Tokamak Research

    E-Print Network [OSTI]

    JT-60 Modification Plan for Long Pulse Advanced Tokamak Research Colloquium of Max Planck Institute as one step to DEMO · Advanced tokamak researches · Scientific achievements of JT-60 and its phase Tokamak Commercializa tion pease JT-60 Decision system of prototype reactor Electricity Generation

  8. Theory of Electrical Conductivities of Ferrogels J. P. Huang

    E-Print Network [OSTI]

    Huang, Ji-Ping

    conductivity of a metal-polymer composite should depend on the conductivity of particles, the particle shapeTheory of Electrical Conductivities of Ferrogels J. P. Huang Max Planck Institute for Polymer, while magnetic fields can offer a correction. I. Introduction Conductive polymers1 have received much

  9. CRISSCROSS THROUGH OUR SOLAR SYSTEM

    E-Print Network [OSTI]

    Waliser, Duane E.

    CRISSCROSS THROUGH OUR SOLAR SYSTEM Dawn is the ninth Discovery mission scheduled for funding from Laboratory; German Space Center; Max Planck Institute for Solar System Research; and Italian Space Agency and other objects in outer space A rocky solar system object that is smaller than a planet and orbits

  10. Meeting report: Cirrus and the Earth System

    E-Print Network [OSTI]

    Nowack, Peer

    2015-10-29

    their instruments to high altitudes for in-situ measurements, as has recently been performed with the NASA Global Hawk UAV as part of the Airborne Tropical Tropopause Experiment (ATTREX) campaign. Stephan Borrmann (Max-Planck-Institute Mainz and the University...

  11. History of Humanities Associate Editors

    E-Print Network [OSTI]

    Mateo, Jill M.

    History of Humanities Associate Editors Rick Altman, Film Studies, University of Iowa Carolyn History of Science and Humanities, Utrecht University David Cram, History of Linguistics, University, Max Planck Institute for the History of Science Caroline van Eck, Art and Architecture, Leiden

  12. Ion Storage Ring Measurements of Dielectronic Recombination for Astrophysically Relevant Feq+ Ions

    E-Print Network [OSTI]

    Savin, Daniel Wolf

    Ion Storage Ring Measurements of Dielectronic Recombination for Astrophysically Relevant Feq+ Ions. Using the heavy- ion storage ring at the Max-Planck-Institute for Nuclear Physics in Heidelberg, Germany. Measurements are underway for other charge states of iron. INTRODUCTION Heavy-ion storage rings, coupled

  13. Ocean losing ability to `soak up' CO2 New research by UEA provides the first evidence

    E-Print Network [OSTI]

    Feigon, Brooke

    Ocean losing ability to `soak up' CO2 New research by UEA provides the first evidence that recent climate change has weakened one of the Earth's natural carbon `sinks'. Published in the journal Science, the four-year study by scientists from UEA, British Antarctic Survey (BAS) and the Max-Planck Institute

  14. (Sub)mm Interferometry Applications in Star Formation Research

    E-Print Network [OSTI]

    Beuther, Henrik

    (Sub)mm Interferometry Applications in Star Formation Research H. Beuther1 Max-Planck Institute for Astronomy, K¨onigstuhl 17, 69117 Heidelberg, Germany beuther@mpia.de Abstract. Interferometry at (sub)mm structure e.g. details of accretion disks or molecular outflows and the sub(mm) wavelength bands

  15. VOLUME 86, NUMBER 10 P H Y S I C A L R E V I E W L E T T E R S 5 MARCH 2001 Quantum Computing of Quantum Chaos and Imperfection Effects

    E-Print Network [OSTI]

    Shepelyansky, Dima

    of Quantum Chaos and Imperfection Effects Pil Hun Song1 and Dima L. Shepelyansky2 1 Max-Planck-Institut für model in the regime of quantum chaos. It is shown that there are two types of physical characteristics of imperfection effects we analyze in this paper their influence on a quantum compu- tation of quantum chaos

  16. Name: Steve Marschner Title: Associate Professor

    E-Print Network [OSTI]

    Keinan, Alon

    to the Cornell High Energy Synchrotron Source (CHESS) Users meeting 2008. · "Rendering Materials with Complex 3D Optics of Entertainment: Computing the appearance of everyday materials for the movies," invited talk Structure", MaxPlanck Institute for Informatics, Saarbruecken, Germany, June 2008. · "Modeling

  17. A search for circumstellar dust disks with ADONIS O. Schutz1, H. Bohnhardt1, E. Pantin2, M. Sterzik3,

    E-Print Network [OSTI]

    Hahn, Joseph M.

    . Sterzik3, S. Els4, J. Hahn5, and Th. Henning1 1 Max-Planck-Institut f¨ur Astronomie, K¨onigstuhl 17, D (Beckwith, Henning, & Nakagawa 2000). The final stages of this process remain to be charac- terised structures which can be at- tributed to its tidal interaction with disk material (Liou & Zook 1999

  18. 2012 Landes Bioscience. Do not distribute.

    E-Print Network [OSTI]

    Jackson, David

    , Austria; 2 Max Planck Institute of Molecular Plant Physiology; Golm, Germany; 3 Cold Spring Harbor Laboratories; Cold Spring Harbor, NY USA Keywords: chaperonins, homeodomain, plasmodesmata, intercellular in a genetic screen for factors interfering with transport of KN1 fusion proteins. A gene named CHAPERONIN

  19. The Inverse Effect of Annual-Mean State and Annual-Cycle Changes on ENSO SOON-IL AN,* YOO-GEUN HAM,1 JONG-SEONG KUG,# AXEL TIMMERMANN,@

    E-Print Network [OSTI]

    Kang, In-Sik

    circulation model (CGCM) ECHAM5/Max Planck Institute Ocean Model (MPI-OM1). In a green- house warming, especially the surface warming in the western Pacific and the thermocline deepening in the central Pacific the annual-cycle amplitude, and vice versa. The western Pacific warming acts to reduce air­sea coupling

  20. Atmos. Chem. Phys., 3, 13011336, 2003 www.atmos-chem-phys.org/acp/3/1301/ Atmospheric

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    Research, Private Bag No. 1, Aspendale 3195, Australia 6Cape Grim Baseline Air Pollution Station, 15913 1Air Chemistry Department, Max-Planck Institute of Chemistry, P.O. Box 3060, 55020 Mainz, Germany Dufferin Street, Toronto, Ont. M3H 5T4, Canada 9Department of Oceanography, University of Hawaii, 1000 Pope

  1. Interactive Data Mining Considered Harmful (If Done Wrong)

    E-Print Network [OSTI]

    Waldmann, Uwe

    Interactive Data Mining Considered Harmful (If Done Wrong) Pauli Miettinen Max-Planck-Institut für Informatik Saarbrücken, Germany pauli.miettinen@mpi-inf.mpg.de ABSTRACT Interactive data mining can, there is a serious risk that the user of powerful interactive data mining tools will only find the results she

  2. ClimateCarbon Cycle Feedback Analysis: Results from the C4 Model Intercomparison

    E-Print Network [OSTI]

    Zeng, Ning

    . MATTHEWS,g,n T. RADDATZ,o P. RAYNER,a C. REICK,o E. ROECKNER,p K.-G. SCHNITZLER,p R. SCHNUR,p K. STRASSMANN, Canada h University of California, Berkeley, Berkeley, California i Lawrence Livermore National, Boulder, Colorado n University of Calgary, Calgary, Alberta, Canada o Max Planck Institute

  3. Mathematical Biology 3 Jurgen Jost

    E-Print Network [OSTI]

    Arnold, Anton

    Mathematical Biology 3 J¨urgen Jost Max Planck Institute for Mathematics in the Sciences Leipzig, Germany Mathematical Biology 3 ­ p. 1 #12;Biological networks In biology, we find many examples of interacting elements: Mathematical Biology 3 ­ p. 2 #12;Biological networks In biology, we find many examples

  4. Potential of metabolomics as a functional genomics tool

    E-Print Network [OSTI]

    Wurtele, Eve Syrkin

    Potential of metabolomics as a functional genomics tool Raoul J. Bino1,2,3 , Robert D. Hall2 3 Centre for BioSystems Genomics, POB 98, 6700 AB Wageningen, The Netherlands 4 Max-Planck Institute Australian Centre for Plant Functional Genomics, School of Botany, University of Melbourne, Victoria 3010

  5. Intermittency of plasma edge fluctuation data: Multifractal analysis B. A. Carreras and V. E. Lynch

    E-Print Network [OSTI]

    van Milligen, Boudewijn

    , University of Alaska, Fairbanks, Alaska R. Balbi´n Asociacio´n Euratom-Ciemat, 28040 Madrid, Spain J. Bleuel Asociacio´n Euratom-Ciemat, 28040 Madrid, Spain M. Endler Max-Planck-Institut fu¨r Plasmaphysik, Euratom Association, 85740 Garching, Germany B. van Milligen and E. Sa´nchez Asociacio´n Euratom-Ciemat, 28040 Madrid

  6. Exploiting Correlated Keywords to Improve Approximate Information Filtering

    E-Print Network [OSTI]

    Tryfonopoulos, Christos

    , Christos Tryfonopoulos, and Gerhard Weikum Databases and Information Systems Department Max-Planck Institut- scribe to information sources and be notified whenever new documents of interest are published. In approximate infor- mation filtering only selected information sources, that are likely to publish documents

  7. Perceiving translucent materials Roland W. Fleming1

    E-Print Network [OSTI]

    simple candidate sources of information fail to predict how translucent an object looks. We suggest: the relevant stimulus information remains to be discovered. CR Categories: J.4 [Computer Application]: Social Max Planck Institute for Biological Cybernetics. 2 Computer Graphics Laboratory, UCSD. Abstract Many

  8. Pure recoil corrections to hydrogen energy levels. Krzysztof Pachucki

    E-Print Network [OSTI]

    Pachucki, Krzysztof

    Pure recoil corrections to hydrogen energy levels. Krzysztof Pachucki Max--Planck--Institut F approximation for the hydrogenic energy levels we can assume that the mass of the nucleus is infinite, vacuum polarization, etc. For the precise determination of hydrogenic energy levels we have to include

  9. Complete mergeability and amodal completion Peter Ulric Tse 1

    E-Print Network [OSTI]

    Bucci, David J.

    Complete mergeability and amodal completion Peter Ulric Tse 1 Max Planck Institut fuer Biologische portions of a single occluded object, the object is said to `amodally complete' behind the occluder of such image fragments subtend an obtuse or right angle, the contours are `relatable' and therefore complete

  10. Carl von Ossietzky Universitt Oldenburg Fachbereich Physik, 26111 Oldenburg

    E-Print Network [OSTI]

    Oldenburg, Carl von Ossietzky Universität

    Explosionen massereicher Sterne E. Hilf ISN 27.5.2002 Prof. Dr. Klaus Hasselmann Max-Planck-Institut für Anwendungen in der Medizin Klaus Hinsch AOP 24.6.2002 PD Dr.. Heinz-Peter Breuer Universität Freiburg, zur Funktion der Größe G. Bauer, R. Brüggemann GRECO Ort: Carl von Ossietzky Universität Oldenburg; Zeit

  11. The Supermassive Black Hole at the Galactic Center

    E-Print Network [OSTI]

    Falcke, Heino

    Observatory, The University of Arizona, Tucson, AZ 85721 Heino Falcke Max-Planck-Institut fur Radioastronomie WIND CAPTURE : : : : : : : : : : : : : : : 18 1 Sir Thomas Lyle Fellow and Miegunyah Fellow. #12; Annu dusty ring, ionized gas streamers, di#11;use hot gas, and a powerful supernova-like remnant. Many

  12. SemeSterkalender Sommer 2013

    E-Print Network [OSTI]

    Heermann, Dieter W.

    SemeSterkalender Sommer 2013 Studium Generale #12;impreSSum Herausgeber: der rektor der universität Inhaltsverzeichnis Studium Generale 4/5 #12;evolUtIon verStehen Studium Generale · SOmmerSemeSter 2013 montag, 6. mai vielfalt und komplexität prof. dr. ralf J. Sommer, max-planck-institut für entwicklungsbiologie, tübingen

  13. 78. Funding for this work came from the NHGRI of the NIH as part of the modENCODE project, NIH (grant

    E-Print Network [OSTI]

    Will, Sebastian

    .K.K.); the Helmholtz-Alliance on Systems Biology (Max Delbrück Centrum Systems Biology Network) (S.D.M.); the Wellcome Planck Institute of Molecular Cell Biology and Genetics. Raw microarray data are available from the Gene into cellular and developmental programs, the Drosophila model organism Encyclopedia of DNA Elements (mod

  14. Learning to navigate: experience versus maps Tobias Meilinger a,b,

    E-Print Network [OSTI]

    H. Bülthoff a,d a Max-Planck-Institute for Biological Cybernetics, Spemannstr. 38, 72076 Tübingen, Germany b Research Center for Advanced Science and Technology, The University of Tokyo, 4-6- 1 Komaba Research Center for Advanced Science and Technology, The University of Tokyo 4-6-1 Komaba, Meguro-ku Tokyo

  15. ACCEPTED VERSION, IEEE TRANS. ON SYSTEMS, MAN, AND CYBERNETICS, PART B: CYBERNETICS. FINAL PUBLICATION AVAILABLE AT IEEEXPLORE.IEEE.ORG 1 Human-Centered Design and Evaluation of Haptic

    E-Print Network [OSTI]

    ACCEPTED VERSION, IEEE TRANS. ON SYSTEMS, MAN, AND CYBERNETICS, PART B: CYBERNETICS. FINAL and Technology through the National Research Foundation of Korea (R31-10008), and a Korea Research Foundation. Robuffo Giordano are with the Max Planck Institute for Biological Cybernetics, Spemannstraße 38, 72076 T

  16. Geometric Analysis of Hilbert-Schmidt Independence Criterion Based ICA Contrast Function

    E-Print Network [OSTI]

    McAuliffe, Jon

    Engineering and Complex Systems Research Program, National ICT Australia , Canberra ACT 2601, Australia and Department of Information Engineering, Research School of Information Science and Engineering, The Australian and Perception, Max Planck Institute for Biological Cybernetics, 72076 T¨ubingen, Germany Hao

  17. Novel Technologies for a Personal Air Transport System Heinrich H. Blthoff

    E-Print Network [OSTI]

    for Biological Cybernetics, Tübingen, Germany www.kyb.mpg.de Department of Brain and Cognitive Engineering Korea department at the Max Planck Institute for Biological Cybernetics in Tübingen and also in my research group in the Biological Cybernetics Lab at Korea University we aim to best model human perception and action and to test

  18. Regine Armann (Ph.D.) Curriculum Vitae

    E-Print Network [OSTI]

    -doctoral Researcher Department of Brain and Cognitive Engineering, Biological Cybernetics Lab, Korea University, Anam) Department of Brain and Cognitive Engineering, Biological Cybernetics Lab, Korea University, (with Prof and Cognitive Engineering, Korea University, and Max Planck Institute for Biological Cybernetics 2011 Co

  19. Giant phonon softening in the pseudogap phase of the quantum spin system TiOCl P. Lemmens,1,2

    E-Print Network [OSTI]

    Leonardo, Degiorgi

    . Choi,3 G. Caimi,4 L. Degiorgi,4,5 N. N. Kovaleva,1 A. Seidel,6 and F. C. Chou6 1Max Planck Institute­1­1, Sendai 980­8577, Japan 4Laboratorium für Festkörperphysik, ETH Zürich, CH-8093 Zürich, Switzerland 5 Paul

  20. Journal of Vision (2001) 1, 88-98 http://journalofvision.org/1/2/3/ 88 Driving in the future: Temporal visuomotor

    E-Print Network [OSTI]

    2001-01-01

    : Temporal visuomotor adaptation and generalization Douglas W. Cunningham Max Planck Institute for Biological, a phenomenon that may be referred to as spatial visuomotor adaptation. Here, we use a high-fidelity driving simulator to demonstrate that the sensorimotor system can adapt to temporal misalignments on very complex

  1. Atmos. Chem. Phys., 7, 973980, 2007 www.atmos-chem-phys.net/7/973/2007/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    Chemistry Department, Max-Planck Institute for Chemistry, J.J. Becher Weg 27, 55020 Mainz, Germany Received to the 150 TgC yr-1 total emissions estimated from all an- thropogenic sources including fossil fuel usage and produce secondary organic aerosol, thereby affecting the Earth's radiation energy bud- get (Seinfeld, 2003

  2. Anomalous magnetic moments of free and bound leptons

    E-Print Network [OSTI]

    Pachucki, Krzysztof

    ]. An almost simultaneous calculation by Schwinger [2] showed how the electron self-interaction explains. Jentschura. Max­Planck­Institut f¨ur Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany. e-mail: Ulrich.Jentschura@mpi-hd.mpg to know this part with the maximum possible accuracy. Schwinger's calculation included a single virtual

  3. The Astrophysical Journal, 640:L155L158, 2006 April 1 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.

    E-Print Network [OSTI]

    Moskalenko, Igor V.

    Max-Planck-Institut fu¨r extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany; aws@mpe.mpg thought of as negligible. However, a new calculation of the interstellar radiation field consistent made a calculation of the attenuation of very high energy g-rays in the Galaxy, using this new

  4. The Astrophysical Journal, 648: L29L32, 2006 September 1 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.

    E-Print Network [OSTI]

    Moskalenko, Igor V.

    . Strong Max-Planck-Institut fu¨r extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany; aws@mpe.mpg calculations to the supernova remnants RX J1713.7 3946 and G0.9 0.1, recently observed by HESS. Subject. INTRODUCTION A new calculation (Porter & Strong 2006) of the Galactic interstellar radiation field (ISRF

  5. fur Mathematik in den Naturwissenschaften

    E-Print Network [OSTI]

    Benedikt,1 Alexander A. Auer,1, a) Mike Espig,2, b) and Wolfgang Hackbusch2 1) Max-Planck-Institut for Iron processing11,12 , computer vision13­15 , data mining16­18 , neuroscience19,20 and many more. The advantage

  6. Remote Sensing of Changing Cryosphere, LandIce and Snow -Workshop of the European Association of Remote Sensing Laboratories (EARSeL),

    E-Print Network [OSTI]

    Zahn, Matthias

    Remote Sensing of Changing Cryosphere, LandIce and Snow - Workshop of the European Association of Remote Sensing Laboratories (EARSeL), Bern, Switzerland, 11-13 February 2008 Page 1 Potential and limits Max-Planck Institute of Meteorology, Germany #12;Remote Sensing of Changing Cryosphere, Land

  7. Electrophoresis of colloidal dispersions in the low-salt regime Vladimir Lobaskin,1, 2

    E-Print Network [OSTI]

    Dünweg, Burkhard

    ¨unweg,1 Martin Medebach,3 Thomas Palberg,3 and Christian Holm1, 4 1 Max Planck Institute for Polymer the de- tails of the static and dynamic behavior are the result of the interplay between electrostatic, and the solvent hydrody- namics. Depending on whether the concentration of the background electrolyte (relative

  8. RAPID COMMUNICATIONS PHYSICAL REVIEW E 87, 051001(R) (2013)

    E-Print Network [OSTI]

    Dünweg, Burkhard

    2013-01-01

    1 Max Planck Institute for Polymer Research, Ackermannweg 10, 55128 Mainz, Germany 2 Department fluorescence cross-correlation spectroscopy with Brownian dynamics simulations, we were able to measure analyzed the flow of aqueous electrolytes over glass coated with a layer of poly

  9. Ann. Geophys., 26, 23712382, 2008 www.ann-geophys.net/26/2371/2008/

    E-Print Network [OSTI]

    Bergen, Universitetet i

    for the energy transfer from the solar wind into the magnetosphere. The location of the dayside reconnection line. Puhl-Quinn4, and C. Kletzing5 1Max-Planck-Institut f¨ur extraterrestrische Physik, Garching, Germany 2Department of Physics, University of Bergen, Norway 3GeoForschungsZentrum Potsdam, Potsdam, Germany 4

  10. Atmos. Chem. Phys., 11, 97099719, 2011 www.atmos-chem-phys.net/11/9709/2011/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    University Centre for Environment, P.O. Box 27, University of Helsinki, 00014, Finland 3Wind Energy Division, Risø National Laboratory for Sustainable Energy, Technical University of Denmark, Building 118, Box 49, 4000, Roskilde, Denmark 4Max Planck Institute of Chemistry, J. Becher Weg 27, 55128 Mainz, Germany 5

  11. Interplanetary coronal mass ejection influence on high energy pick-up ions at Venus

    E-Print Network [OSTI]

    California at Berkeley, University of

    -up ions to higher energies at lower altitudes compared to undisturbed solar wind. HoweverInterplanetary coronal mass ejection influence on high energy pick-up ions at Venus T.R. McEnulty a Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany a r t i c l e i n f o

  12. Atmos. Chem. Phys., 12, 19231950, 2012 www.atmos-chem-phys.net/12/1923/2012/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    , 95440 Bayreuth, Germany *now at: T ¨UV S¨ud Industrie Service GmbH Wind Cert Services, Ludwig and exchange of energy and reactive and non-reactive trace gases at a forest site ­ results of the EGER, 95440 Bayreuth, Germany 2Max-Planck-Institute of Chemistry, Biogeochemistry Department, P.O. Box 3060

  13. The Central Parsecs of the Galaxy ASP Conference Series, Vol. 186, 1999

    E-Print Network [OSTI]

    Falcke, Heino

    . Alternatively, one can think of a jet plus wind model (EDAF), where most of the energy goes out without being, Romania 2 Max Planck Institute of Radioastronomy, Auf dem H¨ugel, 69, Bonn, Germany Abstract. We dissipated in the disk. The model resembles the ADAF model at small radii. At large radii the energy

  14. Available online at www.sciencedirect.com The early ontogeny of humanedog communication

    E-Print Network [OSTI]

    Indiana University

    Psychology, Max Planck Institute for Evolutionary Anthropology (Received 12 January 2007; initial acceptance 2 March 2007; final acceptance 28 August 2007; published online 8 November 2007; MS. number: 9231R the flexibility of the puppies' understanding by reducing the degree to which they could use local enhancement

  15. Aging and Gene Expression in the Primate Hunter B. Fraser1*

    E-Print Network [OSTI]

    Khaitovich, Philipp

    of California, Berkeley, California, United States of America, 2 Max-Planck-Institute for Evolutionary, Berkeley, California, United States of America It is well established that gene expression levels in many Anthropology, Leipzig, Germany, 3 Society of Fellows, Harvard University, Cambridge, Massachusetts, United

  16. CERN-INTC-2014-021/INTC-SR-034 EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH

    E-Print Network [OSTI]

    . Wolf1,11 , K. Zuber12 1Max Planck Institute for Nuclear Physics, Heidelberg, Germany 2Uppsala University, Department of Physics, Istanbul, Turkey 5University of Manchester, Manchester, United Kingdom 6GSI Helmholtzzentrum f¨ur Schwerionenforschung GmbH, Darmstadt, Germany 7FAIR GmbH, Darmstadt, Germany

  17. CERN-INTC-2014-038/INTC-P-410 EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH

    E-Print Network [OSTI]

    12 , R. N. Wolf11 , K. Zuber12 1 Max Planck Institute for Nuclear Physics, Heidelberg, Germany 2 of Physics, Istanbul, Turkey 6 University of Manchester, Manchester, United Kingdom 7 Petersburg NuclearH, Darmstadt, Germany 9 FAIR GmbH, Darmstadt, Germany 10 CSNSM-IN2P3-CNRS, Université Paris-Sud, Orsay, France

  18. CERN-INTC-2011-053/INTC-P-317 EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH

    E-Print Network [OSTI]

    . N. Wolf8 , K. Zuber9 1Max Planck Institute for Nuclear Physics, Heidelberg, Germany 2GSI Helmholtzzentrum f¨ur Schwerionenforschung GmbH, Darmstadt, Germany 3IKS Leuven, Belgium 4Department of Physics, University of Istanbul, Istanbul, Turkey 5CERN, Geneva, Switzerland 6CSNSM-IN2P3-CNRS, Universit´e de Paris

  19. The 2005 PASCAL Visual Object Classes Mark Everingham1

    E-Print Network [OSTI]

    Everingham, Mark

    University, Aachen, Germany. 5 TU-Darmstadt, Darmstadt, Germany. 6 France T´el´ecom, Cesson S´evign´e, France Middle East Technical University, Ankara, Turkey. 10 Microsoft Research, Cambridge, UK. 11 Max Planck Institute for Biological Cybernetics, T¨ubingen, Germany. 12 University of Southampton, Southampton, UK

  20. CERN-INTC-2014-024/INTC-P-317-ADD-1 EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH

    E-Print Network [OSTI]

    H, Darmstadt, Germany 2Max Planck Institute for Nuclear Physics, Heidelberg, Germany 3Uppsala University, Department of Physics, Istanbul, Turkey 6CERN, Geneva, Switzerland 7CSNSM-IN2P3-CNRS, Universit´e Paris-Sud, Orsay, France 8Ernst-Moritz-Arndt-University, Greifswald, Germany 9Technical University, Dresden

  1. Prepared for the U.S. Department of Energy under Contract DE-AC02-76CH03073. Princeton Plasma Physics Laboratory

    E-Print Network [OSTI]

    Energy Res. Inst., Naka, JAPAN 13 Max-Planck Institut fur Plasmaphysik, Garching, GERMANY 14 A.F. IoffePrepared for the U.S. Department of Energy under Contract DE-AC02-76CH03073. Princeton Plasma This report is posted on the U.S. Department of Energy's Princeton Plasma Physics Laboratory Publications

  2. Theresa Johnson, PhD PhD Candidate

    E-Print Network [OSTI]

    Lin, Xi

    campaign in collaboration with the Max Planck Institut fur Kernphysik in Heidelberg, Germany, and led worked on aerospace projects in UAVs, high altitude wind energy, robotics, balloon-based internet access massive than previously observed. The EMP production is the result of the growth of the unstable Weibel

  3. Supplement to: The CO2 release and Oxygen uptake from Fossil Fuel Emission

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    Consumption for non-energy uses F80 Fossil fuel use: Oil production, transmission and handling, gas flaring , C. Minejima2,4 , H. Mukai2 1 Max Planck Institute for Biogeochemistry, Jena, Germany 2 Center to observations at the station Ochsenkopf in Germany. #12;EDGAR 3.2 usage type Corresponding UN usage type(s) code

  4. Increased stray gas abundance in a subset of drinking water wells near Marcellus shale gas extraction

    E-Print Network [OSTI]

    Jackson, Robert B.

    are transforming energy production, but their potential environmental effects remain contro- versial. We analyzed 91768 Edited by Susan E. Trumbore, Max Planck Institute for Biogeochemistry, Jena, Germany, and approved fingerprinting | fracking | hydrology and ecology Unconventional sources of gas and oil are transforming energy

  5. original article The new england journal of medicine

    E-Print Network [OSTI]

    Hoehe, Margret

    .-U.L.); and the Max Planck Institute for Molecular Genetics, Berlin, Germany (M.R.H.). Address reprint requests to Dr Sedentary life- styles,high-fat,energy and triggers the production of a melanocyte-stimulating hor- mone by means of proopiomelanocortin (POMC

  6. Geosci. Model Dev., 8, 4349, 2015 www.geosci-model-dev.net/8/43/2015/

    E-Print Network [OSTI]

    Robock, Alan

    Research, Boulder, Colorado, USA 2Max Planck Institute for Meteorology, Hamburg, Germany 3Department and regional temperature and precipitation, the energy budget, sea ice, climate extremes, and crop pro- duction., 2014), and a re- duction of agricultural production (Xia et al., 2014). Further, SRM reduces extreme

  7. January 2008 EPL, 81 (2008) 20005 www.epljournal.org

    E-Print Network [OSTI]

    Wohrer, Adrien

    2008-01-01

    'Ulm, 75005 Paris, France 2 Max Planck Institute for Mathematics in the Sciences - Inselstr. 22, 04103 Leipzig numerically investigate an approximate basin of attraction, A, of the periodic orbit and use Markov process terminates the firing by taking it out of the basin of attraction of the stable limit cycle. Stronger noise

  8. Synchronized vehicle motion recording and playback

    E-Print Network [OSTI]

    -Rec: Battery and hard disk 25/06/2014 (c) 2014 - Max Planck Institute for Biological Cybernetics 10 · Large battery: ­ Longex 12LC-150 ­ 12V ­ 160Ah ­ ~4-5 hours operation · Small battery: ­ VARTA LAD85 ­ 12V ­ 85-Rec: Data flow INS Video Audio RAW INS files RAW Video files start/stop/reset warnings/errors RECORDING

  9. Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies

    E-Print Network [OSTI]

    Bianchini, Federico; Calabrese, Matteo; Bielewicz, Pawel; Gonzalez-Nuevo, Joaquin; Baccigalupi, Carlo; Danese, Luigi; de Zotti, Gianfranco; Bourne, Nathan; Cooray, Asantha; Dunne, Loretta; Eales, Stephen

    2015-01-01

    We present an improved and extended analysis of the cross-correlation between the map of the Cosmic Microwave Background (CMB) lensing potential derived from the Planck mission data and the high-redshift galaxies detected by the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) in the photometric redshift range $z_{\\rm ph} \\ge 1.5$. We compare the results based on the 2013 and 2015 Planck datasets, and investigate the impact of different selections of the H-ATLAS galaxy samples. Significant improvements over our previous analysis have been achieved thanks to the higher signal-to-noise ratio of the new CMB lensing map recently released by the Planck collaboration. The effective galaxy bias parameter, $b$, for the full galaxy sample, derived from a joint analysis of the cross-power spectrum and of the galaxy auto-power spectrum is found to be $b = 3.54^{+0.15}_{-0.14}$. Furthermore, a first tomographic analysis of the cross-correlation signal is implemented, by splitting the galaxy sample into two re...

  10. Constraining models of f(R) gravity with Planck and WiggleZ power spectrum data

    SciTech Connect (OSTI)

    Dossett, Jason; Parkinson, David; Hu, Bin E-mail: hu@lorentz.leidenuniv.nl

    2014-03-01

    In order to explain cosmic acceleration without invoking ''dark'' physics, we consider f(R) modified gravity models, which replace the standard Einstein-Hilbert action in General Relativity with a higher derivative theory. We use data from the WiggleZ Dark Energy survey to probe the formation of structure on large scales which can place tight constraints on these models. We combine the large-scale structure data with measurements of the cosmic microwave background from the Planck surveyor. After parameterizing the modification of the action using the Compton wavelength parameter B{sub 0}, we constrain this parameter using ISiTGR, assuming an initial non-informative log prior probability distribution of this cross-over scale. We find that the addition of the WiggleZ power spectrum provides the tightest constraints to date on B{sub 0} by an order of magnitude, giving log{sub 10}(B{sub 0}) < ?4.07 at 95% confidence limit. Finally, we test whether the effect of adding the lensing amplitude A{sub Lens} and the sum of the neutrino mass ?m{sub ?} is able to reconcile current tensions present in these parameters, but find f(R) gravity an inadequate explanation.

  11. Importance Sampling Variance Reduction for the Fokker-Planck Rarefied Gas Particle Method

    E-Print Network [OSTI]

    Collyer, Benjamin; Lockerby, Duncan

    2015-01-01

    Models and methods that are able to accurately and efficiently predict the flows of low-speed rarefied gases are in high demand, due to the increasing ability to manufacture devices at micro and nano scales. One such model and method is a Fokker-Planck approximation to the Boltzmann equation, which can be solved numerically by a stochastic particle method. The stochastic nature of this method leads to noisy estimates of the thermodynamic quantities one wishes to sample when the signal is small in comparison to the thermal velocity of the gas. Recently, Gorji et al have proposed a method which is able to greatly reduce the variance of the estimators, by creating a correlated stochastic process which acts as a control variate for the noisy estimates. However, there are potential difficulties involved when the geometry of the problem is complex, as the method requires the density to be solved for independently. Importance sampling is a variance reduction technique that has already been shown to successfully redu...

  12. Neutrinos help reconcile Planck measurements with both Early and Local Universe

    E-Print Network [OSTI]

    Cora Dvorkin; Mark Wyman; Douglas H. Rudd; Wayne Hu

    2014-09-17

    In light of the recent BICEP2 B-mode polarization detection, which implies a large inflationary tensor-to-scalar ratio r_{0.05}=0.2^{+0.07}_{-0.05}, we re-examine the evidence for an extra sterile massive neutrino, originally invoked to account for the tension between the cosmic microwave background (CMB) temperature power spectrum and local measurements of the expansion rate H0 and cosmological structure. With only the standard active neutrinos and power-law scalar spectra, this detection is in tension with the upper limit of rgravitational waves. An extra sterile species with the same energy density as is needed to reconcile the CMB data with H0 measurements can also alleviate this new tension. By combining data from the Planck and ACT/SPT temperature spectra, WMAP9 polarization, H_0, baryon acoustic oscillation and local cluster abundance measurements with BICEP2 data, we find the joint evidence for a sterile massive neutrino increases to DeltaNeff=0.98\\pm 0.26 for the effective number and ms= 0.52\\pm 0.13 eV for the effective mass or 3.8 sigma and 4 sigma evidence respectively. We caution the reader that these results correspond to a joint statistical evidence and, in addition, astrophysical systematic errors in the clusters and H0 measurements, and small-scale CMB data could weaken our conclusions.

  13. Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors

    E-Print Network [OSTI]

    Wang, Yun

    2015-01-01

    We explore the systematic uncertainties in dark energy constraints using the latest observational data from Type Ia Supernovae (SNe Ia), galaxy clustering, and cosmic microwave background anisotropy (CMB) data. We use the Joint Lightcurve Analysis (JLA) set of 740 SNe Ia, galaxy clustering measurements of H(z)s and D_A(z)/s (where s is the sound horizon at the drag epoch) from the Sloan Digital Sky Survey (SDSS) at z=0.35 (SDSS DR7) and z=0.57 (BOSS DR11), and the distance priors that we have derived from the 2015 Planck data (we present the mean values and covariance matrices required for using these). We find that omitting the BOSS DR11 measurement of H(z)s at z=0.57 leads to more concordant cosmological constraints, indicative of possible systematic uncertainties that affect the measurement of the line-of-sight galaxy clustering. We also find that flux-averaging of SNe Ia at z>= 0.5 gives significantly tighter constraints on dark energy; this can be due to the reduction in the distance measurement bias fro...

  14. Non-local scalar fields inflationary mechanism in light of Planck $2013$

    E-Print Network [OSTI]

    Haidar Sheikhahmadi; Soheyla Ghorbani; Khaled Saaidi

    2015-02-18

    A generalization of the canonical and non-canonical theory of inflation is introduced in which the kinetic energy term in action is written as non-local term. The inflationary universe within the framework of considering this non-locality will be studied. To investigate the effects of non-locality on the inflationary parameters we consider two well known models of inflationary scenario includes of chaotic and exponential inflation proposals. For such scenarios some important parameters include slow roll parameters, scalar and tensor power spectra, spectral indices, the tensor-to-scalar ratio and so on for both mentioned models, chaotic and exponential inflationary scenarios, will be calculated. Also the Hamilton-Jacobi formalism, as an easiest way to study the effect of perturbation based on e-folding number $N$, to investigate inflationary attractors will be used. The free theoretical parameters of this model will be compared with observations by means of Planck $2013$, $WMAP9+eCMB+BAO+H_0$ data sets in addition to $BICEP2$ data surveying. It will be shown that our theoretical results are in acceptable range in comparison to observations. For instance the tensor-to-scalar ratio for exponential potential, by considering $BICEP2$ is in best agreement in comparison with chaotic inflation.

  15. The Knotted Sky I: Planck constraints on the primordial power spectrum

    SciTech Connect (OSTI)

    Aslanyan, Grigor; Price, Layne C.; Easther, Richard [Department of Physics, University of Auckland, Private Bag 92019, Auckland (New Zealand); Abazajian, Kevork N., E-mail: g.aslanyan@auckland.ac.nz, E-mail: lpri691@aucklanduni.ac.nz, E-mail: kevork@uci.edu, E-mail: r.easther@auckland.ac.nz [Department of Physics, University of California at Irvine, Irvine, CA 92697 (United States)

    2014-08-01

    Using the temperature data from Planck we search for departures from a power-law primordial power spectrum, employing Bayesian model-selection and posterior probabilities. We parametrize the spectrum with n knots located at arbitrary values of logk, with both linear and cubic splines. This formulation recovers both slow modulations and sharp transitions in the primordial spectrum. The power spectrum is well-fit by a featureless, power-law at wavenumbers k>10{sup -3} Mpc{sup -1}. A modulated primordial spectrum yields a better fit relative to ?CDM at large scales, but there is no strong evidence for a departure from a power-law spectrum. Moreover, using simulated maps we show that a local feature at k ? 10{sup -3} Mpc{sup -1} can mimic the suppression of large-scale power. With multi-knot spectra we see only small changes in the posterior distributions for the other free parameters in the standard ?CDM universe. Lastly, we investigate whether the hemispherical power asymmetry is explained by independent features in the primordial power spectrum in each ecliptic hemisphere, but find no significant differences between them.

  16. Constraining parameters of effective field theory of inflation from Planck data

    E-Print Network [OSTI]

    Banerjee, Anindya

    2015-01-01

    The Cosmic Microwave Background can provide information regarding physics of the very early universe, more specifically, of the matter-radiation distribution of the inflationary era. Starting from the effective field theory of inflation, we use the Goldstone action to calculate the three point correlation function for the Goldstone field, whose results can be directly applied to the field describing the curvature perturbations around a de Sitter solution for the inflationary era. We then use the data from the recent Planck mission for the parameters $f_{NL}^{equil}$ and $f_{NL}^{orthog}$ which parametrize the size and shape of non-Gaussianities generated in single field models of inflation. Using these known values, we calculate the parameters relevant to our analysis, $f_{NL}^{\\dot{\\pi}^3}$, $f_{NL}^{\\dot{\\pi}(\\partial _i \\pi)^2}$ and the speed of sound $c_s$ which parametrize the non-Gaussianities arising from two different kinds of generalized interactions of the scalar field in question.

  17. Constraining parameters of effective field theory of inflation from Planck data

    E-Print Network [OSTI]

    Anindya Banerjee; Himanshu Khanchandani

    2015-09-01

    The Cosmic Microwave Background can provide information regarding physics of the very early universe, more specifically, of the matter-radiation distribution of the inflationary era. Starting from the effective field theory of inflation, we use the Goldstone action to calculate the three point correlation function for the Goldstone field, whose results can be directly applied to the field describing the curvature perturbations around a de Sitter solution for the inflationary era. We then use the data from the recent Planck mission for the parameters $f_{NL}^{equil}$ and $f_{NL}^{orthog}$ which parametrize the size and shape of non-Gaussianities generated in single field models of inflation. Using these known values, we calculate the parameters relevant to our analysis, $f_{NL}^{\\dot{\\pi}^3}$, $f_{NL}^{\\dot{\\pi}(\\partial _i \\pi)^2}$ and the speed of sound $c_s$ which parametrize the non-Gaussianities arising from two different kinds of generalized interactions of the scalar field in question.

  18. Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps

    E-Print Network [OSTI]

    Adam, R; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benoît, A; Benoit-Lévy, A; Bernard, J -P; Bersanelli, M; Bertincourt, B; Bielewicz, P; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bucher, M; Burigana, C; Calabrese, E; Cardoso, J -F; Catalano, A; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Clements, D L; Colombi, S; Colombo, L P L; Combet, C; Couchot, F; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Désert, F -X; Diego, J M; Dole, H; Donzelli, S; Doré, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, T A; Eriksen, H K; Falgarone, E; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Giraud-Héraud, Y; Gjerløw, E; González-Nuevo, J; Górski, K M; Gratton, S; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versillé, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, T S; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Jeune, M Le; Leahy, J P; Lellouch, E; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vørnle, M; López-Caniego, M; Lubin, P M; Macías-Pérez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Martin, P G; Martínez-González, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschênes, M -A; Moneti, A; Montier, L; Moreno, R; Morgante, G; Mortlock, D; Moss, A; Mottet, S; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nørgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Pratt, G W; Prézeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rusholme, B; Sandri, M; Santos, D; Sauvé, A; Savelainen, M; Savini, G; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Watson, R; Wehus, I K; Yvon, D; Zacchei, A; Zonca, A

    2015-01-01

    This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the 2.5 year full mission include almost five independent full-sky surveys. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To get the best accuracy on the calibration over such a large range, two different photometric calibration schemes have been used. The 545 and 857 GHz data are calibrated using models of planetary atmospheric emission. The lower frequencies (from 100 to 353 GHz) are calibrated using the time-variable cosmological microwave background dipole which we call the orbital dipole. This source of calibration only depends on the satellite velocity with respect to the solar system and permits an independent measurement of the amplitude of the CMB solar dipole (3364.5 +/- 0.8 \\mu K) which is 1\\sigma\\ higher than the WMAP measurement wit...

  19. Planck Scale Physics, Gravi-Weak Unification and the Higgs Inflation

    E-Print Network [OSTI]

    L. V. Laperashvili; H. B. Nielsen; B. G. Sidharth

    2015-04-24

    Starting with a theory of the discrete space-time at the Planck scale, we developed a Gravi-Weak Unification (GWU) - a $Spin(4,4)$-invariant model unified gravity with weak $SU(2)$ gauge and Higgs fields in the visible and invisible sectors of the Universe. Considering the Gravi-Weak symmetry breaking, we showed that the obtained sub-algebras contain the self-dual left-handed gravity in the OW, and the anti-self-dual right-handed gravity in the MW. Finally, at the low energy limit, we have only the Standard Model (SM) and the Einstein-Hilbert's gravity. The Froggatt-Nielsen's prediction of the top-quark and Higgs masses was given in the assumption that there exist two degenerate vacua in the SM. This prediction was improved by the next order calculations. We have developed a model of the Higgs Inflation using the GWU action. According to this inflationary model, a scalar field (inflaton) starts trapped from the "false vacuum" of the Universe at the Higgs field's VEV $v_2 \\sim 10^{18}$ GeV. The interaction between the ordinary and mirror Higgs fields $\\phi$ and $\\widetilde{\\phi}$ generates a Hybrid model by A.~Linde of the Higgs Inflation in our Universe.

  20. Planck Scale Physics, Gravi-Weak Unification and the Higgs Inflation

    E-Print Network [OSTI]

    Laperashvili, L V; Sidharth, B G

    2015-01-01

    Starting with a theory of the discrete space-time at the Planck scale, we developed a Gravi-Weak Unification (GWU) - a $Spin(4,4)$-invariant model unified gravity with weak $SU(2)$ gauge and Higgs fields in the visible and invisible sectors of the Universe. Considering the Gravi-Weak symmetry breaking, we showed that the obtained sub-algebras contain the self-dual left-handed gravity in the OW, and the anti-self-dual right-handed gravity in the MW. Finally, at the low energy limit, we have only the Standard Model (SM) and the Einstein-Hilbert's gravity. The Froggatt-Nielsen's prediction of the top-quark and Higgs masses was given in the assumption that there exist two degenerate vacua in the SM. This prediction was improved by the next order calculations. We have developed a model of the Higgs Inflation using the GWU action. According to this inflationary model, a scalar field (inflaton) starts trapped from the "false vacuum" of the Universe at the Higgs field's VEV $v_2 \\sim 10^{18}$ GeV. The interaction bet...

  1. Institutional Change Basics for Sustainability | Department of...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change Basics for Sustainability Institutional Change Basics for Sustainability Institutional change integrates technology, policy, and behavior to make new...

  2. Resources on Institutional Change for Sustainability | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change Resources on Institutional Change for Sustainability Resources on Institutional Change for Sustainability The Federal Energy Management Program (FEMP)...

  3. Use of Institutional Controls

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2003-04-09

    The Policy ensures that the Department of Energy will use institutional controls in the management of resources, facilities and properties under its control, and in implementing its programmatic responsibilities. Certified 1-28-11. Superseded by Chg 1 (Admin Chg), dated 12-7-15.

  4. Use of Institutional Controls

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2003-04-09

    The Policy ensures that the Department of Energy will use institutional controls in the management of resources, facilities and properties under its control, and in implementing its programmatic responsibilities. Certified 1-28-11. Supersedes DOE P 454.1, dated 4-9-03.

  5. Commitment Institutional Change Principle

    Broader source: Energy.gov [DOE]

    Commitment can be a crucial element that helps federal agencies inject and emphasize sustainability in their organizational culture. Institutions and people change when they have made definite commitments to change, especially when those commitments relate to future conditions. Research shows that explicit commitments improve the rate at which people adopt energy-efficient behaviors.

  6. Multiple equilibria on planet Dune: climatevegetation dynamics on a sandy planet

    E-Print Network [OSTI]

    D'Andrea, Fabio

    Torino, Torino, Italy; 2 International Max Planck Research School on Earth System Modelling, Hamburg.cresto-aleina@zmaw.de $Now at: International Max Planck Research School on Earth System Modelling, H

  7. The 60-month all-sky BAT Survey of AGN and the Anisotropy of...

    Office of Scientific and Technical Information (OSTI)

    Garching, Max Planck Inst., MPE ; Madejski, G.M. ; KIPAC, Menlo Park ; Gehrels, N. ; NASA, Goddard ; Burlon, D. ; Garching, Max Planck Inst., MPE Publication Date: 2012-04-02...

  8. When do stochastic max-plus linear systems have a cycle time ?

    E-Print Network [OSTI]

    Merlet, Glenn

    2007-01-01

    We analyze the asymptotic behavior of the sequence of random variables (x(n, x0))n \\in N defined by x(0, x0) = x0 and x(n+1, x0) = A(n)x(n, x0), where (A(n))n \\in N is a stationary and ergodic sequence of random matrices with entries in the semiring (R \\cup {-\\infinity}, max, +). Such sequences model a large class of discrete event systems, among which timed event graphs, 1-bounded Petri nets, some queuing networks, train or computer networks. We give a necessary condition for 1/n x(n, x0) n \\in N to converge almost-surely, which proves to be sufficient when the A(n) are i.i.d. Moreover, we construct a new example, in which (A(n))n \\in N is strongly mixing, that condition is satisfied, but 1/n x(n, x0) n \\in N do not converge almost-surely.

  9. Institutions or, who does what and why

    E-Print Network [OSTI]

    Handy, Susan L.

    it is infused with value" ­ Philip Selznick #12;Importance of Institutions Institutional characteristics

  10. Massachusetts Institute of Technology MIT Web Survey Service Institutional Research,

    E-Print Network [OSTI]

    Reif, Rafael

    Massachusetts Institute of Technology MIT Web Survey Service Institutional Research, Office.mit.edu/ist/isnews/v21/n02/210210.html 1. Coordination with the MIT Institutional Research & Web Survey Service. The MIT, intended audience, and desired schedule. The Web Survey Service will host certain web surveys

  11. Materials Research Institute 199 Materials Research Institute Building

    E-Print Network [OSTI]

    Lee, Dongwon

    promise to transform the field of materials research in areas such as energy, health, and the environment of Materials Research A New Building for the 21st Century he Materials Research Institute promotes interdisciMaterials Research Institute 199 Materials Research Institute Building The Pennsylvania State

  12. An In-Depth Look at Ground Source Heat Pumps and Other Electric Loads in Two GreenMax Homes

    SciTech Connect (OSTI)

    Puttagunta, Srikanth; Shapiro, Carl

    2012-04-01

    Building America research team Consortium for Advanced Residential Buildings (CARB) partnered with WPPI Energy to answer key research questions on in-field performance of ground-source heat pumps and lighting, appliance, and miscellaneous loads (LAMELs) through extensive field monitoring at two WPPI GreenMax demonstration homes in Wisconsin. These two test home evaluations provided valuable data on the true in-field performance of various building mechanical systems and LAMELs.

  13. Robotics | Breeding Research | Nanotechnology GAME THEORY

    E-Print Network [OSTI]

    where Erlenmeyer flasks and Bunsen burners once stood, a magazine such as MaxPlanckResearch must evolve

  14. 21 SEPTEMBER 2012 VOL 337 SCIENCE www.sciencemag.org1444 NEWS&ANALYSIS

    E-Print Network [OSTI]

    a "cultural pattern" can be detected, says team mem- ber Shannon McPherron, an archaeologist at the Max Planck

  15. Goodlad Institute for Educational Renewal

    E-Print Network [OSTI]

    Matrajt, Graciela

    Goodlad Institute for Educational Renewal Annual Report October 2010 #12; Page | 1 PREFACE The Goodlad Institute for Educational Renewal honors the remarkable. Goodlad initiated a national effort to support educational quality and renewal. Looking beyond high

  16. Institutions G.C. Sciara

    E-Print Network [OSTI]

    Handy, Susan L.

    an institution when it is infused with value" ­ Philip Selznick #12;Why they matter... ·They plan, implement

  17. An SZ/X-ray galaxy cluster model and the X-ray follow-up of the Planck clusters

    E-Print Network [OSTI]

    A. Chamballu; J. G. Bartlett; J. -B. Melin; M. Arnaud

    2008-05-28

    Sunyaev-Zel'dovich (SZ) cluster surveys will become an important cosmological tool over next few years, and it will be essential to relate these new surveys to cluster surveys in other wavebands. We present an empirical model of cluster SZ and X-ray observables constructed to address this question and to motivate, dimension and guide X-ray follow-up of SZ surveys. As an example application of the model, we discuss potential XMM-Newton follow-up of Planck clusters.

  18. Langevin and Fokker-Planck analyses of inhibited molecular passing processes controlling transport and reactivity in nanoporous materials

    SciTech Connect (OSTI)

    Wang, Chi-Jen [Ames Laboratory; Ackerman, David M. [Ames Laboratory; Slowing, Igor I. [Ames Laboratory; Evans, James W. [Ames Laboratory

    2014-07-14

    Inhibited passing of reactant and product molecules within the linear pores of nanoporous catalytic materials strongly reduces reactivity. The dependence of the passing propensity P on pore radius R is analyzed utilizing Langevin dynamics to account for solvent effects. We find that P?(R?Rc)?, where passing is sterically blocked for R?Rc, with ? below the transition state theory value. Deeper insight comes from analysis of the corresponding high-dimensional Fokker-Planck equation, which facilitates an effective small-P approximation, and dimensional reduction enabling utilization of conformal mapping ideas. We analyze passing for spherical molecules and also assess the effect of rotational degrees of freedom for elongated molecules.

  19. Advanced Studies Institute

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room News Publications Traditional Knowledge KiosksAboutHelp &Advanced Simulation andInstitute

  20. INSTITUTE COLLOQUIA AND SEMINARS

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverse (JournalvivoHighHussein KhalilResearch8 IEEEINL5-March 31, 2006INSTITUTE

  1. INSTITUTE OF PHYSICS PUBLISHING

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverse (JournalvivoHighHussein KhalilResearch8 IEEEINL5-March 31, 2006INSTITUTE4

  2. INSTITUTE OF PHYSICS PUBLISHING

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverse (JournalvivoHighHussein KhalilResearch8 IEEEINL5-March 31, 2006INSTITUTE46

  3. Zentrale Angelegenheiten Central Matters

    E-Print Network [OSTI]

    Seite 93Personal Seite 106Tochtergesellschaften Seite 114Organigramm Seite 116Personelle Zusammensetzung Report Max Planck Society 2014 Die Zuschüsse zum Haushalt der Max-Planck-Gesellschaft (MPG and federal states each provide half of the subsidies for the Max Planck Society's budget (MPG Application

  4. Special Publication 800-127 Guide to Securing WiMAX

    E-Print Network [OSTI]

    by providing technical leadership for the nation's measurement and standards infrastructure. ITL develops tests of technical, physical, administrative, and management standards and guidelines for the cost-effective security of the National Institute of Standards and Technology KarenScarfone CyrusTibbs MatthewSexton #12;Guide to Securing

  5. Ectopic expression of a soybean phytase in developing seeds of Glycine max to improve phosphorus availability

    E-Print Network [OSTI]

    Finer, John J.

    (*author for correspondence; e-mail egrabau@vt.edu); 2 Department of Horticulture and Crop Science, OARDC, Physiology, and Weed Science, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, USA., 1989). Similar to other agriculturally important crops, soybean contains 60­80% of total seed P

  6. Institutional Change for Sustainability Case Studies | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change for Sustainability Case Studies Institutional Change for Sustainability Case Studies These case studies show examples of institutional change successfully...

  7. Cyclotron Institute Upgrade Project

    SciTech Connect (OSTI)

    Clark, Henry; Yennello, Sherry; Tribble, Robert

    2014-08-26

    The Cyclotron Institute at Texas A&M University has upgraded its accelerator facilities to extend research capabilities with both stable and radioactive beams. The upgrade is divided into three major tasks: (1) re-commission the K-150 (88”) cyclotron, couple it to existing beam lines to provide intense stable beams into the K-500 experimental areas and use it as a driver to produce radioactive beams; (2) develop light ion and heavy ion guides for stopping radioactive ions created with the K-150 beams; and (3) transport 1+ ions from the ion guides into a charge-breeding electron-cyclotron-resonance ion source (CB-ECR) to produce highly-charged radioactive ions for acceleration in the K-500 cyclotron. When completed, the upgraded facility will provide high-quality re-accelerated secondary beams in a unique energy range in the world.

  8. Tokyo Institute of Technology Tokyo Institute of Technology

    E-Print Network [OSTI]

    Shimodaira, Hidetoshi

    Tokyo Institute of Technology 2004 #12; Tokyo Institute of Technology k O(n-k/2) (Efron et al 1996) 2O(B) (Shimodaira 2002, 2004) O(B) #12; Tokyo Institute of Technology of Technology 1 2 3 4 5 1 2 3 4 5 1 2 3 4 5 1 23 4 5 1 2 3 4 5 1 2 3 4 5 1 2 3 4 5 1 23 4 5 1 2 3 4 5

  9. Georgia Institute of Laboratory Safety

    E-Print Network [OSTI]

    ENVIRONMENTAL HEALTH AND SAFETY POLICY.......................................10 Purpose Institute Council for Environmental Health and Safety (IC.........................................................................................12 Chemical and Environmental Safety Committee (CESC

  10. Fiscal Year 2012 Peer Institution

    E-Print Network [OSTI]

    Fiscal Year 2012 Highlights Peer Institution Comparisons Cost to Students Economic Impact access to the University's audited financial information and openly share how we deploy resources

  11. Continuous Change Institutional Change Principle

    Broader source: Energy.gov [DOE]

    ecause it takes time to establish institutional change, federal agencies need multiyear plans that continuously work to achieve, reinforce, and improve significant and persistent sustainability goals.

  12. Essays in Economics and Institutions

    E-Print Network [OSTI]

    Schihl, Michael Kristjian

    2010-01-01

    to (the New) Institutional Economics . . . . .3.4.2Governance. Journal of Law, Economics, and Organization, 7:Journal of Development Economics, 77(2):341–366, August

  13. Clean Energy Manufacturing Innovation Institute for Composites...

    Office of Environmental Management (EM)

    Clean Energy Manufacturing Innovation Institute for Composites Materials and Structures Clean Energy Manufacturing Innovation Institute for Composites Materials and Structures...

  14. Joint Genome Institute's Automation Approach and History

    E-Print Network [OSTI]

    Roberts, Simon

    2006-01-01

    Joint Genome Institute’s Automation Approach and Historythroughput environment; – automation does not necessarilyissues “Islands of Automation” – modular instruments with

  15. Clean Energy Manufacturing Innovation Institute for Composite...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Clean Energy Manufacturing Innovation Institute for Composite Materials And Structures Webinar Clean Energy Manufacturing Innovation Institute for Composite Materials And...

  16. Southface Energy Institute: Advanced Commercial Buildings Initiative...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Southface Energy Institute: Advanced Commercial Buildings Initiative - 2015 Peer Review Southface Energy Institute: Advanced Commercial Buildings Initiative - 2015 Peer Review...

  17. Integrative Bioengineering Institute

    SciTech Connect (OSTI)

    Eddington, David; Magin,L,Richard; Hetling, John; Cho, Michael

    2009-01-09

    Microfabrication enables many exciting experimental possibilities for medicine and biology that are not attainable through traditional methods. However, in order for microfabricated devices to have an impact they must not only provide a robust solution to a current unmet need, but also be simple enough to seamlessly integrate into standard protocols. Broad dissemination of bioMEMS has been stymied by the common aim of replacing established and well accepted protocols with equally or more complex devices, methods, or materials. The marriage of a complex, difficult to fabricate bioMEMS device with a highly variable biological system is rarely successful. Instead, the design philosophy of my lab aims to leverage a beneficial microscale phenomena (e.g. fast diffusion at the microscale) within a bioMEMS device and adapt to established methods (e.g. multiwell plate cell culture) and demonstrate a new paradigm for the field (adapt instead of replace). In order for the field of bioMEMS to mature beyond novel proof-of-concept demonstrations, researchers must focus on developing systems leveraging these phenomena and integrating into standard labs, which have largely been ignored. Towards this aim, the Integrative Bioengineering Institute has been established.

  18. Navigating Mnoa Institutional Research Website Mnoa Institutional Research Office (MIRO)

    E-Print Network [OSTI]

    ;Surveys #12;FACTS ­ Fast Facts #12;FACTS ­College Navigator #12;Information Sources: MIRO reportsNavigating Mnoa Institutional Research Website Mnoa Institutional Research Office (MIRO) University of information #12;Two Dimensions of Navigation HOME REPORTS RANKINGS SURVEYS FACTS DECISION SUPPORT Fast Facts

  19. SAN FRANCISCO ESTUARY INSTITUTE CONTRIBUTION

    E-Print Network [OSTI]

    SAN FRANCISCO ESTUARY INSTITUTE CONTRIBUTION NO. 548 JANUARY 2008 7770 Pardee Lane, Second floor, Oakland, CA 94621 p: 510-746-7334 (SFEI), f: 510-746-7300, www.sfei.org San Francisco Estuary National Williams San Francisco Estuary Institute In collaboration with San Francisco Estuary partners including

  20. SAN FRANCISCO ESTUARY INSTITUTE CONTRIBUTION

    E-Print Network [OSTI]

    SAN FRANCISCO ESTUARY INSTITUTE CONTRIBUTION NO. 663 APRIL 2012 4911 Central Avenue, Richmond, CA on the Margins of San Francisco Bay Draft Report by Craig Jones Sea Engineering, Inc. Donald Yee Jay A. Davis Lester J. McKee Ben K. Greenfield Aroon R. Melwani Michelle A. Lent San Francisco Estuary Institute #12

  1. Annual Report 20102011 ITS INSTITUTE

    E-Print Network [OSTI]

    Minnesota, University of

    Annual Report 2010­2011 ITS INSTITUTE Human-centered technology to enhance safety and mobility #12 of Minnesota 200 Transportation and Safety Building 511 Washington Ave. S.E. Minneapolis, MN 55455- assist system (DAS) developed by ITS Institute, 2011. ITS staff photo. Nighttime car crash on major

  2. Determine Institutional Change Sustainability Goals

    Broader source: Energy.gov [DOE]

    The first step in the institutional change process is defining your federal agency's sustainability goals. That is, decide what outcomes are desired (or required) over what period of time. Behavioral, organizational, and institutional changes typically are means to achieve desired energy, resource, or greenhouse gas emission outcomes. They are not ends in and of themselves.

  3. April 19, 2011 Smithsonian Institution

    E-Print Network [OSTI]

    Mathis, Wayne N.

    -fuel and hybrid vehicles. The Smithsonian fulfilled the renewable energy goal by purchasing green power from windApril 19, 2011 Smithsonian Institution 2010 Scorecard on Sustainability and Energy Performance Below is the Smithsonian Institution's fiscal year 2010 scorecard on sustainability and energy

  4. Internet Institute University of Oxford

    E-Print Network [OSTI]

    The Oxford Internet Institute University of Oxford #12;A significant proportion of social, economic Science Internet Economics Connectivity, Inclusion and InequalityEducation, Wellbeing and Digital Life Digital Knowledge and Culture #12;The Oxford Internet Institute It's an incredibly exciting time

  5. DATALOGISK INSTITUT, AARHUS UNIVERSITET Det Naturvidenskabelige Fakultet

    E-Print Network [OSTI]

    Brodal, Gerth Stølting

    Datalogi Algoritmer og Datastrukturer 1 (2003-ordning) Antal sider i opgavesættet (incl. forsiden): 12 Algoritmer og Datastrukturer 1 (2003-ordning) Skriftlig prøve Side 2 af 12 sider Skriftlig Eksamen Algoritmer multiple-choice-opgaven som: max 0 , s n · v % (Opgavesættet fortsætter) #12;Eksamen august 2010 Algoritmer

  6. DATALOGISK INSTITUT, AARHUS UNIVERSITET Det Naturvidenskabelige Fakultet

    E-Print Network [OSTI]

    Brodal, Gerth Stølting

    Datalogi Algoritmer og Datastrukturer 1 (2003-ordning) Antal sider i opgavesættet (incl. forsiden): 12 Algoritmer og Datastrukturer 1 (2003-ordning) Skriftlig prøve Side 2 af 12 sider Skriftlig Eksamen Algoritmer multiple-choice-opgaven som: max 0 , s n · v % (Opgavesættet fortsætter) #12;Eksamen marts 2012 Algoritmer

  7. Institut fr Hochfrequenztechnik Technische Universitt Braunschweig

    E-Print Network [OSTI]

    ? commercialised by First Solar Inc. : 500 MW installed 2008 16% efficiency under AM 1.5 1 $/Watt manufacturing cost reached in 2008 complete recycling of Cd-compounds guaranteed 1000 MW production capacity planned in 2009 Bipolar II-VI Solar Cells : one successful example Cu2O/ZnO Solar Cells 1.7% max reported

  8. Performance Assessment Institute-NV

    SciTech Connect (OSTI)

    Lombardo, Joesph

    2012-12-31

    The National Supercomputing Center for Energy and the Environment’s intention is to purchase a multi-purpose computer cluster in support of the Performance Assessment Institute (PA Institute). The PA Institute will serve as a research consortium located in Las Vegas Nevada with membership that includes: national laboratories, universities, industry partners, and domestic and international governments. This center will provide a one-of-a-kind centralized facility for the accumulation of information for use by Institutions of Higher Learning, the U.S. Government, and Regulatory Agencies and approved users. This initiative will enhance and extend High Performance Computing (HPC) resources in Nevada to support critical national and international needs in "scientific confirmation". The PA Institute will be promoted as the leading Modeling, Learning and Research Center worldwide. The program proposes to utilize the existing supercomputing capabilities and alliances of the University of Nevada Las Vegas as a base, and to extend these resource and capabilities through a collaborative relationship with its membership. The PA Institute will provide an academic setting for interactive sharing, learning, mentoring and monitoring of multi-disciplinary performance assessment and performance confirmation information. The role of the PA Institute is to facilitate research, knowledge-increase, and knowledge-sharing among users.

  9. Institutional computing (IC) information session

    SciTech Connect (OSTI)

    Koch, Kenneth R; Lally, Bryan R

    2011-01-19

    The LANL Institutional Computing Program (IC) will host an information session about the current state of unclassified Institutional Computing at Los Alamos, exciting plans for the future, and the current call for proposals for science and engineering projects requiring computing. Program representatives will give short presentations and field questions about the call for proposals and future planned machines, and discuss technical support available to existing and future projects. Los Alamos has started making a serious institutional investment in open computing available to our science projects, and that investment is expected to increase even more.

  10. 2007200777 12121122 TOKYO INSTITUTE OF TECHNOLOGY

    E-Print Network [OSTI]

    2007200777 12121122 #12;06 06 TOKYO INSTITUTE OF TECHNOLOGY 0201 CONTENTS 03 08 09 10 15 17 25 31 33 37 41 0201 08 23 TokyoTech #12;TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY 0403 20 1 5 11 #12;TOKYO INSTITUTE OF TECHNOLOGY TOKYO INSTITUTE OF TECHNOLOGY 0605 4 3 2 5 5 4 3 #12;TOKYO

  11. Multiple Motivations Institutional Change Principle

    Broader source: Energy.gov [DOE]

    The multiple motivations principle suggests that a portfolio approach—rather than a single strategy—may be required to achieve change. Research demonstrates that people and institutions adopt new...

  12. 2nd Edition Institutional Animal

    E-Print Network [OSTI]

    Rau, Don C.

    2nd Edition 2002 Institutional Animal Care and Use Committee Guidebook #12;2nd Edition 2002 ....................................................................... 83 C.1. Fundamental Issues .............................................................. 85 C.2. Agricultural Research............................................... 121 C.3.b. Antibody Production

  13. TRANSMITTAL Florida Institute of Technology

    E-Print Network [OSTI]

    Wood, Stephen L.

    TRANSMITTAL Florida Institute of Technology Department of Marine and Environmental Systems TO: Dr to West Marine for donating the marine coatings and other supplies. Thanks to Bill Bailey for all his.............................................................................................................. 16 4.2. Existing Energy Conversion Systems

  14. Institutional owners and competitive rivalry 

    E-Print Network [OSTI]

    Connelly, Brian Lawrence

    2008-10-10

    stream_source_info Connelly.pdf.txt stream_content_type text/plain stream_size 200734 Content-Encoding UTF-8 stream_name Connelly.pdf.txt Content-Type text/plain; charset=UTF-8 INSTITUTIONAL OWNERS AND COMPETITIVE... Major Subject: Management INSTITUTIONAL OWNERS AND COMPETITIVE RIVALRY A Dissertation by BRIAN L. CONNELLY Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree...

  15. Forschungsbericht 201030 Institut fr Biophysikalische Chemie

    E-Print Network [OSTI]

    Manstein, Dietmar J.

    Forschungsbericht 201030 BIOCHEMIE Institut für Biophysikalische Chemie Direktor: Prof. Dr werden. Ziel der am Institut für Bio- physikalische Chemie durchgeführten Arbeiten ist es ein besseres mit der Arbeitsgruppe von Frau Prof. Dr. Françoise H. Routier (Institut für Zelluläre Chemie) haben

  16. Forschungsbericht 201136 Institut fr Biophysikalische Chemie

    E-Print Network [OSTI]

    Manstein, Dietmar J.

    Forschungsbericht 201136 BIOCHEMIE Institut für Biophysikalische Chemie Direktor: Prof. Dr werden. Ziel der am Institut für Bio- physikalische Chemie durchgeführten Arbeiten ist es ein besseres Arbeitsgruppe von Frau Prof. Dr. Françoise H. Routier (Institut für Zelluläre Chemie) haben wir den

  17. MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY

    E-Print Network [OSTI]

    Poggio, Tomaso

    MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY and CENTER FOR BIOLOGICAL Sciences Massachusetts Institute of Technology Cambridge, MA 02139 y Artificial Intelligence Laboratory Institute of Technology, 1995. This report describes research done partly at the Artificial Intelligence

  18. Institutional Causes of California's Budget Problem

    E-Print Network [OSTI]

    Cain, Bruce E.; Noll, Roger

    2010-01-01

    2, Issue 3 Institutional Causes of California’s BudgetCain and Noll: Institutional Causes of California’s BudgetPolicy Institutional Causes of California’s Budget Problem

  19. Canadian Aeronautics and Space Institute Institut aronautique et spatial du Canada

    E-Print Network [OSTI]

    Zingg, David W.

    Canadian Aeronautics and Space Institute Institut aéronautique et spatial du Canada Patron H CANADIAN AERONAUTICS AND SPACE INSTITUTE ANNOUNCES 2012 SENIOR AWARD HONOUREES Mr. Dave Muir, President of the Canadian Aeronautics and Space Institute for 2012

  20. 1870 VOLUME 58J O U R N A L O F T H E A T M O S P H E R I C S C I E N C E S 2001 American Meteorological Society

    E-Print Network [OSTI]

    Siebesma, Pier

    -Planck-Institut fu¨r Meteorologie, Hamburg, Germany **Instituto Nacional Meteorologia, Madrid, Spain Institute

  1. Randomized min-max optimization: the exact risk of multiple cost levels Algo Car`e, Simone Garatti, Marco C. Campi

    E-Print Network [OSTI]

    Garatti, Simone

    . Our goal is to evaluate the risks associated to the various costs, where the risk associated to a cost. This evaluation characterizes completely the risks associated to the costs, and represents a full-fledged resultRandomized min-max optimization: the exact risk of multiple cost levels Algo Car`e, Simone Garatti

  2. IEEE TRANSACTIONS ON WIRELESS COMMUNICATIONS, VOL. XX, NO. XX, MONTH 2008 1 Redefinition of Max-Min Fairness in Multi-hop Wireless Networks

    E-Print Network [OSTI]

    Jiang, Hai

    . Zhuang is with the Centre for Wireless Com- munications, Department of Electrical and ComputerIEEE TRANSACTIONS ON WIRELESS COMMUNICATIONS, VOL. XX, NO. XX, MONTH 2008 1 Redefinition of Max-Min Fairness in Multi-hop Wireless Networks Ping Wang, Member, IEEE, Hai Jiang, Member, IEEE, Weihua Zhuang

  3. Reprocessing of line FFI-161 of the Brazos-Galveston area using Pro-MAX 2D to evaluate migration techniques 

    E-Print Network [OSTI]

    Fofang, Nicholas Ndeh

    1996-01-01

    ProMAX 2D, a software for the interactive and batch processing of two dimensional seismic data, was used to process approximately 25 km of seismic data from line FFI-161 of the Brazos-Galveston area of the Gulf of Mexico. ...

  4. Renewable Energy Institutional Arrangements for Implementation...

    Open Energy Info (EERE)

    Renewable Energy Institutional Arrangements for Implementation Terms of Reference Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Renewable Energy Institutional...

  5. MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY

    E-Print Network [OSTI]

    Poggio, Tomaso

    MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY and CENTER FOR BIOLOGICAL and Cognitive Sciences and the Artificial Intelligence Laboratory at the Massachusetts Institute of Technology

  6. MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY

    E-Print Network [OSTI]

    Poggio, Tomaso

    MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY and CENTER FOR BIOLOGICAL and the Artificial Intelligence Laboratory of the Massachusetts Institute of Technology. This research was sponsored

  7. DOE - Office of Legacy Management -- Massachusetts Institute...

    Office of Legacy Management (LM)

    Massachusetts Institute of Technology Hood Building - MA 01 FUSRAP Considered Sites Site: MASSACHUSETTS INSTITUTE OF TECHNOLOGY, HOOD BUILDING (MA.01 ) Eliminated from further...

  8. Project Management Institute Highlights Savannah River Nuclear...

    Office of Environmental Management (EM)

    Management Institute Highlights Savannah River Nuclear Solutions in Publication Project Management Institute Highlights Savannah River Nuclear Solutions in Publication February 6,...

  9. Shaoxing Jinggong Mechanical and Electrical Research Institute...

    Open Energy Info (EERE)

    Shaoxing Jinggong Mechanical and Electrical Research Institute Company SJMERI Jump to: navigation, search Name: Shaoxing Jinggong Mechanical and Electrical Research Institute...

  10. Institutional Change Process for Sustainability | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Process for Sustainability Institutional Change Process for Sustainability For establishing institutional change in a federal agency to achieve sustainability or other energy...

  11. Institutional Change for Sustainability | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Institutional Change for Sustainability Institutional Change for Sustainability Motivate Staff to be More Sustainable Motivate Staff to be More Sustainable Learn how making public...

  12. Measure and Evaluate Institutional Change for Sustainability...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Measure and Evaluate Institutional Change for Sustainability Measure and Evaluate Institutional Change for Sustainability Graphic showing 5 gears. They progress from Determine Goal...

  13. Climate Change Science Institute | Clean Energy | ORNL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Climate Change Science Institute SHARE Climate Change Science Institute To advance understanding of the Earth system, describe the consequences of climate change, and evaluate and...

  14. Environmental Justice Activities: Community Leaders' Institute...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Dr. David Satcher speaks at the Community Leaders' Institute at Morehouse School of Medicine in Atlanta, Georgia. Atlanta Community Leaders' Institute Conference Dr. Kathy...

  15. Institutional Change Principles for Fostering Sustainability...

    Office of Environmental Management (EM)

    to achieve institutional change-but they are not the strategies themselves. They are derived from academic literature and inform the framework for achieving institutional change...

  16. THE INSTITUTE FOR SOLID STATE PHYSICS 2006 THE INSTITUTE FOR SOLID STATE PHYSICS 2006

    E-Print Network [OSTI]

    Katsumoto, Shingo

    #12;#12;#12;2 THE INSTITUTE FOR SOLID STATE PHYSICS 2006 #12;3 THE INSTITUTE FOR SOLID STATE PHYSICS 2006 #12;4 THE INSTITUTE FOR SOLID STATE PHYSICS 2006 #12;5 THE INSTITUTE FOR SOLID STATE PHYSICS 2006 #12;6 THE INSTITUTE FOR SOLID STATE PHYSICS 2006 #12;7 THE INSTITUTE FOR SOLID STATE PHYSICS 2006

  17. Power law inflation with a non-minimally coupled scalar field in light of Planck and BICEP2 data: The exact versus slow roll results

    E-Print Network [OSTI]

    Sergio del Campo; Carlos Gonzalez; Ramon Herrera

    2015-01-23

    We study power law inflation in the context of non-minimally coupled to the scalar curvature. We analyze the inflationary solutions under an exact analysis and also in the slow roll approximation. In both solutions, we consider the recent data from Planck and BICEP2 data to constraint the parameter in our model. We find that the slow roll approximation is disfavored in the presence of non-minimal couplings during the power law expansion of the Universe.

  18. A Fokker-Planck-Landau collision equation solver on two-dimensional velocity grid and its application to particle-in-cell simulation

    SciTech Connect (OSTI)

    Yoon, E. S.; Chang, C. S., E-mail: cschang@pppl.gov [Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543 (United States); Korea Advanced Institute of Science and Technology, Yuseong-gu, DaeJeon 305-701 (Korea, Republic of)

    2014-03-15

    An approximate two-dimensional solver of the nonlinear Fokker-Planck-Landau collision operator has been developed using the assumption that the particle probability distribution function is independent of gyroangle in the limit of strong magnetic field. The isotropic one-dimensional scheme developed for nonlinear Fokker-Planck-Landau equation by Buet and Cordier [J. Comput. Phys. 179, 43 (2002)] and for linear Fokker-Planck-Landau equation by Chang and Cooper [J. Comput. Phys. 6, 1 (1970)] have been modified and extended to two-dimensional nonlinear equation. In addition, a method is suggested to apply the new velocity-grid based collision solver to Lagrangian particle-in-cell simulation by adjusting the weights of marker particles and is applied to a five dimensional particle-in-cell code to calculate the neoclassical ion thermal conductivity in a tokamak plasma. Error verifications show practical aspects of the present scheme for both grid-based and particle-based kinetic codes.

  19. Numerical Solution of 3D Poisson-Nernst-Planck Equations Coupled with Classical Density Functional Theory for Modeling Ion and Electron Transport in a Confined Environment

    SciTech Connect (OSTI)

    Meng, Da; Zheng, Bin; Lin, Guang; Sushko, Maria L.

    2014-08-29

    We have developed efficient numerical algorithms for the solution of 3D steady-state Poisson-Nernst-Planck equations (PNP) with excess chemical potentials described by the classical density functional theory (cDFT). The coupled PNP equations are discretized by finite difference scheme and solved iteratively by Gummel method with relaxation. The Nernst-Planck equations are transformed into Laplace equations through the Slotboom transformation. Algebraic multigrid method is then applied to efficiently solve the Poisson equation and the transformed Nernst-Planck equations. A novel strategy for calculating excess chemical potentials through fast Fourier transforms is proposed which reduces computational complexity from O(N2) to O(NlogN) where N is the number of grid points. Integrals involving Dirac delta function are evaluated directly by coordinate transformation which yields more accurate result compared to applying numerical quadrature to an approximated delta function. Numerical results for ion and electron transport in solid electrolyte for Li ion batteries are shown to be in good agreement with the experimental data and the results from previous studies.

  20. The Petascale Data Storage Institute

    SciTech Connect (OSTI)

    Gibson, Garth; Long, Darrell; Honeyman, Peter; Grider, Gary; Kramer, William; Shalf, John; Roth, Philip; Felix, Evan; Ward, Lee

    2013-07-01

    Petascale computing infrastructures for scientific discovery make petascale demands on information storage capacity, performance, concurrency, reliability, availability, and manageability.The Petascale Data Storage Institute focuses on the data storage problems found in petascale scientific computing environments, with special attention to community issues such as interoperability, community buy-in, and shared tools.The Petascale Data Storage Institute is a collaboration between researchers at Carnegie Mellon University, National Energy Research Scientific Computing Center, Pacific Northwest National Laboratory, Oak Ridge National Laboratory, Sandia National Laboratory, Los Alamos National Laboratory, University of Michigan, and the University of California at Santa Cruz.