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1

Max-Planck-Institut fr molekulare Genetik  

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R K F L #12;Max-Planck-Institut für molekulare Genetik EBSV06 The Model Variables #12;MaxMax-Planck-Institut für molekulare Genetik EBSV06 Martin Vingron Max-Planck-Institut für molekulare;Max-Planck-Institut für molekulare Genetik EBSV06 Amino Acid Replacement #12;Max-Planck-Institut für

Spang, Rainer

2

Max-Planck-Institut fr Plasmaphysik  

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.15 is produced externally W R5 350 MJ 10 MJ1 MJ0.2 MJ Courtesy of Tim Hender, Culham #12;Max-Planck-Institut fürMax-Planck-Institut für Plasmaphysik Max-Planck-Institut für Plasmaphysik Wendelsteinstra?e 1 with that of the stellarator." V.D. Shafranov, 1980 #12;Max-Planck-Institut für Plasmaphysik 2/36 The classical stellarator #12

3

Max-Planck-Institut fur Mathematik  

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Universal Approximation in Embodied Systems by Guido Mont´ufar, Nihat Ay, and Keyan Ghazi-Zahedi Preprint no Planck Institute for Mathematics in the Sciences montufar@mis.mpg.de Nihat Ay Max Planck Institute

4

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Approach to Prediction and Deliberative Decision Making of Embodied Systems by Nihat Ay, and Keyan Zahedi Making of Embodied Systems Nihat Ay1,2 and Keyan Zahedi1 1 Max Planck Institute for Mathematics

5

Max-Planck-Institut fur Mathematik  

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information by Nils Bertschinger, Johannes Rauh, Eckehard Olbrich, J¨urgen Jost, and Nihat Ay Preprint no1 , J¨urgen Jost1,2 , Nihat Ay1,2 1Max Planck Institute for Mathematics in the Sciences, Leipzig

6

Max-Planck-Institut fur Mathematik  

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and Approximation Errors of Restricted Boltzmann Machines by Guido Mont´ufar, Johannes Rauh, and Nihat Ay Preprint F. Montufar1 , Johannes Rauh1 , Nihat Ay1,2 1 Max Planck Institute for Mathematics in the Sciences

7

Max-Planck-Institut fur Mathematik  

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on complexity and stochastic interaction by Nihat Ay Preprint no.: 95 2001 #12; #12; Information Geometry on Complexity and Stochastic Interaction Nihat Ay Max-Planck-Institute for Mathematics in the Sciences Inselstr

8

Max-Planck-Institut fur Mathematik  

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of Conditional Probability Polytopes by Guido Mont´ufar, Johannes Rauh, and Nihat Ay Preprint no.: 87 2014 #12 , and Nihat Ay1,2,3 {montufar, jrauh, nay}@mis.mpg.de 1 Max Planck Institute for Mathematics in the Sciences

9

Max-Planck-Institut fur Mathematik  

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of Conditional Restricted Boltzmann Machines for Sensorimotor Control by Guido Mont´ufar, Nihat Ay, and Keyan for Sensorimotor Control Guido Mont´ufar1 , Nihat Ay1,2,3 , and Keyan Zahedi1 1 Max Planck Institute

10

Max-Planck-Institut fur Mathematik  

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of Information Inequalities by Nihat Ay, and Walter Wenzel Preprint no.: 16 2011 #12;#12;On Solution Sets of Information Inequalities Nihat Ay1,2 & Walter Wenzel1,3 {nay, wenzel}@mis.mpg.de 1Max Planck Institute

11

Max-Planck-Institut fur Mathematik  

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Max-Planck-Institut f¨ur Mathematik in den Naturwissenschaften Leipzig A Note on Resistance of NPT 2013 #12;#12;A Note on Resistance of NPT to Mixture of Separable States Bobo Hua1 , Xiu-Hong Gao2 of the whole matrix. Hence the positivity of T1 is equivalent to the positivity of T2 . A quantum state

12

Max-Planck-Institut fur Mathematik  

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, and Nihat Ay Preprint no.: 60 2013 #12;#12;Information-driven intrinsic motivation in reinforcement learning Keyan Zahedi1 , Georg Martius1 , and Nihat Ay1,2 1 Information Theory of Cognitive Systems, Max Planck

13

Participants EWASS 2012 Symposium 2 Albertsson, T., Max-Planck-Institut fur Astronomie  

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Occhiogrosso, A., University College London Parise, B., Max-Planck-Institut fur Radioastronomie 1 #12;Pilbratt

Hinton, Jim

14

MaxPlanckInstitut fur Mathematik  

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of strongly interacting Markov chains by Nihat Ay and Thomas Wennekers Preprint no.: 107 2001 #12; #12; Dynamical Properties of Strongly Interacting Markov Chains Nihat Ay and Thomas Wennekers Max

15

Max-Planck-Institut f ur Mathematik  

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stochastic interaction in directed acyclic networks (revised version: March 2002) by Nihat Ay Preprint no.: 54 2001 #12; #12; Locality of Global Stochastic Interaction in Directed Acyclic Networks Nihat Ay Max

16

Max-Planck-Institut fur Mathematik  

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-organization of complex robotic behaviors by Georg Martius, Ralf Der, and Nihat Ay Preprint no.: 15 2013 #12;#12;Information driven self-organization of complex robotic behaviors Georg Martius1, Ralf Der1, Nihat Ay1,2 1Max

17

MaxPlanckInstitut fur Mathematik  

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separating arbitrary vertex classes in n­cubes by Walter Wenzel, Nihat Ay and Frank Pasemann Preprint no.: 35 Wenzel y Institute of Mathematics, Technical University of Chemnitz, D­09107 Chemnitz, Germany, Nihat Ay

18

Max-Planck-Institut fur Mathematik  

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separating arbitrary vertex classes in n-cubes by Walter Wenzel, Nihat Ay and Frank Pasemann Preprint no.: 35 Institute of Mathematics, Technical University of Chemnitz, D-09107 Chemnitz, Germany, Nihat Ay, and Frank

19

MaxPlanckInstitut f ur Mathematik  

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discrimination without entanglement by Bo Li, Shao­Ming Fei, Zhi­Xi Wang, and Heng Fan Preprint no.: 11 2012 #12, 3 and Heng Fan 1, + 1 Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China 2

20

Living and working in Germany A guide for international scientists at Max Planck Institutes  

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Living and working in Germany A guide for international scientists at Max Planck Institutes #12 and the hospitality in your town. You will quickly find that Germany is a country of many facets ­ a country Planck Society is Germany's most successful scientific or- ganisation in basic research. Max Planck

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21

Keynote speakers Susan E. Trumbore -Max-Planck-Institute for Biogeochemistry Jena, Germany  

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Keynote speakers Susan E. Trumbore - Max-Planck-Institute for Biogeochemistry Jena, Germany http for Landscape Biogeochemistry, Germany http://www.arthur-gessler.de/ PhillippeTortell, University of British

Daniel, Rosenfeld

22

Max Planck Institute for Biological Cybernetics, Tbingen, Germany VSS 2002, #18.3 ID501 Spatial updating in virtual environments  

E-Print Network [OSTI]

Max Planck Institute for Biological Cybernetics, Tübingen, Germany VSS 2002, #18.3 ID501 Spatial: What are vestibular cues good for? MPI for Biological Cybernetics, Germany 2 "Voluntary" vs Cybernetics, Germany 3 Methods - Setup · Vestibular stimuli: 6 dof Motion Platform · Visual stimuli: LCD video

23

Max-Planck-Institute for Meteorology, Hamburg, Germany Swedish Meteorological and Hydrological Institute, Norrkoping, Sweden  

E-Print Network [OSTI]

Institute, Norrko?ping, Sweden 3 Finnish Meteorological Institute, Helsinki, Finland 4 Rossby Centre, Norrko?ping, Sweden 5 German Weather Service, Offenbach, Germany 6 Institute for Marine Research, University of Kiel, Sweden A comprehensive model inter-comparison study investigating the water budget during the BALTEX

Lindau, Ralf

24

6 MaxPlanckForschung 4 | 09 PERSPEKTIVEN  

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", zu dem die Max- Planck-Gesellschaft und Siemens ber 400 Wissenschaftler, Politiker und Manager msse. Siemens setze bereits ganz auf grne Technologien, so Siemens-Chef Peter Lscher. Max-Planck-Gesellschaft und Siemens laden zum Future Dialogue Unter dem Titel ,,The Evolution of Me- dicine" fand vom 14. bis

25

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

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

Planck Society President Peter Gruss, and Consul General of the Federal Republic of Germany in New York Busso von Alvensleben meet to sign an agreement launching the new Max...

26

Max Planck Society for the Advancement of Science  

E-Print Network [OSTI]

Max Planck Society for the Advancement of Science Pressand features are hardly noticeable when the whole face is inverted (rotated 180), but strikingly grotesque are still important. "Although we look at the eyes first our neural functions still grasp the whole picture

27

Original Message Subject: [Cisprimary] [jobs] Max Planck Society seeks faculty in Autonomous  

E-Print Network [OSTI]

Original Message Subject: [Cisprimary] [jobs] Max Planck Society seeks faculty in AutonomousVjx@mail.gmail.com> > > Max Planck Society seeks faculty in Autonomous Systems at all levels > > The Max Planck Society is establishing a major new research direction > in "Autonomous Systems" to investigate and understand

Plotkin, Joshua B.

28

The Max Planck Society At home in Germany -present throughout the world  

E-Print Network [OSTI]

1 The Max Planck Society At home in Germany - present throughout the world Internationalisation ­ the Max Planck Society's role in safeguarding Germany's future Cooperation across national borders is one the internationalisation of science, both on its own behalf and also on behalf of Germany as a research location. To do

29

Bringing ATLAS production to HPC resources - A use case with the Hydra supercomputer of the Max Planck Society  

E-Print Network [OSTI]

Bringing ATLAS production to HPC resources - A use case with the Hydra supercomputer of the Max Planck Society

Kluth, Stefan; The ATLAS collaboration; Mazzaferro, Luca; Walker, Rodney

2015-01-01T23:59:59.000Z

30

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

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

31

Max-Planck-Institut fur Mathematik  

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discrimination without entanglement by Bo Li, Shao-Ming Fei, Zhi-Xi Wang, and Heng Fan Preprint no.: 11 2012 #12;#12;Assisted state discrimination without entanglement Bo Li,1, 2, Shao-Ming Fei,3, 4 Zhi-Xi Wang,3 and Heng

32

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

and geometry for Bell-diagonal states with weak measurements by Yao-Kun Wang, Teng Ma, Heng Fan, Shao-Ming Fei-diagonal states with weak measurements Yao-Kun Wang,1, 2 Teng Ma,1 Heng Fan,3 Shao-Ming Fei,1, 4 and Zhi-Xi Wang1

33

MaxPlanckInstitut f ur Mathematik  

E-Print Network [OSTI]

States by Zong­Guo Li, Ming­Jing Zhao, Shao­Ming Fei, Heng Fan, and W.M. Liu Preprint no.: 8 2012 #12; #12; Mixed maximally entangled states Zong­Guo Li 1,2 , Ming­Jing Zhao 3,4 , Shao­Ming Fei 4 , Heng

34

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

States by Zong-Guo Li, Ming-Jing Zhao, Shao-Ming Fei, Heng Fan, and W.M. Liu Preprint no.: 8 2012 #12;#12;Mixed maximally entangled states Zong-Guo Li1,2 , Ming-Jing Zhao3,4 , Shao-Ming Fei4 , Heng Fan2 , and W

35

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

of the body (see [Cia97, Cia00] for the approach via formal asymptotic expansion). The pioneering works

36

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

and nonlinear shells by the method of formal asymptotic expansions can be found in [Cia00]. In the case

37

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

] that such a motion was created by the constant ``kicks'' on the relatively heavy pollen by the light water molecules the heavy particle (the pollen) and the light particles (the water molecules) obey Newton's law. Therefore of a pollen suspended in water was erratic [5]. This led to the kinetic explanation by Einstein in 1905 [14

38

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

as a result of energetic competition . . . . . 11 3 Bulk scalings 14 3.1 The small particle limit . . . . . . . . . . . . . . . . . . . . . . . . 87 8.1.2 Identification of four scaling regimes . . . . . . . . . . 91 8.1.3 Asymptotic identification of the unstable mode in Regime III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 8

39

MAX-PLANCK-INSTITUT FR QUANTENOPTIK  

E-Print Network [OSTI]

Laserspektroskopie. Hochpräzise Spektroskopie von Wasserstoff stellt einen Test der Theorie der Quantenelektrodynamik Wasserstoff erzielt. Ein neuer Forschungs- schwerpunkt ist die Frequenzkammspektroskopie von Wasserstoff- und

Hänsch, Theodor W.

40

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

- 1)/2, D2 = d2(d2 - 1)/2, and Cmn = |mn. Here, |mn := (Lm Ln)| , with Lm, m = 1, ..., D1, Ln, n = 1

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

distribution to construct a nonintersecting lightlike transversal vector bun- dle of the tangent bundle. Since

42

Max-Planck-Institut fur Mathematik  

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, China University of Petroleum, 266580 Qingdao, China 3 College of Mathematics and Statistics, Hainan. Moreover, our lower bound of the Grothendieck constant of order three gives a refined bound for mixed states, the situation is more compli- cated. There are no general methods to judge whether a mixed

43

MaxPlanckInstitut f ur Mathematik  

E-Print Network [OSTI]

of the Science, China University of Petroleum, 266580 Qingdao, China 3 College of Mathematics and Statistics. Moreover, our lower bound of the Grothendieck constant of order three gives a refined bound­locality coincide. However for mixed states, the situation is more compli­ cated. There are no general methods

44

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

a destabilizing factor leading to the extinction of species, we here demonstrate complementarily that delay--9], subsequently leading to the extinction of species. Most ecological models neglect delays or employ sin gle systems including twospecies systems, food chains, and food webs. Twospecies models. We first study twospecies

45

Max-Planck-Institut fur Mathematik  

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. In organisms proteins fold into a compact state attaining a well defined biological function by exposing

46

Max-Planck-Institut fur Mathematik  

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-assembly in dif- ferent physico-chemical systems like micelle formation, proteins folding, macro- and microphase

47

MaxPlanckInstitut fur Mathematik  

E-Print Network [OSTI]

of ferromagnetic materials. Such conditions here stated in the form of a generalized Weierstrass maximum principle combined with the Weierstrass maximum principle, see [28, Sec tion 5.3]. The identification of a linear the state of the body\\Omega ae IR n , n = 2; 3, depends on a position x 2\\Omega and has a given temperature

48

Max-Planck-Institut fur Mathematik  

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1 gives a schematic illustration of this architecture. Since the first appearance of DBMs, a number). The undirected nature of DBMs leads to interesting and desirable properties, but it also brings of DBMs still are missing formal verification. In our main result we prove that narrow DBMs have

49

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Finster and J¨urgen Tolksdorf Preprint no.: 12 2012 #12;#12;arXiv:1201.5497v2[math-ph]1May2012 BOSONIC, the solution of the Cauchy problem is expressed in terms of tree diagrams which involve the retarded Green's function and have one outgoing leg. In order to obtain general tree diagrams, we set up a "classical

50

MaxPlanckInstitut fur Mathematik  

E-Print Network [OSTI]

. SCHN ¨ URER Abstract. A classical problem in geometric optics is to find surfaces that reflect light is reflected at a hypersurface according to the reflection law to the new direction T (x) = x \\Gamma 2hx; šiš: Antenna, geometric optics, parabolic Monge­Amp`ere equation, 2nd bound­ ary value problem. 1 #12; 2 Oliver

51

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Functions and Systems Design by Johannes Rauh and Nihat Ay Preprint no.: 66 2012 #12;#12;ROBUSTNESS, CANALYZING FUNCTIONS AND SYSTEMS DESIGN JOHANNES RAUH AND NIHAT AY Abstract. We study a notion of robustness #12;2 JOHANNES RAUH AND NIHAT AY input nodes are knocked out. We formalize our robustness requirements

52

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

­Information by Nihat Ay and Andreas Knauf Preprint no.: 42 2003 #12; #12; MAXIMIZING MULTI­INFORMATION NIHAT AY; 2 NIHAT AY AND ANDREAS KNAUF # (1,1) 1 2 # (0,0) + # (1,1) #1; 1 2 # (1,0) + # (0,1) #1; # (1

53

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Divergence from Statistical Models defined by Neural Networks by Guido Mont´ufar, Johannes Rauh, and Nihat Ay Networks Guido Mont´ufar1 , Johannes Rauh2 , and Nihat Ay2,3 1 Department of Mathematics, Pennsylvania

54

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

to Complexity by Nihat Ay, Eckehard Olbrich, Nils Bertschinger, and J¨urgen Jost Preprint no.: 53 2011 #12;#12;A Geometric Approach to Complexity Nihat Ay1,2, Eckehard Olbrich1, Nils Bertschinger1, J¨urgen Jost1,2 {nay

55

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

of stationary process realizations (revised version: November 2011) by Nihat Ay, Markus Mueller, and Arleta Szkola Preprint no.: 2 2010 #12;#12;Effective complexity of stationary process realizations Nihat Ay 1

56

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

and Global Information Geometry by Nihat Ay and Wilderich Tuschmann Preprint no.: 24 2002 #12; #12; DUALLY FLAT MANIFOLDS AND GLOBAL INFORMATION GEOMETRY Nihat Ay and Wilderich Tuschmann February 26, 2002

57

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

of the information divergence from an exponential family by FrantiŸsek Mat??uŸs and Nihat Ay Preprint no.: 46 2003 #12 of the information divergence from an exponential family Franti²ek Matú² # and Nihat Ay + Abstract. The information

58

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

for Neuromanifolds of Stochastic Dynamics by Nihat Ay, Guido Mont´ufar, and Johannes Rauh Preprint no.: 15 2011 #12;#12;Selection Criteria for Neuromanifolds of Stochastic Dynamics Nihat Ay1,2 , Guido Mont´ufar1 , Johannes Rauh1

59

MaxPlanckInstitut f ur Mathematik  

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of the information divergence from an exponential family, a problem which was first formulated by Nihat Ay in [1

60

Max-Planck-Institut fur Mathematik  

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of Classical and Non-Commutative Processes by Wolfgang L¨ohr, Arleta Szkola, and Nihat Ay Preprint no.: 52 2011 Nihat Ay1,3 August 19, 2011 Abstract We treat observable operator models (OOM) and their non

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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61

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Computation (revised version: June 2013) by Keyan Zahedi and Nihat Ay Preprint no.: 11 2013 #12;#12;Quantifying Morphological Computation Keyan Zahedi1 and Nihat Ay1,2 1 Information Theory of Cognitive Systems

62

MaxPlanckInstitut f ur Mathematik  

E-Print Network [OSTI]

Independence Ideals by Johannes Rauh, and Nihat Ay Preprint no.: 63 2011 #12; #12; ROBUSTNESS AND CONDITIONAL INDEPENDENCE IDEALS JOHANNES RAUH 1 , NIHAT AY 1,2 Abstract. We study notions of robustness of Markov kernels: September 29, 2011. 1 #12; 2 JOHANNES RAUH 1 , NIHAT AY 1,2 is important. Similarly, in the analysis

63

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

Independence Ideals by Johannes Rauh, and Nihat Ay Preprint no.: 63 2011 #12;#12;ROBUSTNESS AND CONDITIONAL INDEPENDENCE IDEALS JOHANNES RAUH1 , NIHAT AY1,2 Abstract. We study notions of robustness of Markov kernels(x) > 0} Date: September 29, 2011. 1 #12;2 JOHANNES RAUH1, NIHAT AY1,2 is important. Similarly

64

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

­information in the thermodynamic limit by Ionas Erb and Nihat Ay Preprint no.: 58 2003 #12; #12; Multi­information in the thermodynamic limit Ionas Erb # Nihat Ay + July 3, 2003 Abstract From information theory, mutual information

65

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

and Sufficient Statistics by Nihat Ay, J¨urgen Jost, H^ong V^an L^e, and Lorenz J. Schwachh¨ofer Preprint no.: 65 2012 #12;#12;INFORMATION GEOMETRY AND SUFFICIENT STATISTICS NIHAT AY1,5 , J¨URGEN JOST1,4,5 , H^ONG V

66

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

and the Tent Map by Oliver Pfante, Eckehard Olbrich, Nils Bertschinger, Nihat Ay, and J¨urgen Jost Preprint no BERTSCHINGER1,C), NIHAT AY1,2,D), J¨URGEN JOST1,2,E) Abstract. We quantify the relationship be- tween

67

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

­theoretic grounding of finite automata in neural systems by Thomas Wennekers and Nihat Ay Preprint no.: 52 2002 #12; #12; Information­theoretic grounding of finite automata in neural systems Thomas Wennekers and Nihat

68

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

from a hierarchical model of quantum states by Stephan Weis, Andreas Knauf, Nihat Ay, and Ming STATES STEPHAN WEIS1 , ANDREAS KNAUF2 , NIHAT AY1,3,4 AND MING-JING ZHAO5 Abstract. We quantify higher

69

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

Flatness in Quantum Information Geometry (revised version: August 2002) by Nihat Ay and Wilderich Tuschmann Preprint no.: 69 2002 #12; #12; DUALITY VERSUS DUAL FLATNESS IN QUANTUM INFORMATION GEOMETRY NIHAT AY as to pure state estimation theory (cf. [FN1], [FN2], [Mats]). Date: August 15, 2002. 1 #12; 2 NIHAT AY

70

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

.H. Leo S. Muller y Abstract The elastic energy of a sequence of splitting particles is computed-measures with the calculation of Khachaturyan et al. 1] for the elastic energy of cuboidal particles, doublets and octets. In the in nite splitting limit, the elastic energy of particles that split in one spatial dimension (a sequence

71

MaxPlanckInstitut fur Mathematik  

E-Print Network [OSTI]

P.H. Leo \\Lambda S. Muller y Abstract The elastic energy of a sequence of splitting particlesmeasures with the calculation of Khachaturyan et al. [1] for the elastic energy of cuboidal particles, doublets and octets. In the infinite splitting limit, the elastic energy of particles that split in one spatial dimension (a sequence

72

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

. The main results of this paper are formulated in Lemma 1 and Theorem 2. Lemma 1 is proved in Section 2. In Section 3 an example of applications of our result is given. There is a large literature [1, 2, 3||. (11) We assume that a(t) > 0, a(t) ten

73

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

, 2004 Abstract In this paper we show that the Higgs boson of the (minimal) Standard Model has at most) Standard Model the three possible gauge inequivalent ground states of the Higgs boson are shown to fully by the hypercharge of the Higgs boson. In [Tolk'03(c)] it has been shown that the symmetry of electromagnetism under

74

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

, then the corresponding energy is trapping, and orbits, visiting these sup- ports in any prescribed succession, can if the boundary of Hill's region is non-empty and not homeomorphic to a sphere. For non-trapping energies we introduce a topological degree which can be non-trivial for low energies, and for Coulombic and other singu

75

Max-Planck-Institut f ur Mathematik  

E-Print Network [OSTI]

Applications Australian National University Canberra ACT 0200, Australia chaudhur@maths.anu.edu.au and Stefan M

76

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

.2 Compatibility & incompatibility . . . . . . . . . . . . . . . . . . 5 2.3 Self . Moreover, our arguments illustrate the role of self-accommodation to achieve the minimal scaling

77

MaxPlanckInstitut fur Mathematik  

E-Print Network [OSTI]

a new physical length scale: the slippage length b. It is believed that this microscopic length scale.1 Energetics and kinetics With respect to the energetics, we assume that the spreading is driven by capillarity

78

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

compact manifolds. When M is noncompact, geometry and analysis on it becomes more complicated. Concretely these findings to Ricci solitons and self-shrinkers. Keywords and phrases: Omori-Yau maximum principle, V-Laplacian, V-harmonic map, Ricci soliton, self-shrinker. MSC 2000: 58E20, 53C27. 1. Introduction

79

Max-Planck-Institut fr molekulare Genetik  

E-Print Network [OSTI]

Large-scale Network Data · Random Graph Model (Erdös-Renyi) · Small-world model (Strogatz Large-scale analysis of protein complexes 1. Cell-lysation 2. tandem affinity-purification 3. gel with complex formation · protein identification through MS Limitations · In vivo · Large-scale, unbiased · 56

Spang, Rainer

80

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

. 2010 Mathematics Subject Classification. 20F65 (54E35,20F18,22E25,05C63). Key words and phrases. metric

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81

Leipzig, February 27 -March 01, 2013 Max Planck Institute  

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Conceptual and Mathematical Foundations of Embodied Intelligence Scientific Organizers Nihat Ay Ralf Der

82

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

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the1 - September 2006 TheSteven AshbyDepartment ofGE's E.Gilman About UsSciencePaulCenter

83

MAX-PLANCK-INSTITUT FR BIOPHYSIKALISCHE CHEMIE KARL-FRIEDRICH-BONHOEFFER-INSTITUT  

E-Print Network [OSTI]

· Interpretation of single-molecule experiments · Statistical mechanisms of biomolecules · Accurate free energy available interdisciplinary Ph. D. pro- grams, with three years funding and extension possibility

Grubmüller, Helmut

84

Living and working in Germany A guide for international scientists at Max Planck Institutes  

E-Print Network [OSTI]

expertise from the world's best scientific facilities and universities. The international character & leisure 42 3.13. Religion and holidays 44 3.14. Sanitation 46 3.15. Electricity 46 3.16. Sorting waste- stitutions. More than 90% of its financing comes from public funds from the federal government, the Länder

Falge, Eva

85

PROF. DR. FRANK JLICHER Max Planck Institute for the Physics of Complex Systems  

E-Print Network [OSTI]

-Krumbhaar Europhys. Lett. 11, 657 (1990). [2] Influence of Size of Regions of Interest on PET Evaluation of Caudate Glucose Consumption T. Kuwert, T. Ganslandt, P. Jansen, F. Jülicher, H. Lange, H. Herzog, D

Jülicher, Frank

86

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

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLas ConchasPassive Solar HomePromising Science for1Principal Investigators Postdoctoral

87

Curriculum Vitae Arne Max Erich Winguth, Ph.D.  

E-Print Network [OSTI]

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

Winguth, Arne

88

Max-Planck-Institute for the Physics of Complex Systems, Dresden, Germany MPI-PKS Institute Retreat  

E-Print Network [OSTI]

Flach Localizing Energy Through Nonlinearity and Discreteness Dining Hall 12:15 - 13:00 © Lunch 13 arrive in Gro? D¨olln 12:30 - 13:15 Check-In Hotel D¨ollnsee-Schorfheide Dining Hall 13:15 - 14:15 Lunch 16:30 - 17:20 Ilya Eremin Routes to Unconventional Superconductivity Dining Hall 18:30 - 19:30 Dinner

Jülicher, Frank

89

International Max Planck Research School  

E-Print Network [OSTI]

and February. Please check the web-page http://www.mpi-hd.mpg.de/imprs-ptfs for details. It is expected or English system. Composition of the Universe. What lies behind the mysterious Dark Matter and Dark Energy and how does it lead to the baryon asymme- try of the Universe? What are the properties of Dark Matter

90

WISE'06, Wuhan, ChinaWISE'06, Wuhan, China 11 Max-Planck Institute for Informatics, Saarbrcken, Germany  

E-Print Network [OSTI]

·· Contract between Web ServicesContract between Web Services ·· Contract between User & BrowserInteraction Contracts (IC) Framework ·· Contract between Web ServicesContract between Web Services ·· Contract between

91

AFFILIATIONS: Neggers--Royal Netherlands Meteorological Institute (KNMI), De Bilt, Netherlands; siebesma--Royal  

E-Print Network [OSTI]

AFFILIATIONS: Neggers--Royal Netherlands Meteorological Institute (KNMI), De Bilt, Netherlands; siebesma--Royal Netherlands Meteorological Institute (KNMI), De Bilt, and Delft University of Technology, Delft, Netherlands; Heus--Max Planck Institut für Meteorologie, Hamburg, Germany CORRESPONDING AUTHOR: R

Siebesma, Pier

92

Determination of the Planck constant using a watt balance with a superconducting magnet system at the National Institute of Standards and Technology  

E-Print Network [OSTI]

For the past two years, measurements have been performed with a watt balance at the National Institute of Standards and Technology (NIST) to determine the Planck constant. A detailed analysis of these measurements and their uncertainties has led to the value $h=6.626\\,069\\,79(30)\\times 10^{-34}\\,$J$\\,$s. The relative standard uncertainty is $ 45\\times 10^{-9}$. This result is $141\\times 10^{-9}$ fractionally higher than $h_{90}$. Here $h_{90}$ is the conventional value of the Planck constant given by $h_{90}\\equiv 4 /( K_{\\mathrm{J-90}}^2R_{\\mathrm{K-90}})$, where $K_{\\mathrm{J-90}}$ and $R_{\\mathrm{K-90}}$ denote the conventional values of the Josephson and von Klitzing constants, respectively.

Schlamminger, Stephan; Seifert, Frank; Chao, Leon S; Newell, David B; Liu, Ruimin; Steiner, Richard L; Pratt, Jon R

2014-01-01T23:59:59.000Z

93

The hydrological cycle tirelessly distributes water between land, ocean, atmosphere and cryosphere. Stefan Hagemann and his colleagues at the Max Planck Institute for Meteorology  

E-Print Network [OSTI]

substance across the globe, but they also carry along thermal energy in the process ­ albeit hidden into liquid water or freezes to form ice. Conversely, energy input is necessary for ice to melt or sublimeThe hydrological cycle tirelessly distributes water between land, ocean, atmosphere and cryosphere

94

Planck 2010  

ScienceCinema (OSTI)

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.

None

2011-10-06T23:59:59.000Z

95

Controlling oscillation phase through precisely timed closed-loop1 optogenetic stimulation: a computational study2  

E-Print Network [OSTI]

Neurotechnology, Gttingen, Germany19 20 Demian Battaglia*, Max Planck Institute for Dynamics and Self. Demian Battaglia (shared last authorship)31 Max Planck Institut for Dynamics and Selforganization32

Battaglia, Demian

96

80 MaxPlanckForschung 4 | 11 xxxxxxxxxxxx  

E-Print Network [OSTI]

zeugen die Felsmalereien im Wadi Howar, sdlich des Gilf el-Kebir. Das Wadi zieht sich vom Tschad bis

97

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)

98

Atmos. Chem. Phys., 10, 33093319, 2010 www.atmos-chem-phys.net/10/3309/2010/  

E-Print Network [OSTI]

Research Centre Geesthacht, Institute for Coastal Research, Max-Planck-Str. 1, 21502 Geesthacht, Germany 4

Paris-Sud XI, Université de

99

1194 VOLUME 10J O U R N A L O F C L I M A T E 1997 American Meteorological Society  

E-Print Network [OSTI]

, United Kingdom u Institute for Atmospheric Physics, GKSS­Research Center, Max-Planck-Strasse, Geesthacht

Xue, Yongkang

100

Soil Control on Runoff Response to Climate Change in Regional Climate Model Simulations  

E-Print Network [OSTI]

, Switzerland #GKSS Forschungszentrum, Geesthacht, Germany @Max Planck Institute for Meteorology, Hamburg

Haak, Hein

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to obtain the most current and comprehensive results.


101

Abstract Submitted for the DPP05 Meeting of  

E-Print Network [OSTI]

, Forschungszentrum Juelich, IPP (Germany), F. LEUTERER, Max Planck Institut fuer Plasmaphysik (Germany), E. WESTERHOF

102

Planck-Length Phenomenology  

E-Print Network [OSTI]

This author's recent proposal of interferometric tests of Planck-scale-related properties of space-time is here revisited from a strictly phenomenological viewpoint. The results announced previously are rederived using elementary dimensional considerations. The dimensional analysis is then extended to the other two classes of experiments (observations of neutral kaons at particle accelerators and observations of the gamma rays we detect from distant astrophysical sources) which have been recently considered as opportunities to explore "foamy" properties of space-time. The emerging picture suggests that there is an objective and intuitive way to connect the sensitivities of these three experiments with the Planck length. While in previous studies the emphasis was always on some quantum-gravity scenario and the analysis was always primarily aimed at showing that the chosen scenario would leave a trace in a certain class of doable experiments, the analysis here reported takes as starting point the experiments and, by relating in a direct quantitative way the sensitivities to the Planck length, provides a model-independent description of the status of Planck-length phenomenology.

Giovanni Amelino-Camelia

2000-08-04T23:59:59.000Z

103

Boundary value problems for nonlinear first-order ODEs -constructing generalised solutions via the max-plus algebra  

E-Print Network [OSTI]

the max-plus algebra RICAM Georg Regensburger Johann Radon Institute for Computational and Applied Theory of Differential Equations Heriot-Watt University, Edinburgh, 9 August, 2006 SFB F1322 #12;Max), is a (generalized) solution of (1) Then Max-plus linear combination (Min-plus) #12;Max-plus Interpolation Given

Eilbeck, Chris

104

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

E-Print Network [OSTI]

(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)and the Max-Planck-Institut für Plasmaphysik, (Garching, Germany)and the Max-Planck-Institut für Plasmaphysik

105

Kurzfassungen der Meteorologentagung DACH, Vol. 1, DACH2007-A-00083, 2007  

E-Print Network [OSTI]

Forschungszentrum, Geesthacht, (2) Meteorologisches Institut der Universität Hamburg , (3) Max Planck Institut für

Zahn, Matthias

106

Copyright 2004, 2005 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are  

E-Print Network [OSTI]

Copyright 2004, 2005 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are registered trademarks of the WiMAX ForumTM. * All trademarks are the properties of their respective owners. WiMAX Forum Internal Use Only WiMAX System Modeling Methodology Raj Jain Professor of Computer Science and Engineering

Jain, Raj

107

ComputerScience,TexasA&MUniversity JetMax: Scalable Max-Min  

E-Print Network [OSTI]

1 ComputerScience,TexasA&MUniversity JetMax: Scalable Max-Min Congestion Control for High- Speed Heterogeneous Networks JetMax: Scalable MaxJetMax: Scalable Max--MinMin Congestion Control for High congestion control and its designed properties · Analysis of existing max-min methods XCP, MKC, and MKC

Loguinov, Dmitri

108

QwMaxSat: A Weighted Partial MaxSAT Solver  

E-Print Network [OSTI]

#12; Koshimura, M., Zhang, T., Fujita, H., & Hasegawa, R. (2012). QMaxSAT: A Partial Max-SAT SolverQwMaxSat: A Weighted Partial MaxSAT Solver 2013725 C304 ERATO #12;Problem Solving with MaxSAT 2 Original Problem MaxSAT Problem MaxSAT Model Max

Banbara, Mutsunori

109

Summary Max Total Units  

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

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 Delicious RankCombustion |Energy Usage »of Energy Strain Rate4 Recovery Act/BuySummary Max Total Units *If All

110

Improved Approximations for Max Set Splitting and Max NAE SAT  

E-Print Network [OSTI]

Improved Approximations for Max Set Splitting and Max NAE SAT #3; Jiawei Zhang and Yinyu Ye y Nanjing, 210093, P.R.China August 16, 2000, Revised January 22, 2001. #3; This research was supported Fudan University, Shanghai, R.R.China. z This work was done while the author was visiting Computational

Ye, Yinyu

111

Atmos. Chem. Phys., 12, 74657474, 2012 www.atmos-chem-phys.net/12/7465/2012/  

E-Print Network [OSTI]

, Stellenbosch 7599, South Africa 2Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, 21502 Geesthacht, Germany 3Max-Planck-Institut f¨ur Chemie, Hahn-Meitner-Weg 1, 55128 Mainz, Germany

Meskhidze, Nicholas

112

EMSL - climate  

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

2014GB004826:

  • Max Planck Institute for Biogeochemistry, Jena, Germany
  • Earth System Modeling Program
  • Max Planck Institute for Intelligent...

113

INSTITUTE OF PHYSICS PUBLISHING PLASMA PHYSICS AND CONTROLLED FUSION Plasma Phys. Control. Fusion 47 (2005) 919940 doi:10.1088/0741-3335/47/6/012  

E-Print Network [OSTI]

-Planck-Institut f¨ur Plasmaphysik, Greifswald, 17491, Germany 2 Plasma Research Laboratory, Australian National

Howard, John

114

Planck Surveyor On Its Way to Orbit  

ScienceCinema (OSTI)

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

None

2010-01-08T23:59:59.000Z

115

MATERIALS AND MOLECULAR RESEARCH DIVISION, ANNUAL REPORT 1976  

E-Print Network [OSTI]

tpresent address: Institut flir Atom-und Festkorper- physik,Max Planck Insi tute flir Festkorperfurschung, Stuttgart,

Authors, Various

2010-01-01T23:59:59.000Z

116

Information driven self-organization: The dynamical system approach to autonomous robot  

E-Print Network [OSTI]

Nihat Ay1,3 , Ralf Der1 , Mikhail Prokopenko2 1 Max Planck Institute for Mathematics, Leipzig, Germany 2

Der, Ralf

117

Predictive information and emergent cooperativity in a chain of mobile robots , Frank Guttler#  

E-Print Network [OSTI]

¨uttler# , Nihat Ay+ * Max-Planck Institute for Mathematics in the Sciences Leipzig, Germany # University Leipzig

Der, Ralf

118

Evidence cross-validation and Bayesian inference of MAST plasma G. T. von Nessi, M. J. Hole, J. Svensson, and L. Appel  

E-Print Network [OSTI]

University, Canberra ACT 0200, Australia 2 Max-Planck-Institut fur Plasmaphysik, D-17491 Greifswald, Germany

119

Neuron-Less Neural-Like Networks with Exponential Association Capacity  

E-Print Network [OSTI]

Battaglia Department of Nonlinear Dynamics, Max-Planck-Institute for Dynamics and Self-Organization, D37073

Battaglia, Demian

120

Proceedings of the Work-in-Progress Session of the 20th IEEE Real-Time and Embedded Technology and Applications Symposium  

E-Print Network [OSTI]

for Software Systems #12;© Copyright 2014 Max Planck Institute for Software Systems. All rights reserved. The copyright of this collection is with the Max Planck Institute for Software Systems. The copyright, to discuss, and to network. Björn B. Brandenburg Max Planck Institute for Software Systems Kaiserslautern

Ungerer, Theo

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

Crystal Structure of the Minimalist Max-E47 Protein Faraz Ahmadpour1  

E-Print Network [OSTI]

Crystal Structure of the Minimalist Max-E47 Protein Chimera Faraz Ahmadpour1 , Rodolfo Ghirlando2, Canada Abstract Max-E47 is a protein chimera generated from the fusion of the DNA-binding basic region of Max and the dimerization region of E47, both members of the basic region/helix-loop-helix (b

Guarne, Alba

122

Cosmological science enabled by Planck  

E-Print Network [OSTI]

Planck will be the first mission to map the entire cosmic microwave background (CMB) sky with mJy sensitivity and resolution better than 10'. The science enabled by such a mission spans many areas of astrophysics and cosmology. In particular it will lead to a revolution in our understanding of primary and secondary CMB anisotropies, the constraints on many key cosmological parameters will be improved by almost an order of magnitude (to sub-percent levels) and the shape and amplitude of the mass power spectrum at high redshift will be tightly constrained.

Martin White

2006-06-27T23:59:59.000Z

123

Min-max and min-max regret versions of some combinatorial optimization problems : a survey  

E-Print Network [OSTI]

of such events. The purpose of this paper is to review the existing literature on the min-max and min-max rMin-max and min-max regret versions of some combinatorial optimization problems : a survey Hassene Aissi , Cristina Bazgan , and Daniel Vanderpooten Résumé Les critères min-max et min-max regret sont

Boyer, Edmond

124

Heat Hyperbolic Diffusion in Planck Gas  

E-Print Network [OSTI]

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

Miroslaw Kozlowski; Janina Marciak-Kozlowska

2006-07-06T23:59:59.000Z

125

Frederic Laquai Seminar: Photocurrent Generation in Low-Bandgap...  

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

| 3:30 PM - 4:30 PM Frederic Laquai Head, Max Planck Research Group for Organic Optoelectronics Max Planck Institute for Polymer Research Photocurrent Generation in Low-Bandgap...

126

Cloud Security by Max Garvey  

E-Print Network [OSTI]

Cloud Security Survey by Max Garvey #12;Cloudy Cloud is Cloudy What is the cloud? On Demand Service Network access Resource pooling Elasticity of Resources Measured Service #12;Cloud Types/Variants Iaa Cloud Public Cloud Hybrid Cloud combination. Private cloud with overflow going to public cloud. #12

Tolmach, Andrew

127

Finitely presented groups 4 Max Neunhffer  

E-Print Network [OSTI]

under rotation and inversion and all r R are reduced. Max Neunhöffer (University of St Andrews.e.: pa, pb R for a, b ^X with a = b. Max Neunhöffer (University of St Andrews) Finitely presented is a piece, we have |p| r|. (|r| is the length in letters). Max Neunhöffer (University of St Andrews

Neunhöffer, Max

128

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

E-Print Network [OSTI]

aus, Wasserstoff sicherer und Platz sparender zu speichern; und sie legen die Grundlagen, um Batterien

129

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

E-Print Network [OSTI]

aus, Wasserstoff sicherer und Platz sparender zu speichern; und sie legen die Grundlagen, um Batterien

130

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLas ConchasPassive Solar Home DesignPresentations Presentations926Innovation| Princeton Plasma

131

International Max Planck Research School on Adapting Behavior in a Fundamentally Uncertain World  

E-Print Network [OSTI]

of the universities' main building. As early as 8.15 am the course program started. All lecturers were guarded by local students, introducing them to the au dience and offering assistance during analysis. Due to the bad weather, the welcome tour nament had to be cancelled. Nevertheless

132

Measuring CMB polarisation with the Planck mission  

E-Print Network [OSTI]

In this paper, we discuss why and how the Planck mission, originally designed and proposed for mapping CMB intensity fluctuations, has been revised for polarisation measurement capability as well.

J. Delabrouille

2003-07-31T23:59:59.000Z

133

Semimartingales from the Fokker-Planck Equation  

SciTech Connect (OSTI)

We show the existence of a semimartingale of which one-dimensional marginal distributions are given by the solution of the Fokker-Planck equation with the pth integrable drift vector (p > 1)

Mikami, Toshio [Department of Mathematics, Hokkaido University, Sapporo 060-0810 (Japan)], E-mail: mikami@math.sci.hokudai.ac.jp

2006-03-15T23:59:59.000Z

134

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

Office of Environmental Management (EM)

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

135

E-Print Network 3.0 - analysen der neuesten Sample Search Results  

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

DACH, Vol. 1, DACH2007-A-00083, 2007 Meteorologentagung DACH... Forschungszentrum, Geesthacht, (2) Meteorologisches Institut der Universitt Hamburg , (3) Max Planck Institut...

136

E-Print Network 3.0 - association vilamoura portugal Sample Search...  

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

ur Plasmaphysik, EURATOM Association, Greifswald, Germany dInstitute for Plasma Research, ... Source: Coster, David - Max-Planck-Institut fr Plasmaphysik Collection:...

137

Extended metabolite profile of the human spinal cord Andreas Hock1  

E-Print Network [OSTI]

for Biomedical Engineering, University and ETH Zurich, Zurich, Switzerland, 2 Dept. of Clinical Research Institute of Neuroradiology, University Hospital of Zurich, Zurich, Switzerland, 4 Max Planck Institute

138

The Planck Surveyor mission: astrophysical prospects  

E-Print Network [OSTI]

Although the Planck Surveyor mission is optimized to map the cosmic microwave background anisotropies, it will also provide extremely valuable information on astrophysical phenomena. We review our present understanding of Galactic and extragalactic foregrounds relevant to the mission and discuss on one side, Planck's impact on the study of their properties and, on the other side, to what extent foreground contamination may affect Planck's ability to accurately determine cosmological parameters. Planck's multifrequency surveys will be unique in their coverage of large areas of the sky (actually, of the full sky); this will extend by two or more orders of magnitude the flux density interval over which mm/sub-mm counts of extragalactic sources can be determined by instruments already available (like SCUBA) or planned for the next decade (like the LSA-MMA or the space mission FIRST), which go much deeper but over very limited areas. Planck will thus provide essential complementary information on the epoch-dependent luminosity functions. Bright radio sources will be studied over a poorly explored frequency range where spectral signatures, essential to understand the physical processes that are going on, show up. The Sunyaev-Zeldovich effect, with its extremely rich information content, will be observed in the direction of a large number of rich clusters of Galaxies. Thanks again to its all sky coverage, Planck will provide unique information on the structure and on the emission properties of the interstellar medium in the Galaxy. At the same time, the foregrounds are unlikely to substantially limit Planck's ability to measure the cosmological signals. Even measurements of polarization of the primordial Cosmic Microwave background fluctuations appear to be feasible.

G. De Zotti; L. Toffolatti; F. Argeso; R. D. Davies; P. Mazzotta; R. B. Partridge; G. F. Smoot; N. Vittorio

1999-03-27T23:59:59.000Z

139

Planck 2015 results. XIII. Cosmological parameters  

E-Print Network [OSTI]

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints fr...

,

2015-01-01T23:59:59.000Z

140

Cyclic jobshop problem and (max, +)-algebra August 29, 2011  

E-Print Network [OSTI]

-plus algebra and discrete event systems The (max, +) algebra is the set R - endowed with the max operator 3 / 29 #12;Max-plus algebra and discrete event systems The (max, +) algebra is the set R - endowedCyclic jobshop problem and (max, +)-algebra L. Houssin LAAS-CNRS August 29, 2011 L. Houssin Cyclic

Ingrand, François

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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141

Ideal Quantum Gases with Planck Scale Limitations  

E-Print Network [OSTI]

A thermodynamic system of non-interacting quantum particles changes its statistical distribution formulas if there is a universal limitation for the size of energetic quantum leaps (magnitude of quantum leaps smaller than Planck energy). By means of a restriction of the a priori equiprobability postulate one can reach a thermodynamic foundation of these corrected distribution formulas. The number of microstates is determined by means of a suitable counting method and combined with thermodynamics via the Boltzmann principle. The result is that, for particle energies that come close to the Planck energy, the thermodynamic difference between fermion and boson distribution vanishes. Both distributions then approximate a Boltzmann distribution. The wave and particle character of the quantum particles, too, can be influenced by choosing the size of the temperature and particle energy parameters relative to the Planck energy, as you can see from the associated fluctuation formulas. In the case of non-relativistic de...

Collier, Rainer

2015-01-01T23:59:59.000Z

142

Astrophysical Bounds on Planck Suppressed Lorentz Violation  

E-Print Network [OSTI]

This article reviews many of the observational constraints on Lorentz symmetry violation (LV). We first describe the GZK cutoff and other phenomena that are sensitive to LV. After a brief historical sketch of research on LV, we discuss the effective field theory description of LV and related questions of principle, technical results, and observational constraints. We focus on constraints from high energy astrophysics on mass dimension five operators that contribute to LV electron and photon dispersion relations at order E/M_Planck. We also briefly discuss constraints on renormalizable operators, and review the current and future contraints on LV at order (E/M_Planck)^2.

Ted Jacobson; Stefano Liberati; David Mattingly

2004-07-30T23:59:59.000Z

143

Planck's Radiation Law in the Quantized Universe  

E-Print Network [OSTI]

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.

Rainer Collier

2014-09-15T23:59:59.000Z

144

Acceleration radiation and the Planck scale  

E-Print Network [OSTI]

A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiation. We point out that this field-theory effect can be derived, for any dimension higher than two, without actually invoking very high energy physics. This supports the view that this phenomenon is robust against Planck-scale physics and, therefore, should be compatible with any underlying microscopic theory.

I. Agullo; J. Navarro-Salas; G. J. Olmo; L. Parker

2008-02-27T23:59:59.000Z

145

Planck Scale Cosmology in Resummed Quantum Gravity  

E-Print Network [OSTI]

We show that, by using resummation techniques based on the extension of the methods of Yennie, Frautschi and Suura to Feynman's formulation of Einstein's theory, we get quantum field theoretic predictions for the UV fixed-point values of the dimensionless gravitational and cosmological constants. Connections to the phenomenological asymptotic safety analysis of Planck scale cosmology by Bonanno and Reuter are discussed.

B. F. L. Ward

2008-08-23T23:59:59.000Z

146

Planck Scale Cosmology and Resummed Quantum Gravity  

E-Print Network [OSTI]

We show that, by using amplitude-based resummation techniques for Feynman's formulation of Einstein's theory, we get quantum field theoretic 'first principles' predictions for the UV fixed-point values of the dimensionless gravitational and cosmological constants. Connections to the phenomenological asymptotic safety analysis of Planck scale cosmology by Bonanno and Reuter are discussed.

B. F. L. Ward

2009-10-13T23:59:59.000Z

147

Special Publication 800-127 Guide to Securing WiMAX  

E-Print Network [OSTI]

Padgette of Booz Allen Hamilton. The authors would also like to thank the WiMAX Forum of the National Institute of Standards and Technology (NIST) and Cyrus Tibbs and Matthew Sexton of Booz Allen Hamilton, wish to thank their colleagues who reviewed drafts of this document and contributed to its

148

Copyright 2004, 2005, 2006, 2007 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are  

E-Print Network [OSTI]

://www.wimaxforum.org/apps/org/workgroup/aatg/ download.php/25704/WiMAX_System_Evaluation_M ethodology_071215R2.pdf #12;Copyright 2004, 2005, 2006, 2007Copyright 2004, 2005, 2006, 2007 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are registered trademarks of the WiMAX ForumTM. * All trademarks are the properties of their respective owners

Jain, Raj

149

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...

150

MAX232, MAX232I DUAL EIA 232 DRIVERS/RECEIVERS  

E-Print Network [OSTI]

+ C1- C2+ C2- VS- T2OUT R2IN VCC GND T1OUT R1IN R1OUT T1IN T2IN R2OUT MAX232 . . . D, DW, N, OR NSIN T2OUT R2INR2OUT 11 10 12 9 14 7 13 8 #12;MAX232, MAX232I DUAL EIA 232 DRIVERS/RECEIVERS SLLS047LMAX232, MAX232I DUAL EIA 232 DRIVERS/RECEIVERS SLLS047L - FEBRUARY 1989 - REVISED MARCH 2004 1POST

Ravikumar, B.

151

Application of Planck's law to thermionic conversion  

SciTech Connect (OSTI)

A simple, highly accurate, mathematical model of heat-to-electricity conversion is developed from Planck's law for the distribution of the radiant exitance of heat at a selected temperature. An electrical power curve is calculated by integration of the heat law over a selected range of electromagnetic wavelength corresponding to electrical voltage. A novel wavelength-voltage conversion factor, developed from the known wavelength-electron volt conversion factor, establishes the wavelength ({lambda}) for the integration. The Planck law is integrated within the limits {lambda} to 2{lambda}. The integration provides the ideal electrical power that is available from heat at the emitter temperature. When multiplied by a simple ratio, the calculated ideal power closely matches published thermionic converter experimental data. The thermal power model of thermionic conversion is validated by experiments with thermionic emission of ordinary electron tubes. A theoretical basis for the heat law based model of thermionic conversion is found in linear oscillator theory.

Caldwell, F.

1998-07-01T23:59:59.000Z

152

Boolean Max-Co-Clones ANDREI A. BULATOV1  

E-Print Network [OSTI]

on a systematic study of max-co-clones. Intuitively, applying max-quantification to a re- lation R(x1, . . . , xn, y1, . . . , yk) results in the relation max(y1, . . . , yk)R(x1, . . . , xn, y1, . . . , ykBoolean Max-Co-Clones ANDREI A. BULATOV1 Simon Fraser University In our ISMVL 2012 paper we

Bulatov, Andrei

153

Boolean Max-Co-Clones Andrei A. Bulatov  

E-Print Network [OSTI]

on a systematic study of max-co-clones. Intuitively, applying max-quantification to a relation R(x1, . . . , xn, y1, . . . , yk) results in the relation max(y1, . . . , yk)R(x1, . . . , xn, y1, . . . , ykBoolean Max-Co-Clones Andrei A. Bulatov Abstract. In our ISMVL 2012 paper we introduced the notion

Bulatov, Andrei

154

ON CYCLIC CLASSES AND ATTRACTION CONES IN MAX SERGEI SERGEEV  

E-Print Network [OSTI]

of linear algebra developed over the max- times semiring Rmax,? which is the set of nonnegative numbers R-plus semiring Rmax,+ = (R {-}, = max, = +), developed over the set of real numbers R with adjoined element to Rmax,+ and Rmax,?. Another well-known semiring is the max-min semiring Rmax,min = (R {-} {}, = max

Butkovic, Peter

155

MAP and Planck vs the Real Universe  

E-Print Network [OSTI]

The Microwave Anisotropy Probe (MAP) and Planck Surveyor satellites promise to provide accurate maps of the sky at a range of frequencies and angular scales, from which it will be possible to extract estimates for cosmological parameters. But the real Universe is a nasty, messy place, full of non-linear astrophysics. It is certainly clear that MAP and Planck will fix the background cosmology at an unprecedented level. However, they will have to contend with everything that the Universe throws at them: multiple foregrounds; structure formation effects; and other complications we haven't even thought of yet. Some examples of such effects will be presented. Only an ideal, theorist's universe can be described by a number of free parameters in the single digits, while in reality it is likely that a greater wealth of information waits to be discovered. These `higher-order' processes should be considered as potentially measurable signals, rather than contaminants. The capabilities of Planck seem ideally suited to fully understanding the physics encoded in the microwave sky.

Douglas Scott

1998-10-21T23:59:59.000Z

156

Hardness of Max-2Lin and Max-3Lin over integers, reals, and large cyclic Ryan O'Donnell  

E-Print Network [OSTI]

systems of linear equations. Given a ring R, the Max-kLin(R) problem is defined as follows: An input, this easily implies the same hardness for Max--3Lin(Q) and Max--3Lin(R). In- deed, it shows a kind of "bicriHardness of Max-2Lin and Max-3Lin over integers, reals, and large cyclic groups Ryan O

O'Donnell, Ryan

157

E-Print Network 3.0 - alcohol industries case Sample Search Results  

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

1 200607HIGHLIGHT POLICY AND PRACTICE Summary: & Tropical Medicine) and colleagues in Russia and at the Max Planck Institute, Germany, conducted a case... -control study...

158

E-Print Network 3.0 - atomic quantum bits Sample Search Results  

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

Dynamics group, Max-Planck-Institut fr Quantenoptik Collection: Physics 19 insight review articles 238 NATURE | VOL 416 | 14 MARCH 2002 | www.nature.com Summary:...

159

E-Print Network 3.0 - attosecond transient recorder Sample Search...  

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

. The attosecond transient recorder uses linearly polarized few-cycle infrared laser fields. An attosecond ... Source: Kling, Matthias - Max-Planck-Institut fr Quantenoptik...

160

E-Print Network 3.0 - arabidopsis ath1 microarray Sample Search...  

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

Universiteit - Department of Plant Systems Biology, Bioinformatics and Evolutionary Genomics Division; Weigel, Detlef - Abteilung 6 Molekularbiologie, Max-Planck-Institut fr...

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

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

SciTech Connect (OSTI)

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.

Dubilier, Nicole [Max Planck Institute

2014-03-19T23:59:59.000Z

162

E-Print Network 3.0 - anglo-american news paradigm Sample Search...  

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

and Information Sciences 54 David Gill, Tim Minshall and Martin Rigby Summary: as the Fraunhofer Gesellschaft and the Max Planck Institutes) largely absent in the...

163

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

Office of Environmental Management (EM)

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

164

X-ray and neutron scattering studies of the complex compounds...  

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

by Dr. Hoyoung Jang, Max Planck Institute for Solid State Research in Stuttgart, Germany In condensed matter physics, in particular a field of complex oxide materials, most...

165

E-Print Network 3.0 - arndt wiessner peter Sample Search Results  

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

Renewable Energy ; Geosciences 2 Max Planck Institute for Molecular Genetics, Berlin, Germany Otto Warburg International Summer School and Workshop on Summary: Tobias Muller...

166

Solving Protein Structures from Scratch | U.S. DOE Office of...  

Office of Science (SC) Website

Contact Ilme Schlichting Max Planck Institute for Medical Research, Heidelberg, Germany ilme.schlichting@mpimf-heidelberg.mpg.de Funding Portions of this research were...

167

E-Print Network 3.0 - andrei surzhenkov priit Sample Search Results  

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

Juan Antonio Navarro Perez and Andrei Voronkov. Proof systems for effec- tively Source: Navarro Prez, Juan Antonio - Max-Planck-Institut fr Softwaresysteme Collection:...

168

Variational Analysis of the Spectral Abscissa at a Matrix with a ...  

E-Print Network [OSTI]

Computational Methods in Systems and Control Theory,. Max Planck Institute for ..... applications in computer graphics, are studied in [Gru11, Chapters 2 and 4].

2012-10-18T23:59:59.000Z

169

Expressive Power and Approximation Errors of Restricted Boltzmann Machines  

E-Print Network [OSTI]

, Johannes Rauh1 , Nihat Ay1,2 1 Max Planck Institute for Mathematics in the Sciences, Inselstra?e 22 04103

170

E-Print Network 3.0 - arabidopsis thaliana seed Sample Search...  

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

Max-Planck-Institut fr Entwicklungsbiologie Collection: Biology and Medicine 26 EMS Mutagenesis 101 From: Methods in Molecular Biology, vol. 323: Arabidopsis Protocols,...

171

E-Print Network 3.0 - arabidopsis thaliana seeds Sample Search...  

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

Max-Planck-Institut fr Entwicklungsbiologie Collection: Biology and Medicine 26 EMS Mutagenesis 101 From: Methods in Molecular Biology, vol. 323: Arabidopsis Protocols,...

172

E-Print Network 3.0 - alpacas lama pacos Sample Search Results  

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

trust. Alpaca is an authentication... using the former using their existing, unmodified certificates. Alpaca builds on Proof Source: Ford, Bryan - Max-Planck-Institut fr...

173

E-Print Network 3.0 - alpaca lama pacos Sample Search Results  

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

trust. Alpaca is an authentication... using the former using their existing, unmodified certificates. Alpaca builds on Proof Source: Ford, Bryan - Max-Planck-Institut fr...

174

E-Print Network 3.0 - attosecond pulse trains Sample Search Results  

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

Trains In HHG... polarized. Therefore, attosecond pulses generally are produced in a train, with two pulses ... Source: Kling, Matthias - Max-Planck-Institut fr Quantenoptik...

175

E-Print Network 3.0 - alpha-radionuklidov ra pb Sample Search...  

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

Steven L. Goldstein Max-Planck Institut ... Source: Rudnick, Roberta L. - Department of Geology, University of Maryland at College Park Collection: Geosciences 16 Mobile...

176

E-Print Network 3.0 - answer set programming Sample Search Results  

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

(ASP). A brief, but comprehensive introduction... properties of answer ... Source: Navarro Prez, Juan Antonio - Max-Planck-Institut fr Softwaresysteme Collection: Computer...

177

E-Print Network 3.0 - atomos communication system Sample Search...  

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

un conjunto numerable L cuyos elementos son llamados atomos; los conectivos Source: Navarro Prez, Juan Antonio - Max-Planck-Institut fr Softwaresysteme Collection: Computer...

178

Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum  

E-Print Network [OSTI]

We update the all-sky Planck catalogue of 1227 clusters and cluster candidates (PSZ1) published in March 2013, derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. Addendum. We deliver an updated version of the PSZ1 catalogue, reporting the further confirmation of 86 Planck-discovered clusters. In total, the PSZ1 now contains 947 confirmed clusters, of which 214 were confirmed as newly discovered clusters through follow-up observations undertaken by the Planck Collaboration. The updated PSZ1 contains redshifts for 913 systems, of which 736 (~80.6%) are spectroscopic, and associated mass estimates derived from the Y_z mass proxy. We also provide a new SZ quality flag, derived from a novel artificial neural network classification of the SZ signal, for the remaining 280 candidates. Based on this assessment, the purity of the updated PSZ1 catalogue is estimated to be 94%. In this release, we provide the full updated catalogue and an additional readme ...

Ade, P A R; Armitage-Caplan, C; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; Aussel, H; Baccigalupi, C; Banday, A J; Barreiro, R B; Barrena, R; Bartelmann, M; Bartlett, J G; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bikmaev, I; Bobin, J; Bock, J J; Bhringer, H; Bonaldi, A; Bond, J R; Borrill, J; Bouchet, F R; Bridges, M; Bucher, M; Burenin, R; Burigana, C; Butler, R C; Cardoso, J -F; Carvalho, P; Catalano, A; Challinor, A; Chamballu, A; Chary, R -R; Chen, X; Chiang, H C; Chiang, L -Y; Chon, G; Christensen, P R; Churazov, E; Church, S; Clements, D L; Colombi, S; Colombo, L P L; Comis, B; Couchot, F; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Da Silva, A; Dahle, H; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Dmocls, J; Dsert, F -X; Dickinson, C; Diego, J M; Dolag, K; Dole, H; Donzelli, S; Dor, O; Douspis, M; Dupac, X; Efstathiou, G; Enlin, T A; Eriksen, H K; Feroz, F; Ferragamo, A; Finelli, F; Flores-Cacho, I; Forni, O; Frailis, M; Franceschi, E; Fromenteau, S; Galeotta, S; Ganga, K; Gnova-Santos, R T; Giard, M; Giardino, G; Gilfanov, M; Giraud-Hraud, Y; Gonzlez-Nuevo, J; Grski, K M; Grainge, K J B; Gratton, S; Gregorio, A; N,; Groeneboom, E; Gruppuso, A; Hansen, F K; Hanson, D; Harrison, D; Hempel, A; Henrot-Versill, S; Hernndez-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Hurley-Walker, N; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihnen, E; Keskitalo, R; Khamitov, I; Kisner, T S; Kneissl, R; Knoche, J; Knox, L; Kunz, M; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Laureijs, R J; Lawrence, C R; Leahy, J P; Leonardi, R; Len-Tavares, J; Lesgourgues, J; Li, C; Liddle, A; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; MacTavish, C J; Maffei, B; Maino, D; Mandolesi, N; Maris, M; Marshall, D J; Martin, P G; Martnez-Gonzlez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Mazzotta, P; Mei, S; Meinhold, P R; Melchiorri, A; Melin, J -B; Mendes, L; Mennella, A; Migliaccio, M; Mikkelsen, K; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J A; Naselsky, P; Nastasi, A; Nati, F; Natoli, P; Nesvadba, N P H; Netterfield, C B; Nrgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; O'Dwyer, I J; Olamaie, M; Osborne, S; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrott, Y C; Perrotta, F; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Popa, L; Poutanen, T; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reach, W T; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rowan-Robinson, M; Rubio-Martn, J A; Rumsey, C; Rusholme, B; Sandri, M; Santos, D; Saunders, R D E; Savini, G; Schammel, M P; Scott, D; Seiffert, M D; Shellard, E P S; Shimwell, T W; Spencer, L D; Starck, J -L; Stolyarov, V; Stompor, R; Streblyanska, A; Sudiwala, R; Sunyaev, R; Sureau, F; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tomasi, M; Tramonte, D; Tristram, M; Tucci, M; Tuovinen, J; Trler, M; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vibert, L; Vielva, P; Villa, F; Vittorio, N; Wade, L A; Wandelt, B D; White, M; White, S D M; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

179

On visualization scaling, subeigenvectors and Kleene stars in max algebra  

E-Print Network [OSTI]

and Kleene stars in max algebra #12;Max Algebra a, b R+ a + b, ab A, B Rm?n + A + B, AB, . a b = max(a, b;(Ar )ij = max (i,j;r) (i, j; r)(A) (I A · · · An-1)ij = max(i.j,r) (i, j; r) : r = 0, . . . n - 1 A definite: (A) = 1 (I A · · · An-1)ij = max(i,j) (i, j) : r = 0, . . . , Hans Schneider based on joint

Schneider, Hans

180

Bare Higgs mass at Planck scale  

E-Print Network [OSTI]

We compute one- and two-loop quadratic divergent contributions to the bare Higgs mass in terms of the bare couplings in the Standard Model. We approximate the bare couplings, defined at the ultraviolet cutoff scale, by the MS-bar ones at the same scale, which are evaluated by the two-loop renormalization group equations for the Higgs mass around 126GeV in the Standard Model. We obtain the cutoff scale dependence of the bare Higgs mass, and examine where it becomes zero. We find that when we take the current central value for the top quark pole mass, 173GeV, the bare Higgs mass vanishes if the cutoff is about 10^{23}GeV. With a 1.3 sigma smaller mass, 170GeV, the scale can be of the order of the Planck scale.

Yuta Hamada; Hikaru Kawai; Kin-ya Oda

2015-01-19T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

MINI REVIEW ARTICLE published: 28 April 2014  

E-Print Network [OSTI]

to individual differences in brain structure? Jenny Gu1 * and Ryota Kanai1,2 1 School of Psychology, University Edited by: Burkhard Pleger, Max Planck Institute for Human Cognitive and Brain Sciences, Germany Reviewed by: Marco Taubert, Max-Planck-Institute for Human Cognitive and Brain Sciences, Germany Christopher J

Sussex, University of

182

de r eche r che INSTITUT NATIONAL DE RECHERCHE EN INFORMATIQUE ET EN AUTOMATIQUE  

E-Print Network [OSTI]

'' (R[ f\\Gamma1g; max; +), or the ``tropical semiring'' (N[f+1g;min;+), have been invented'alg??ebre lin??eaire (max,+) R??esum??e : Il s'agit d'une br??eve introduction au semi­anneau (max,+) et autres semiISSN 0249­6399 appo r t de r eche r che INSTITUT NATIONAL DE RECHERCHE EN INFORMATIQUE ET EN

O'Sullivan, Joseph A.

183

Extended Fokker Planck model: properties and solutions  

E-Print Network [OSTI]

In the current paper Fokker Planck model of random walks has been extended to non conservative cases characterized by explicit dependence of diffusion and energy on time. A given generalization allows describing of such non equilibrium processes as Levy flights in a classical differential form without use of fractal PDE. Besides it takes into account mixing properties that are obligatory for a certain class of chaotic systems such as Kolmogorov K system. It was shown that an abnormal transport is a consequence of the equilibrium distortion and not stationary diffusion. The particular case of fixed boundaries was considered. According to the received solutions it was shown that a system structure can resist a weak disturbance in the vicinity of the discrete regimes, defined by a system scale and its nonlinear properties. These regimes correspond to the exponential increase of quasi regular structure fluctuations. Only fast disruption of regime is possible for other states of the system. It leads to an immediate transition to the chaos.

Sergey Kamenshchikov

2014-01-20T23:59:59.000Z

184

Neurton Damage and MAX Phase Ternary Compounds  

SciTech Connect (OSTI)

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.

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

2014-06-17T23:59:59.000Z

185

Max Ambiental S A | 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 CenterFranconia, Virginia: Energy Resources Jump to:46 - 429Lacey,(MonasterLowellis aMaury County, Tennessee: Energy Resources JumpMaviMax

186

Institutional INSTITUTIONAL DATA BOOK  

E-Print Network [OSTI]

that institutions provide for their learning and personal development. The University of Minnesota is an equal ORGANIZATIONAL STRUCTURE UMM Organizational Chart as of August 2009

Minnesota, University of

187

On the Usefulness of Predicates Per Austrin, Aalto University and KTH Royal Institute of Technology  

E-Print Network [OSTI]

of Technology Johan Hastad, KTH Royal Institute of Technology Motivated by the pervasiveness of strong as saying that P is useful for P itself. We say that P is useless if it is not useful for any Q. This turns characterization of useful Max-CSPs defined by a predicate: such a Max-CSP is useless if and only

Hstad, Johan

188

Min-max-min robustness - Optimization Online  

E-Print Network [OSTI]

or the minimum spanning tree problem turn NP-hard in the new approach. ..... [9] Melvyn, S., Robust optimization, Ph.D. thesis, Massachusetts Institute of.

2014-11-27T23:59:59.000Z

189

Implications of SCUBA observations for the Planck Surveyor  

E-Print Network [OSTI]

We investigate the implications for the Planck Surveyor of the recent sub-millimetre number counts obtained using the SCUBA camera. Since it observes at the same frequency as one of the higher frequency science channels on Planck, SCUBA can provide constraints on the point-source contribution to the CMB angular power spectrum, which require no extrapolation in frequency. We have calculated the two-point function of these sub-millimetre sources, using a Poisson model normalized to the observed counts. While the current data are uncertain, under reasonable assumptions the point-source contribution to the anisotropy is comparable to the noise in the 353GHz channel. The clustering of these sources is currently unknown, however if they cluster like the z~3 Lyman-break galaxies their signal would be larger than the primary anisotropy signal on scales smaller than about 10 arcmin. We expect the intensity of these sources to decrease for wavelengths longward of 850 microns. At the next lowest Planck frequency, 217GHz, the contribution from both the clustered and Poisson terms are dramatically reduced. Hence we do not expect these sources to seriously affect Planck's main science goal, the determination of the primordial anisotropy power spectrum. Rather, the potential determination of the distribution of sub-mm sources is a further piece of cosmology that Planck may be able to tackle.

Douglas Scott; Martin White

1999-03-18T23:59:59.000Z

190

Planck 2015 results. XXI. The integrated Sachs-Wolfe effect  

E-Print Network [OSTI]

This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS and WISE catalogues, and the Planck 2015 convergence lensing map. This cross-correlation yields a detection at $4\\,\\sigma$, where most of the signal-to-noise is due to the Planck lensing and NVSS. In fact, the ISW effect is detected only from the Planck data (through the ISW-lensing bispectrum) at $\\approx 3\\,\\sigma$, which is similar to the detection level achieved by combining the cross-correlation signal coming from all the catalogues. This cross-correlation analysis is performed only with the Planck temperature data, since the polarization scales available in the 2015 release do not permit significant improvement of the CMB-LSS cross-correlation detectability. Nevertheless, polarization data is used to study the anomalously large ISW signal previously reported through the aperture photometry on stacked CMB features at the locat...

Ade, P A R; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Casaponsa, B; Catalano, A; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Church, S; 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; Dsert, F -X; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, T A; Eriksen, H K; Fergusson, J; Fernandez-Cobos, R; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Gnova-Santos, R T; Giard, M; Giraud-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versill, S; Hernndez-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Ili?, S; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihnen, E; Keskitalo, R; Kisner, T S; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Langer, M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Ma, Y -Z; Macas-Prez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Marcos-Caballero, A; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, 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; Nrgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Popa, L; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reach, W T; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubio-Martn, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Schaefer, B M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sunyaev, 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; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

191

Deciding Unambiguity and Sequentiality from a Finitely Ambiguous MaxPlus Automaton  

E-Print Network [OSTI]

with multiplicities in the max­plus semiring R max = (R # {-#},max, +). Roughly speaking, it is an automaton with two tapes: an input tape labelled by a finite alphabet #, and an output tape weighted in R max . The weightDeciding Unambiguity and Sequentiality from a Finitely Ambiguous Max­Plus Automaton Ines Klimann

Fondements et Applications, Université Paris 7

192

APPLICATION OF THE FUZZY MIN-MAX NEURAL NETWORK CLASSIFIER  

E-Print Network [OSTI]

. The fuzzy min-max classi cation network constitutes a promisimg pattern recognition approach that is based. Experimental results us- ing the modi ed model on a di cult pattern recognition prob- lem establishes of the fuzzy min-max clas- si cation neural network on a pattern recognition problem that involves both

Blekas, Konstantinos

193

Modcomp MAX IV System Processors reference guide  

SciTech Connect (OSTI)

A user almost always faces a big problem when having to learn to use a new computer system. The information necessary to use the system is often scattered throughout many different manuals. The user also faces the problem of extracting the information really needed from each manual. Very few computer vendors supply a single Users Guide or even a manual to help the new user locate the necessary manuals. Modcomp is no exception to this, Modcomp MAX IV requires that the user be familiar with the system file usage which adds to the problem. At General Atomics there is an ever increasing need for new users to learn how to use the Modcomp computers. This paper was written to provide a condensed Users Reference Guide'' for Modcomp computer users. This manual should be of value not only to new users but any users that are not Modcomp computer systems experts. This Users Reference Guide'' is intended to provided the basic information for the use of the various Modcomp System Processors necessary to, create, compile, link-edit, and catalog a program. Only the information necessary to provide the user with a basic understanding of the Systems Processors is included. This document provides enough information for the majority of programmers to use the Modcomp computers without having to refer to any other manuals. A lot of emphasis has been placed on the file description and usage for each of the System Processors. This allows the user to understand how Modcomp MAX IV does things rather than just learning the system commands.

Cummings, J.

1990-10-01T23:59:59.000Z

194

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

E-Print Network [OSTI]

J. Ashdown et al. : Making Maps from Planck LFI 30GHz DataJ. Ashdown et al. : Making Maps from Planck LFI 30GHz Datain this study. The hit map is shown in the ecliptic (left)

Ashdown, M.A.J.

2010-01-01T23:59:59.000Z

195

On the Fokker-Planck Equation for Stochastic Hybrid Systems  

E-Print Network [OSTI]

On the Fokker-Planck Equation for Stochastic Hybrid Systems: Application to a Wind Turbine Model- speed wind turbine, with a switching controller that combines stall regulation and pitch control FPE is stated. Then the theory is applied to a variable-speed wind turbine model, yielding

Boyer, Edmond

196

Making Maps from Planck LFI 30GHz Data  

E-Print Network [OSTI]

This paper is one of a series describing the performance and accuracy of map-making codes as assessed by the Planck CTP working group. We compare the performance of multiple codes written by different groups for making polarized maps from Planck-sized, all-sky cosmic microwave background (CMB) data. Three of the codes are based on destriping algorithm, whereas the other three are implementations of a maximum-likelihood algorithm. Previous papers in the series described simulations at 100 GHz (Poutanen et al. 2006) and 217 GHz (Ashdown et al. 2006). In this paper we make maps (temperature and polarisation) from the simulated one-year observations of four 30 GHz detectors of Planck Low Frequency Instrument (LFI). We used Planck Level S simulation pipeline to produce the observed time-ordered-data streams (TOD). Our previous studies considered polarisation observations for the CMB only. For this paper we increased the realism of the simulations and included polarized galactic foregrounds to our sky model. Our simulated TODs comprised of dipole, CMB, diffuse galactic emissions, extragalactic radio sources, and detector noise. The strong subpixel signal gradients arising from the foreground signals couple to the output map through the map-making and cause an error (signal error) in the maps. Destriping codes have smaller signal error than the maximum-likelihood codes. We examined a number of schemes to reduce this error. On the other hand, the maximum-likelihood map-making codes can produce maps with lower residual noise than destriping codes.

M. A. J. Ashdown; C. Baccigalupi; A. Balbi; J. G. Bartlett; J. Borrill; C. Cantalupo; G. de Gasperis; K. M. Gorski; V. Heikkila; E. Hivon; E. Keihanen; H. Kurki-Suonio; C. R. Lawrence; P. Natoli; T. Poutanen; S. Prunet; M. Reinecke; R. Stompor; B. Wandelt

2007-02-19T23:59:59.000Z

197

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

E-Print Network [OSTI]

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

Lin, Gang

198

Board of Directors : Prof. Alfred Leipertz (Coordinator) Prof. Michael Schmidt (Co-Coordinator)  

E-Print Network [OSTI]

in their respective fields and has as its aim the promotion of innovation and leadership skills in all specialist in the SAOT. · Max Planck Institute for the Science of Light (MPL) · Fraunhofer Institute for Integrated

Fiebig, Peter

199

Atmos. Chem. Phys., 13, 70077021, 2013 www.atmos-chem-phys.net/13/7007/2013/  

E-Print Network [OSTI]

-Zentrum Geesthacht, Institute of Coastal Research, Department for Environmental Chemistry, Max-Planck-Str. 1, 21502 Geesthacht, Germany 5Institute of Environmental Physics, University of Heidelberg, Im Neuenheimer Feld 229

Meskhidze, Nicholas

200

Figure 2: Pulse sequence: Navigators are applied before inner-volume saturation (IVS), up-/downfield  

E-Print Network [OSTI]

, and Anke Henning1,3 1 Institute for Biomedical Engineering, University and ETH Zurich, Zurich, Switzerland, 2 Institute of Neuroradiology, University Hospital of Zurich, Zurich, Switzerland, 3 Max Planck

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Component-based Face Recognition with 3D Morphable Models B. Weyrauch  

E-Print Network [OSTI]

@mpi-sb.mpg.de Honda Research Institute USA, Inc. Max-Planck-Institute for Computer Science Boston, MA Saarbr. In this paper, we combine morphable models and component-based recognition. The morphable model is em- ployed

Poggio, Tomaso

202

A 0.5-APPROXIMATION ALGORITHM FOR MAX DICUT WITH GIVEN SIZES OF PARTS  

E-Print Network [OSTI]

(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;nding a directed cut ?A 0.5-APPROXIMATION ALGORITHM FOR MAX DICUT WITH GIVEN SIZES OF PARTS ALEXANDER AGEEV #3; , REFAEL(X) with maximum total weight. In this paper we consider a version of max dicut|max dicut with given sizes of parts

Ageev, Alexandr

203

New Bounds for MAX-SAT by Clause Learning Alexander S. Kulikov  

E-Print Network [OSTI]

New Bounds for MAX-SAT by Clause Learning Alexander S. Kulikov Konstantin Kutzkov May 3, 2009 c MAX-SAT for formulas with constant clause density; · 2K/6 , where K is the number of clauses, for MAX-2-SAT; · 2N/6.7 for (n, 3)-MAX-2-SAT. All

204

A New Approach to Proving Upper Bounds for MAX-2-SAT Arist Kojevnikov  

E-Print Network [OSTI]

A New Approach to Proving Upper Bounds for MAX-2-SAT Arist Kojevnikov Alexander S. Kulikov problem (MAX-2-SAT). We present a new 2K/5.5 -time algorithm for MAX-2-SAT, where K is the number formula, for a particular case of MAX-2-SAT, where each variable appears in at most three 2-clauses

205

Planck 2015 results. XIV. Dark energy and modified gravity  

E-Print Network [OSTI]

We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG), beyond the cosmological constant scenario. We start with cases where the DE only directly affects the background evolution, considering Taylor expansions of the equation of state, principal component analysis and parameterizations related to the potential of a minimally coupled DE scalar field. When estimating the density of DE at early times, we significantly improve present constraints. We then move to general parameterizations of the DE or MG perturbations that encompass both effective field theories and the phenomenology of gravitational potentials in MG models. Lastly, we test a range of specific models, such as k-essence, f(R) theories and coupled DE. In addition to the latest Planck data, for our main analyses we use baryonic acoustic oscillations, type-Ia supernovae and local measurements of the Hubble constant. We further show the impact of measurements of the cosmological perturbations, such as redshif...

Ade, P A R; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Battye, R; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; 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; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Church, S; 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; Dsert, F -X; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, 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; Giard, M; Giraud-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Heavens, A; Helou, G; Henrot-Versill, S; Hernndez-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huang, Z; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihnen, E; Keskitalo, R; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; Lesgourgues, J; Levrier, F; Lewis, A; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Ma, Y -Z; Macas-Prez, J F; Maggio, G; Mandolesi, N; Mangilli, A; Marchini, A; Martin, P G; Martinelli, M; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, J A; Narimani, A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nrgaard-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; Popa, L; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reach, W T; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rowan-Robinson, M; Rubio-Martn, J A; Rusholme, B; Salvatelli, V; Sandri, M; Santos, D; Savelainen, M; Savini, G; Schaefer, B M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sunyaev, 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; Viel, M; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; White, M; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

206

On the integer max-linear programming problem Peter Butkovic1,  

E-Print Network [OSTI]

and the integer max-linear programming problem. In max-algebra, for a, b R = R {-}, we define a b = max(a, b to Elsevier July 22, 2013 #12;A two-sided max-linear system (TSS) is of the form Ax c = Bx d where A, B R m time, and give a method in this case. If f R n , then the function f(x) = fT x is called max

Butkovic, Peter

207

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

E-Print Network [OSTI]

AND GREGORY B. SORKIN Abstract. The class Max (r, 2)-CSP (or simply Max 2-CSP) consists of constraint(rm/5) for r- valued problems), making it the fastest for Max Cut, and tied (at the time) for Max 2-Sat(·) notation, which ignores leading polynomial factors, is defined in Section 2.1.) For Max 2-CSP we give an O(r

Scott, Alexander Alexander

208

SETI at Planck Energy: When Particle Physicists Become Cosmic Engineers  

E-Print Network [OSTI]

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 ...

Lacki, Brian C

2015-01-01T23:59:59.000Z

209

Planck-scale effects on Bose-Einstein condensates  

E-Print Network [OSTI]

The effects of a Planck-scale deformation of the Minkowski energy-momentum dispersion relation on the phenomenology of non-trapped Bose-Einstein condensates (BECs) are examined. Such a deformation is shown to cause a shift in the condensation temperature $T_{c}$ of the BEC and, for a specific functional form of deformation, this shift can be as large as the current measured precision on $T_{c}$. For a $_{37}^{85}Rb$ cold-atom BEC with a particle density $n\\simeq 10^{12}cm^{-3}$ we find a fractional shift of order $10^{-4}$, but this can be much larger for even more dilute BECs. We discuss the possibility of planning specific experiments with BECs that might provide phenomenological constraints on Planck-scale physics. These corrections to $T_{c}$ are found to be extremely small for ultrarelativistic BECs implying that, in some cases, Planck-scale effects may be more important in low- rather than high-energy processes.

F. Briscese; M. Grether; M. de Llano

2012-06-20T23:59:59.000Z

210

Eigenvalues And Eigenvectors In The Max-Plus Algebra  

E-Print Network [OSTI]

The max-plus algebra defined in the set ! [ f\\Gamma1g is an algebra with two binary operations \\Phi and\\Omega where a \\Phi b is the maximum of a and b, and a\\Omega b is the sum of a and b. These operations form a monoid-field (there is no inverse under \\Phi). This paper implements algorithms for solving linear systems and computing eigenvalues and eigenvectors including the first known polynomial-time algorithm for finding eigenvalues of matrices in the max-plus algebra. Analogs to the characteristic equation and the Cayley-Hamilton theorem are presented. This abstract accurately represents the content of the candidate's thesis. I recommend its publication. Signed David C. Fisher iii Contents 1 The Max-Plus Algebra 1 1.1 Matrix Multiplication in (! max ) n\\Thetan : : : : : : : : : : : : : : : : : 3 1.2 An Application : : : : : : : : : : : : : : : : : : : : : : : : : : : : 5 2 Systems of Linear Equations in (! max ) n 8 2.1 Solving Ax \\Phi b = Cx \\Phi d : : : : : : : : : : : ...

By Misoo; Misoo Chung; William E. Cherowitzo; David C. Fisher; David C. Fisher

211

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.

212

SETI at Planck Energy: When Particle Physicists Become Cosmic Engineers  

E-Print Network [OSTI]

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.

Brian C. Lacki

2015-03-05T23:59:59.000Z

213

TeV Astrophysics Constraints on Planck Scale Lorentz Violation  

E-Print Network [OSTI]

We analyze observational constraints from TeV astrophysics on Lorentz violating nonlinear dispersion for photons and electrons without assuming any a priori equality between the photon and electron parameters. The constraints arise from thresholds for vacuum Cerenkov radiation, photon decay and photo-production of electron-positron pairs. We show that the parameter plane for cubic momentum terms in the dispersion relations is constrained to an order unity region in Planck units. We find that the threshold configuration can occur with an asymmetric distribution of momentum for pair creation, and with a hard photon for vacuum Cerenkov radiation.

Ted Jacobson; Stefano Liberati; David Mattingly

2002-09-24T23:59:59.000Z

214

Iain S. Walker1 and Max H. Sherman1  

E-Print Network [OSTI]

LBNL 50189 1 Iain S. Walker1 and Max H. Sherman1 Sealant Longevity for Residential Ducts Reference by LBNL is being used as a basis for an ASTM Standard under sub-committee E6.41. LBNL tests found sealants. LBNL has also tested advanced tape products being developed by major manufacturers. The results

215

SINGLE-ZONE STACK-DOMINATED INFILTRATION MODELING Max Sherman  

E-Print Network [OSTI]

SINGLE-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 of Energy under Contract No. DE-AC03-76SF00098. #12;2 NOMENCLATURE Neutral level [-]s ELA Effective leakage

216

Structured Region Graphs: Morphing EP into GBP Max Welling  

E-Print Network [OSTI]

Structured Region Graphs: Morphing EP into GBP Max Welling Dept. of Computer Science UC Irvine@eecs.berkeley.edu Abstract GBP and EP are two successful algo­ rithms for approximate probabilistic infer­ ence, which on these structures allow conversion between EP and GBP free ener­ gies. Thus it is revealed that all EP ap

Welling, Max

217

Structured Region Graphs: Morphing EP into GBP Max Welling  

E-Print Network [OSTI]

Structured Region Graphs: Morphing EP into GBP Max Welling Dept. of Computer Science UC Irvine@eecs.berkeley.edu Abstract GBP and EP are two successful algo- rithms for approximate probabilistic infer- ence, which on these structures allow conversion between EP and GBP free ener- gies. Thus it is revealed that all EP ap

Welling, Max

218

Water Quality for Livestock Max Irsik DVM, MAB  

E-Print Network [OSTI]

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

Watson, Craig A.

219

Joint Planck and WMAP Assessment of Low CMB Multipoles  

E-Print Network [OSTI]

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...

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

2015-01-01T23:59:59.000Z

220

DOE FY10_Svc_Cont_Inv 122910 v2 MAX.xlsx | Department of Energy  

Energy Savers [EERE]

MAX.xlsx DOE FY10SvcContInv 122910 v2 MAX.xlsx More Documents & Publications Service Contract Inventory ClassWaiverWC-1982-001-FormerlyWA-1982-017.pdf...

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While these samples are representative of the content of NLEBeta,
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to obtain the most current and comprehensive results.


221

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

E-Print Network [OSTI]

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

Banbara, Mutsunori

222

An Approximation Algorithm for MAX DICUT with Given Sizes of Parts  

E-Print Network [OSTI]

function w : E(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;nding a directed cut ? weight function w : E(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;ndingAn Approximation Algorithm for MAX DICUT with Given Sizes of Parts Alexander Ageev #3; Sobolev

Sviridenko, Maxim

223

A freely-moving monkey treadmill model Justin D Foster1  

E-Print Network [OSTI]

, Providence, RI 02912, USA 5 Palo Alto Medical Foundation, Palo Alto, CA 94305, USA 6 Max Planck Institute with the speed of individual steps. On a population level, we find that neural state-space trajectories

Shenoy, Krishna V.

224

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...

225

E-Print Network 3.0 - attosecond photoelectron spectroscopy Sample...  

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

Max-Planck-Institut fr Quantenoptik Collection: Physics 3 Attosecond Atomic Physics Review of literature Summary: will be oscillating in time. When such a state is ionized by an...

226

Astron. Astrophys. 338, L75L78 (1998) ASTROPHYSICS  

E-Print Network [OSTI]

1 Max-Planck-Institut f¨ur Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany 2 on the spectrum of CRs, their composition, details of the nuclear cross sections, and propagation in the Galaxy

Moskalenko, Igor V.

227

astroph/9808084 A&A manuscript no.  

E-Print Network [OSTI]

. Strong 1 and O. Reimer 1 1 Max­Planck­Institut f?ur extraterrestrische Physik, Postfach 1603, D­85740, details of the nuclear cross sections, and propagation in the Galaxy. Because they are secondary, an

Strong, Andrew W.

228

Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation  

E-Print Network [OSTI]

, CA 90009, USA g Max-Planck-Institut fu¨r extraterrestrische Physik, Postfach 1603, D-85740 Garching and Be in the model predictions is attributed to uncertainties in the production cross-section data. The latter

Moskalenko, Igor V.

229

E-Print Network 3.0 - aqueduto vestibular alargado Sample Search...  

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

Page: << < 1 2 3 4 5 > >> 1 Max Planck Institute for Biological Cybernetics, Tbingen, Germany VSS 2002, 18.3 ID501 Spatial updating in virtual environments Summary: updating in...

230

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

ScienceCinema (OSTI)

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

Wiegel, Detlef

2011-04-25T23:59:59.000Z

231

III. High-Resolution Imaging of Nearby M dwarfs V. J. S. Bjar1,2  

E-Print Network [OSTI]

la Universidad de La Laguna, 3Centro de Astrobiología, 4Max-Planck-Institut für Astronomie · 5. Flux contribution and variations induced by companions at different separations. Red, blue and green

Complutense de Madrid, Universidad

232

Atmos. Chem. Phys., 13, 64216428, 2013 www.atmos-chem-phys.net/13/6421/2013/  

E-Print Network [OSTI]

, PMB 1, Menai, NSW 2234, Australia 4Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, 21502 Geesthacht, Germany Correspondence to: F. Slemr (franz.slemr@mpic.de) Received: 18 February 2013

Meskhidze, Nicholas

233

On the edge of death: Rates of decline and lower thresholds of biochemical condition in food-deprived fish larvae and juveniles  

E-Print Network [OSTI]

Helgoland, Germany i Helmholtz Centre Geesthacht, Centre for Materials and Coastal Research, Institute for Coastal Research, Max-Planck-Stra?e 1, 21502 Geesthacht, Germany j Department of Biology, Lund University

234

Atmos. Chem. Phys., 8, 14451482, 2008 www.atmos-chem-phys.net/8/1445/2008/  

E-Print Network [OSTI]

Fourier, France 11GKSS-Forschungszentrum Geesthacht GmbH, Institute for Coastal Research, Department for Environmental Chemistry, Max-Planck-Str. 1, 21052 Geesthacht, Germany 12G¨oteborg University and Chalmers

Douglas, Thomas A.

235

Design of a nitrogen-implanted titanium-based superelastic alloy with optimized properties for  

E-Print Network [OSTI]

, Bucharest, Romania 5 Institute of Materials Research, Helmholtz-Zentrum Geesthacht -Zentrum für Material- und Küstenforschung GmbH Max-Planck-Stra?e 1, D-21502 Geesthacht, Germany *Corresponding author: Prof

Paris-Sud XI, Université de

236

Atmos. Chem. Phys., 14, 22192231, 2014 www.atmos-chem-phys.net/14/2219/2014/  

E-Print Network [OSTI]

-Zentrum Geesthacht, Institute of Coastal Research, Department for Environmental Chemistry,Max-Planck-Str. 1, 21502 Geesthacht, Germany 4Environment Canada, Science and Technology Branch, 867 Lakeshore Rd, Burlington, Ontario

Meskhidze, Nicholas

237

7, 1083710931, 2007 Polar mercury review  

E-Print Network [OSTI]

) and Universite Joseph Fourier, France 10 GKSS-Forschungszentrum Geesthacht GmbH, Institute for Coastal Research, Department for Environmental Chemistry Max-Planck-Str. 1, 21052 Geesthacht, Germany 11 G¨oteborg University

Paris-Sud XI, Université de

238

fur Mathematik in den Naturwissenschaften  

E-Print Network [OSTI]

Approximation Results for Deep Belief Networks and Restricted Boltzmann Machines by Guido Mont´ufar, and Nihat Networks and Restricted Boltz- mann Machines Guido Montufar,1, Nihat Ay1, 2 1Max Planck Institute

239

fur Mathematik in den Naturwissenschaften  

E-Print Network [OSTI]

Families and Oriented Matroid Theory by Johannes Rauh, Thomas Kahle, and Nihat Ay Preprint no.: 28 2009 #12 kahle@mis.mpg.de Nihat Ay Max Planck Institute for Mathematics in the Sciences nay@mis.mpg.de Abstract

240

Electron antineutrino search Sudbury Neutrino Observatory 9 Bellerive,  

E-Print Network [OSTI]

, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA Alamos National Laboratory, Alamos Accelerator Center, Menlo Park, California, d Present address: Max­Planck­Institut Nuclear Physics, Heidelberg

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
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to obtain the most current and comprehensive results.


241

Atmos. Chem. Phys., 7, 599608, 2007 www.atmos-chem-phys.net/7/599/2007/  

E-Print Network [OSTI]

System Modelling, Bundesstr. 53, 20146 Hamburg, Germany Received: 4 September 2006 Published in Atmos. Giorgetta1 1Max Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, Germany 2IMPRS on Earth

Paris-Sud XI, Universit de

242

8, 20852127, 2008 Evaluation of radon  

E-Print Network [OSTI]

System Modelling, Hamburg, Germany 3 LAPC, Institute of Atmospheric Physics, Chinese Academy of Sciences Physics, Chinese Academy of Sciences, Beijing, China 2 International Max Planck Research School on Earth

Paris-Sud XI, Universit de

243

Comparison of Circadian Changes in the Retinas of Migrating and Non-migrating Blackcaps, Sylvia atricapilla  

E-Print Network [OSTI]

Animals Male Blackcaps (Sylvia atricapilla) were caught in Tovetorp, Sweden, at the University of Stockholm Zoological field station, with permittage from the Swedish Environmental Protection Agency. They were transported to the Max Planck Institute...

Shockley, Ross

2006-07-11T23:59:59.000Z

244

advance photonics map: Topics by E-print Network  

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

with a CV (gerne auch auf deutsch) Dr. Peter Baum Max-Planck-Institute for Quantum Optics, and Ludwig are table-top and will be operated by yourself and our small team. Our...

245

Model-Free Reconstruction of Excitatory Neuronal Connectivity from Calcium Imaging Signals  

E-Print Network [OSTI]

Stetter1,2,3 , Demian Battaglia1,3 *, Jordi Soriano4 , Theo Geisel1,2,3 1 Max Planck Institute, Battaglia D, Soriano J, Geisel T (2012) Model-Free Reconstruction of Excitatory Neuronal Connectivity from

Battaglia, Demian

246

ORIGINAL RESEARCH ARTICLE published: 07 February 2013  

E-Print Network [OSTI]

the frontiers of neuronal types Demian Battaglia1,2 *, Anastassios Karagiannis3,4 , Thierry Gallopin5 , Harold W, France *Correspondence: Demian Battaglia, Max Planck Institute for Dynamics and Self

Battaglia, Demian

247

Modeling and Algorithm for DynamicModeling and Algorithm for Dynamic Multi-Objective Max-CSPsMulti-Objective Max-CSPs  

E-Print Network [OSTI]

_n is blow m. ­ e.g. m=5 : No (3,3) / Yes (4,1) #12;Multi-Objective Max-CSP (Properties) For a cost vector RModeling and Algorithm for DynamicModeling and Algorithm for Dynamic Multi-Objective Max-CSPsMulti-Objective Max-CSPs Tenda Okimoto ¹², Tony Rebeiro ³, Maxime Clement and Katsumi Inoue ² ¹ Transdisciplinary

Banbara, Mutsunori

248

The Institute of Asian and African Studies The Max Schloessinger Memorial Foundation  

E-Print Network [OSTI]

im Breisgau in Febru- ary 2002. It oers a new approach to problems of Islamic hermeneutics and the understanding of Qur-anic exegesis. It is well known that a central problem of Islamic hermeneutics in Qur

Paris-Sud XI, Universit de

249

Lawrence Berkeley National Laboratory report LBNL-50634 Min-max Identities on Boundaries of  

E-Print Network [OSTI]

in their interiors, then min x bd(K) max f bd(L) f(x) = r0 = min f bd(L) max x bd(K) f(x) . (1) This identity (1) is given by max {r : rL K} = r0 = max {r : rK L } , (2) where K is the polar set of K. Finally, the pairs (x0, f0) R ? (Rn ) that solve both min-max problems in equation (1) have x0 r0 bd(L) bd

250

Theorem: L : Z List. ( p :{Z Z | let m, i = p in max_seg_sum(m; L) max_initseg_sum(i; L)}) L:Z List. (p:{Z Z| let m,i = p in max_seg_sum(m;L) max_initseg_sum(i;L)})  

E-Print Network [OSTI]

(u;u + p2) initseg_sum(r;[u; u1 / v]) )) 2 #12;Theorem: L : Z List. ( p :{Z ? Z | let m, i = p in maxTheorem: L : Z List. ( p :{Z ? Z | let m, i = p in max_seg_sum(m; L) max_initseg_sum(i; L)}) L:Z List. (p:{Z ? Z| let m,i = p in max_seg_sum(m;L) max_initseg_sum(i;L)}) | BY (D 0 THENA Auto) | 1. L

251

4 / 2 0 0 8 M A X P L A N C K F O R S C H U N G 85 MAX PLANCK AKTUELL  

E-Print Network [OSTI]

- sellschaft: Bei den konomen lag Porsche knapp vor der Deutschen Lufthansa und der BMW-Group. Informatiker Deutschland und die BMW- Group. Bei den Ingenieur

252

Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence  

E-Print Network [OSTI]

The Pseudo-Nambu-Goldstone Boson (PNGB) potential, defined through the amplitude $M^4$ and width $f$ of its characteristic potential $V(\\phi) = M^4[1 + \\cos(\\phi~ /~ f)]$, is one of the best-suited models for the study of thawing quintessence. We analyse its present observational constraints by direct numerical solution of the scalar field equation of motion. Observational bounds are obtained using data from Union 2.1 for Supernovae, cosmic microwave background temperature anisotropies from Planck plus WMAP polarization data, and baryon acoustic oscillations data. We find the parameter ranges for which PNGB quintessence remains a viable theory for dark energy. We compare the direct potential analysis and use of an approximate equation-of-state parameterization for thawing theories; this comparison highlights a strong prior dependence to the outcome coming from the choice of modelling methodology, which current data are not sufficient to override.

Smer-Barreto, Vanessa

2015-01-01T23:59:59.000Z

253

Planck's quantum-driven integer quantum Hall effect in chaos  

E-Print Network [OSTI]

The integer quantum Hall effect (IQHE) and chaos are commonly conceived as being unrelated. Contrary to common wisdoms, we find in a canonical chaotic system, the kicked spin-$1/2$ rotor, a Planck's quantum($h_e$)-driven phenomenon bearing a firm analogy to IQHE but of chaos origin. Specifically, the rotor's energy growth is unbounded ('metallic' phase) for a discrete set of critical $h_e$-values, but otherwise bounded ('insulating' phase). The latter phase is topological in nature and characterized by a quantum number ('quantized Hall conductance'). The number jumps by unity whenever $h_e$ decreases passing through each critical value. Our findings, within the reach of cold-atom experiments, indicate that rich topological quantum phenomena may emerge from chaos.

Yu Chen; Chushun Tian

2014-09-18T23:59:59.000Z

254

The Planck/LFI Radiometer Electronics Box Assembly  

E-Print Network [OSTI]

The Radiometer Electronics Box Assembly (REBA) is the control and data processing on board computer of the Low Frequency Instrument (LFI) of the Planck mission (ESA). The REBA was designed and built incorporating state of the art processors, communication interfaces and real time operating system software in order to meet the scientific performance of the LFI. We present a technical summary of the REBA, including a physical, functional, electrical, mechanical and thermal description. Aspects of the design and development, the assembly, the integration and the verification of the equipment are provided. A brief description of the LFI on board software is given including the Low-Level Software and the main functionalities and architecture of the Application Software. The compressor module, which has been developed as an independent product, later integrated in the application, is also described in this paper. Two identical engineering models EM and AVM, the engineering qualification model EQM, the flight model ...

Herreros, J M; Rebolo, R; Chulani, H; Rubino-Martin, J A; Hildebrandt, S R; Bersanelli, M; Butler, R C; Miccolis, M; Pena, A; Pereira, M; Torrero, F; Franceschet, C; Lopez, M; Alcala, C; 10.1088/1748-0221/4/12/T12008

2010-01-01T23:59:59.000Z

255

A Fokker-Planck Model of Rotating Stellar Clusters  

E-Print Network [OSTI]

We have developed a two-dimensional orbit averaged Fokker-Planck model of stellar clusters which expands on spherically symmetric one-dimensional models to include rotation and ellipticity. Physical effects such as collisions, finite stellar lifetimes and bar formation (i.e., a non-axisymmetric component of the potential) can also be included. The first use of the model is to study the evolution of dense clusters (rho(r=0)=~10^7 M_sun/pc^3) that may be expected to have existed at the centres of newly-forming galaxies, with the goal of verifying that angular momentum can be removed from the core of the cluster quickly enough so that rotation no longer prevents the formation of a massive (~10^2 M_sun) object. This could act as the seed black hole for the formation of an AGN.

J. Girash

1997-04-05T23:59:59.000Z

256

Irreversible Thermodynamics of the Universe: Constraints from Planck Data  

E-Print Network [OSTI]

The present work deals with irreversible Universal thermodynamics. The homogenous and isotropic flat model of the universe is chosen as open thermodynamical system and non-equilibrium thermodynamics comes into picture due to the mechanism of particle creation. For simplicity, entropy flow is considered only due to heat conduction. Further, due to Maxwell-Cattaneo modified Fourier law for non-equilibrium phenomenon, the temperature satisfies damped wave equation instead of heat conduction equation. Validity of generalized second law of thermodynamics (GSLT) has been investigated for Universe bounded by apparent or event horizon with cosmic substrutum as perfect fluid with constant or variable equation of state or interacting dark species. Finally, we have used three Planck data sets to constrain the thermal conductivity \\lambda and the coupling parameter b^2. These constraints must be satisfied in order for GSLT to hold for Universe bounded by apparent or event horizons.

Subhajit Saha; Atreyee Biswas; Subenoy Chakraborty

2014-04-04T23:59:59.000Z

257

Planck Scale Cosmology and Asymptotic Safety in Resummed Quantum Gravity  

E-Print Network [OSTI]

In Weinberg's asymptotic safety approach, a finite dimensional critical surface for a UV stable fixed point generates a theory of quantum gravity with a finite number of physical parameters. We argue that, in an extension of Feynman's original formulation of the theory, we recover this fixed-point UV behavior from an exact re-arrangement of the respective perturbative series. Our results are consistent with the exact field space Wilsonian renormalization group results of Reuter {\\it et al.} and with recent Hopf- algebraic Dyson-Schwinger renormalization theory results of Kreimer. We obtain the first "first principles" predictions of the dimensionless gravitational and cosmological constants and our results support the Planck scale cosmology of Bonanno and Reuter. We conclude with an estimate for the currently observed value of the cosmological constant.

B. F. L. Ward

2010-12-13T23:59:59.000Z

258

Elastic properties of superconducting MAX phases from first principles calculations  

E-Print Network [OSTI]

Using first-principles density functional calculations, a systematic study on the elastic properties for all known superconducting MAX phases (Nb2SC, Nb2SnC, Nb2AsC, Nb2InC, Mo2GaC and Ti2InC) was performed. As a result, the optimized lattice parameters, independent elastic constants, indicators of elastic anisotropy and brittle/ductile behavior as well as the so-called machinability indexis were calculated. We derived also bulk and shear moduli, Young's moduli, and Poisson's ratio for ideal polycrystalline MAX aggregates. The results obtained were discussed in comparison with available theoretical and experimental data and elastic parameters for other layered superconductors.

I. R. Shein; A. L. Ivanovskii

2010-06-03T23:59:59.000Z

259

Hypersonic expansion of the Fokker--Planck equation  

SciTech Connect (OSTI)

A systematic study of the hypersonic limit of a heavy species diluted in a much lighter gas is made via the Fokker--Planck equation governing its velocity distribution function. In particular, two different hypersonic expansions of the Fokker--Planck equation are considered, differing from each other in the momentum equation of the heavy gas used as the basis of the expansion: in the first of them, the pressure tensor is neglected in that equation while, in the second expansion, the pressure tensor term is retained. The expansions are valid when the light gas Mach number is O(1) or larger and the difference between the mean velocities of light and heavy components is small compared to the light gas thermal speed. They can be applied away from regions where the spatial gradient of the distribution function is very large, but it is not restricted with respect to the temporal derivative of the distribution function. The hydrodynamic equations corresponding to the lowest order of both expansions constitute two different hypersonic closures of the moment equations. For the subsequent orders in the expansions, closed sets of moment equations (hydrodynamic equations) are given. Special emphasis is made on the order of magnitude of the errors of the lowest-order hydrodynamic quantities. It is shown that if the heat flux vanishes initially, these errors are smaller than one might have expected from the ordinary scaling of the hypersonic closure. Also it is found that the normal solution of both expansions is a Gaussian distribution at the lowest order.

Fernandez-Feria, R.

1989-02-01T23:59:59.000Z

260

A New Approach to Computing Max Flows using Electrical Flows  

E-Print Network [OSTI]

A New Approach to Computing Max Flows using Electrical Flows Yin Tat Lee (MIT) Satish Rao (UC-Kelner-Madry-Spielman-Teng'11]: approximate flow in time Uses electrical flows. 7 #12;Electrical Flows 3 1 S t 8 #12;Electrical Flows Identify Graph with Resistor Network R(e)=1/w(e) 1/3 S t 1 9 #12;Electrical Flows Electrical flow

Rajamani, Sriram K.

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

Hamilton Eye Institute Neuroscience Institute  

E-Print Network [OSTI]

Care Neonatology & Maternal Fetal Pediatric Heart Institute Steve J. Schwab, MD Musculoskeletal A New of Radiology · Mari Assumes Leadership of OB/GYN city attractioNs Levitt Shell Revived Feature Vision

Cui, Yan

262

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

ScienceCinema (OSTI)

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.

Craig Hogan

2010-01-08T23:59:59.000Z

263

RATAN-600 and PLANCK Mission: new results after First General Meeting  

E-Print Network [OSTI]

We present activity at RATAN-600 connected with future PLANCK mission. It includes special radio telescope upgrading, multi-frequencies observations in the 0.6GHz-30GHz band with 40 channels, new results, connected with synchrotron, spinning dust and polarized Galaxy emission at small scales. Much lower limits were found than expected before the First Planck meeting. New deep sub-mJy survey of the 100 sq.deg. field at cm. waves demonstrated, that NVSS objects will dominate at LFI frequencies, and new, invisible by NVSS population will be below PLANCK sensitivity limit with only few exceptions. Preparation to the next generation experiments, connected with PLANCK mission we describe as well. They include high l polarization, SZ- blind survey, and test observations of the cosmological highly redshifted lines at small scales.

Yu. Parijskij; I. Novikov

2004-02-17T23:59:59.000Z

264

Design and Analysis of Stochastic Dynamical Systems with Fokker-Planck Equation  

E-Print Network [OSTI]

Monte-Carlo techniques. Spectral analysis of the discretized Fokker- Planck operator, followed by spurious mode rejection is employed to construct a new semi-analytical algorithm to obtain near real-time approximations of transient FPE response of high...

Kumar, Mrinal

2011-02-22T23:59:59.000Z

265

Does the measured value of the Planck constant depend on the energy of measurements?  

E-Print Network [OSTI]

The measurement of the Avogadro constant opened the way to a comparison of the watt-balance measurements of the Planck constant with the values calculated from the quotients of the Planck constant and the mass of a particle or an atom. Since the energy scales of these measurements span nine energy decades, these data provide insight into the consistency of our understanding of physics.

Massa, Enrico; Jentschel, Michael

2011-01-01T23:59:59.000Z

266

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 Home5b9fcbce19 No revision hasInformation Earth's Heat JumpIncMAKGalwayHydrothermal System,WindMaxWest Environmental Systems

267

Property:Incentive/WindResPercMax | 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 CenterFranconia, Virginia: Energy ResourcesLoadingPenobscot County,ContAddr2 Jump to: navigation,PVYears Jump to:TechDsc JumpWindResPercMax

268

Planck Early Results: The Low Frequency Instrument data processing  

E-Print Network [OSTI]

We describe the data processing pipeline employed by the Low Frequency Instrument (LFI) Data Processing Centre (DPC) to create and characterize the frequency maps used by the ERCSC (Early Release Compact Source Catalogue) first product of Planck to become public. In particular, we discuss the various steps involved in reducing the data, starting from telemetry (TM)packets through to the production of cleaned calibrated timelines and calibrated frequency maps. Data are continuously calibrated using the modulation induced on the mean temperature of the Cosmic Microwave Background Radiation by the proper motion of the spacecraft. The sky signals other than the dipole are removed by an iterative procedure based on simultaneous fitting of calibration parameters and sky maps. Noise properties are estimated from time-ordered data where the sky signal is removed using a Generalized Least Square map-making algorithm. The measured 1/f noise knee-frequencies range from \\sim 100 mHz at 30 GHz to a few tens of mHz at 70 G...

Zacchei, A; Baccigalupi, C; Bersanelli, M; Bonaldi, A; Bonavera, L; Burigana, C; Butler, R C; Cuttaia, F; de Zotti, G; Dick, J; Frailis, M; Galeotta, S; Gonzlez-Nuevo, J; Grski, K M; Gregorio, A; Keihnen, E; Keskitalo, R; Knoche, J; Kurki-Suonio, H; Lawrence, C R; Leach, S; Leahy, J P; Lpez-Caniego, M; Mandolesi, N; Maris, M; Matthai, F; Meinhold, P R; Mennella, A; Morgante, G; Morisset, N; Natoli, P; Pasian, F; Perrotta, F; Polenta, G; Poutanen, T; Reinecke, M; Ricciardi, S; Rohlfs, R; Sandri, M; Suur-Uski, A -S; Tauber, J A; Tavagnacco, D; Terenzi, L; Tomasi, M; Valiviita, J; Villa, F; Zonca, A; Banday, A J; Barreiro, R B; Bartlett, J G; Bartolo, N; Bedini, L; Bennett, K; Binko, P; Borrill, J; Bouchet, F R; Bremer, M; Cabella, P; Cappellini, B; Chen, X; Colombo, L; Cruz, M; Curto, A; Danese, L; Davies, R D; Davis, R J; de Gasperis, G; de Rosa, A; de Troia, G; Dickinson, C; Diego, J M; Donzelli, S; Drl, U; Efstathiou, G; En\\sslin, T A; Eriksen, H K; Falvella, M C; Finelli, F; Franceschi, E; Gaier, T C; Gasparo, F; Gnova-Santos, R T; Giardino, G; Gmez, F; Gruppuso, A; Hansen, F K; Hell, R; Herranz, D; Hovest, W; Jewell, J; Juvela, M; Kisner, T S; Knox, L; Lhteenmki, A; Lamarre, J -M; Leonardi, R; Len-Tavares, J; Lilje, P B; Lubin, P M; Maggio, G; Marinucci, D; Martnez-Gonzlez, E; Massardi, M; Matarrese, S; Meharga, M T; Melchiorri, A; Migliaccio, M; Mitra, S; Moss, A; N\\orgaard-Nielsen, H U; Pagano, L; Paladini, R; Paoletti, D; Partridge, B; Pearson, D; Pettorino, V; Pietrobon, D; Przeau, G; Procopio, P; Puget, J -L; Quercellini, C; Rachen, J P; Rebolo, R; Robbers, G; Rocha, G; Rubi\; Salerno, E; Savelainen, M; Scott, D; Seiffert, M D; Silk, J I; Smoot, G F; Sternberg, J; Stivoli, F; Stompor, R; Tofani, G; Tuovinen, J; Trler, M; Umana, G; Vielva, P; Vittorio, N; Vuerli, C; Wade, L A; Watson, R; White, S D M; Wilkinson, A

2011-01-01T23:59:59.000Z

269

On the Einstein-Cartan cosmology vs. Planck data  

E-Print Network [OSTI]

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.

Davor Palle

2014-05-14T23:59:59.000Z

270

Reconciliation of High Energy Scale Models of Inflation with Planck  

E-Print Network [OSTI]

The inflationary cosmology paradigm is very successful in explaining the CMB anisotropy to the percent level. Besides the dependence on the inflationary model, the power spectra, spectral tilt and non-Gaussianity of the CMB temperature fluctuations also depend on the initial state of inflation. Here, we examine to what extent these observables are affected by our ignorance in the initial condition for inflationary perturbations, due to unknown new physics at a high scale $M$. For initial states that satisfy constraints from backreaction, we find that the amplitude of the power spectra could still be significantly altered, while the modification in bispectrum remains small. For such initial states, $M$ has an upper bound of a few tens of $H$, with $H$ being the Hubble parameter during inflation. We show that for $M\\sim 20 H$, such initial states always (substantially) suppress the tensor to scalar ratio. In particular we show that a general choice of initial conditions can satisfactorily reconcile the simple $1/2 m^2 \\phi^2$ chaotic model with the Planck data.

Amjad Ashoorioon; Konstantinos Dimopoulos; M. M. Sheikh-Jabbari; Gary Shiu

2014-02-06T23:59:59.000Z

271

Deciding Unambiguity and Sequentiality from a Finitely Ambiguous MaxPlus Automaton  

E-Print Network [OSTI]

­anneau max­plus. Le r??esultat principal est le suivant : on peut d??ecider si une s??erie reconnue par unDeciding Unambiguity and Sequentiality from a Finitely Ambiguous Max­Plus Automaton Ines Klimann with weights in the max­plus semiring are considered. The main result is: it is decidable whether a series

Fondements et Applications, Université Paris 7

272

Reducible spectral theory with applications to the robustness of matrices in max algebra  

E-Print Network [OSTI]

.Butkoviµcy R.A.Cuninghame-Greenz S.Gaubertx July 25, 2008 Abstract Let a b = max(a; b) and a b = a + b for a; b 2 R := R [ f 1g. By max-algebra we understand the analogue of linear algebra developed for the pair: The max-algebraic eigenvalue-eigenvector problem is the following: Given A 2 R n n , ...nd all 2 R and x 2

Butkovic, Peter

273

CSR EXPANSIONS OF MATRIX POWERS IN MAX ALGEBRA SERGEi SERGEEV AND HANS SCHNEIDER  

E-Print Network [OSTI]

that for t 3n2, the powers At can be expanded in max-algebraic sums of terms of the form CStR, where C and R the max-times semiring Rmax,? which is the set of nonnegative numbers R+ equipped with the operations-algebraic powers of nonnegative matrices, the main object of our study. The max-plus semiring Rmax,+ = (R

Schneider, Hans

274

Non-linear programs with max-linear constraints: A heuristic approach  

E-Print Network [OSTI]

5, 2009 Abstract Let a b = max(a, b) and a b = a + b for a, b R and extend the pair of operations = max(a, b) and a b = a + b for a, b R and extend the pair of operations to matrices and vectors bkj = maxk(aik + bkj) for all i, j. Also, if R then A = ( aij). Max-algebra has been studied

Butkovic, Peter

275

MaxWeber,"ScienceasaVocation" 'WissenschaftalsBeruf,'fromGesammlteAufsaetzezurWissenschaftslehre(Tubingen,  

E-Print Network [OSTI]

MaxWeber,"ScienceasaVocation" 'Wissenschaftals a sort of moral right to expect some consideration. He also #12;Weber,"ScienceasVocation" 2

Goldreich, Oded

276

Cosmological Constraints from the SDSS maxBCG Cluster Catalog  

SciTech Connect (OSTI)

We use the abundance and weak lensing mass measurements of the SDSS maxBCG cluster catalog to simultaneously constrain cosmology and the richness-mass relation of the clusters. Assuming a flat {Lambda}CDM cosmology, we find {sigma}{sub 8}({Omega}{sub m}/0.25){sup 0.41} = 0.832 {+-} 0.033 after marginalization over all systematics. In common with previous studies, our error budget is dominated by systematic uncertainties, the primary two being the absolute mass scale of the weak lensing masses of the maxBCG clusters, and uncertainty in the scatter of the richness-mass relation. Our constraints are fully consistent with the WMAP five-year data, and in a joint analysis we find {sigma}{sub 8} = 0.807 {+-} 0.020 and {Omega}{sub m} = 0.265 {+-} 0.016, an improvement of nearly a factor of two relative to WMAP5 alone. Our results are also in excellent agreement with and comparable in precision to the latest cosmological constraints from X-ray cluster abundances. The remarkable consistency among these results demonstrates that cluster abundance constraints are not only tight but also robust, and highlight the power of optically-selected cluster samples to produce precision constraints on cosmological parameters.

Rozo, Eduardo; /CCAPP; Wechsler, Risa H.; /KIPAC, Menlo Park /SLAC; Rykoff, Eli S.; /UC, Santa Barbara; Annis, James T.; /Fermilab; Becker, Matthew R.; /Chicago U. /KICP, Chicago; Evrard, August E.; /Michigan U. /Michigan U., MCTP; Frieman, Joshua A.; /Fermilab /KICP, Chicago /Chicago U.; Hansen, Sarah M.; /UC, Santa Cruz; Hao, Jia; /Michigan U.; Johnston, David E.; /Northwestern U.; Koester, Benjamin P.; /KICP, Chicago /Chicago U.; McKay, Timothy A.; /Michigan U. /Michigan U., MCTP; Sheldon, Erin S.; /Brookhaven; Weinberg, David H.; /CCAPP /Ohio State U.

2009-08-03T23:59:59.000Z

277

A&A 552, L3 (2013) DOI: 10.1051/0004-6361/201321080  

E-Print Network [OSTI]

, knowing the maximum possible energy of solar energetic par- ticle (SEP) events and the frequency Observatory (Oulu unit) and Physics Dept., University of Oulu, 99600 Sodankylä, Finland e-mail: Ilya Planck Institute for Solar System Research, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany 8 School

Usoskin, Ilya G.

278

MSC-E Technical Report 1/2003 Intercomparison Study of Numerical Models for  

E-Print Network [OSTI]

-Planck-Strasse 1, D-21502 Geesthacht Germany fax: 49 41 52 87 23 66 e-mail: ebinghaus@dvmc10.gkss.de Ilia ILYIN - Research Centre, Institute of Hydrophysics Max-Planck-Strasse 1 D-21502 Geesthacht GERMANY tel: 49 41 52 87

279

Efficient SIMD technique with parallel Max-Log-MAP Algorithm for Turbo Decoders  

E-Print Network [OSTI]

Efficient SIMD technique with parallel Max-Log-MAP Algorithm for Turbo Decoders David Gnaedig Turbo on a DSP a parallel Max-Log-MAP algorithm for turbo decoders. It consists in using SIMD instructions by the use of an adapted two-dimensional turbo code and its parallel interleaver structure. After a brief

Paris-Sud XI, Université de

280

Max-min Fair Rate Allocation and Routing in Energy Harvesting Networks: Algorithmic Analysis  

E-Print Network [OSTI]

Max-min Fair Rate Allocation and Routing in Energy Harvesting Networks: Algorithmic Analysis Jelena@ee}.columbia.edu ABSTRACT This paper considers max-min fair rate allocation and rout- ing in energy harvesting networks energy profile and focus on the design of efficient and opti- mal algorithms that can serve as benchmarks

Hone, James

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

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

E-Print Network [OSTI]

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

Ohta, Shigemi

282

Visualization in max algebra: An application of diagonal scaling of matrices.  

E-Print Network [OSTI]

Visualization in max algebra: An application of diagonal scaling of matrices. Hans Schneider Schneider with some results from joint work with Peter Butkovic and Sergei SergeevVisualization in max > 0 Definition path in G(A) i(0) i(1) · · · i(k) (i, j), ((i, j; r)) path from i to j (length r

Schneider, Hans

283

An 0.5-Approximation Algorithm for MAX DICUT with Given Sizes of Parts  

E-Print Network [OSTI]

An 0.5-Approximation Algorithm for MAX DICUT with Given Sizes of Parts Alexander Ageev Refael Hassin Maxim Sviridenko Abstract Given a directed graph G and an edge weight function w : E(G) R+, the maximum directed cut problem (max dicut) is that of finding a directed cut (X) with maximum total weight

Atkinson, Katie

284

Journal de la Socit Franaise de Statistique Spatial extremes: Max-stable processes at work  

E-Print Network [OSTI]

and conditional simulation of max-stable processes. The paper ends with the modeling of extreme wind gustsSubmission Journal de la Société Française de Statistique Spatial extremes: Max-stable processes many developments to the functional extreme value theory have been made during the last decades

Ribatet, Mathieu

285

Seaborg 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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLas ConchasPassiveSubmitted forHighlights Nuclear PhysicsDo you seeunseenScottScottInstitute

286

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...

287

Planck Scale Induced Speed of Sound in a Trapped Bose-Einstein Condensate  

E-Print Network [OSTI]

In the present work, we analyze the corrections caused by an anomalous dispersion relation, suggested in several quantum gravity models, upon the speed of sound in a weakly interacting Bose--Einstein Condensate, trapped in a potential of the form $V(r)\\sim r^{2}$. We show that the corresponding ground state energy and consequently, the associated speed of sound, present corrections respect to the usual case, which may be used to explore the sensitivity to Planck--scale effects on these relevant properties associated with the condensate. Indeed, we stress that this type of macroscopic bodies may be more sensitive, under certain conditions, to Planck--scale manifestations than its constituents. In addition, we prove that the inclusion of a trapping potential, together with many--body contributions, improves the sensitivity to Planck--scale signals, compared to the homogeneous system.

E. Castellanos; J. I. Rivas; V. Domnguez-Rocha

2014-07-11T23:59:59.000Z

288

Planck early results: Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources  

E-Print Network [OSTI]

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact Source Catalog (ERCSC) and simultaneous multifrequency data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous observations ranging from radio to gamma-rays. This is the first extensive frequency coverage in the radio and millimetre domains for an essentially complete sample of extragalactic radio sources, and it shows how the individual shocks, each in their own phase of development, moving in the relativistic jet, shape the radio spectra. The SEDs presented in this paper were fitted with second and third degree polynomials to estimate the frequencies of the synchrotron and inverse Compton (IC) peaks, and the spectral indices of low and high frequency radio data, including the Planck ERCSC data, were calculated. SED modelling methods are discussed, with an emphasis on proper, physical modelli...

Aatrokoski, J; Aghanim, N; Aller, H D; Aller, M F; Angelakis, E; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Balbi, A; Banday, A J; Barreiro, R B; Bartlett, J G; Battaner, E; Benabed, K; Benot, A; Berdyugin, A; Bernard, J -P; Bersanelli, M; Bhatia, R; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Burrows, D N; Cabella, P; Capalbi, M; Cappellini, B; Cardoso, J -F; Catalano, A; Cavazzuti, E; Cayn, L; Challinor, A; Chamballu, A; Chary, R -R; Chiang, L -Y; Christensen, P R; Clements, D L; Colafrancesco, S; Colombi, S; Couchot, F; Coulais, A; Cutini, S; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Gasperis, G; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Dickinson, C; Dole, H; Donzelli, S; Dor, O; Drl, U; Douspis, M; Dupac, X; Efstathiou, G; Enlin, T A; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Fuhrmann, L; Galeotta, S; Ganga, K; Gargano, F; Gasparrini, D; Gehrels, N; Giard, M; Giardino, G; Giglietto, N; Giommi, P; Giordano, F; Giraud-Hraud, Y; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Harrison, D; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hovest, W; Hoyland, R J; Huffenberger, K M; Jaffe, A H; Juvela, M; Keihnen, E; Keskitalo, R; King, O; Kisner, T S; Kneissl, R; Knox, L; Krichbaum, T P; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Laureijs, R J; Lavonen, N; Lawrence, C R; Leach, S; Leonardi, R; Len-Tavares, J; Linden-V\\ornle, M; Lindfors, E; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maffei, B; Maino, D; Mandolesi, N; Mann, R; Maris, M; Martnez-Gonzlez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Max-Moerbeck, W; Mazziotta, M N; Mazzotta, P; Melchiorri, A; Mendes, L; Mennella, A; Michelson, P F; Mingaliev, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Monte, C; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, A; Naselsky, P; Natoli, P; Nestoras, I; Netterfield, C B; Nieppola, E; Nilsson, K; N\\orgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; O'Dwyer, I J; Osborne, S; Pajot, F; Partridge, B; Pasian, F; Patanchon, G; Pavlidou, V; Pearson, T J; Perdereau, O; Perotto, L; Perri, M; Perrotta, F; Piacentini, F; Piat, M; Plaszczynski, S; Platania, P; Pointecouteau, E; Polenta, G; Ponthieu, N; Poutanen, T; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rain, S; Reach, W T; Readhead, A; Rebolo, R; Reeves, R; Reinecke, M; Reinthal, R; Renault, C; Ricciardi, S; Richards, J; Riller, T; Riquelme, D; Ristorcelli, I; Rocha, G; Rosset, C; Rowan-Robinson, M; Rubi\; Rusholme, B; Saarinen, J; Sandri, M; Savolainen, P; Scott, D; Seiffert, M D; Sievers, A; Sillanp, A; Smoot, G F; Sotnikova, Y; Starck, J -L; Stevenson, M; Stivoli, F; Stolyarov, V; Sudiwala, R; Sygnet, J -F; Takalo, L; Tammi, J; Tauber, J A; Terenzi, L; Thompson, D J; Toffolatti, L; Tomasi, M; Tornikoski, M; Torre, J -P; Tosti, G; Tramacere, A; Tristram, M; Tuovinen, J; Trler, M; Turunen, M; Umana, G; Ungerechts, H; Valenziano, L; Valtaoja, E; Varis, J; Verrecchia, F; Vielva, P; Villa, F; Vittorio, N; Wandelt, B D; Wu, J; Yvon, D; Zacchei, A; Zensus, J A; Zhou, X; Zonca, A

2011-01-01T23:59:59.000Z

289

Burak Yuksel Information  

E-Print Network [OSTI]

Vehicles. Web · Max Planck Institute, Personal Webpage · Personal Webpage Education Istanbul Technical University, Istanbul, Turkey M.Sc., Control and Automation Engineering, June 2012, GPA: 3.94/4.00 · TopicD. Research Assistant July 2012 to April 2013 Motion Perception and Vehicle Simulation Research Group, Max

290

CURRICULUM VITAE Svante Pbo  

E-Print Network [OSTI]

of Munich, Germany. 1997- Director, Max-Planck-Institute for Evolutionary Anthropology, Leipzig, Germany. 1999- Honorary Professor of Genetics and Evolutionary Biology, University of Leipzig, Germany. 2003 Lecture, Heidelberg, Germany. 1998 Member, Academia Europaea. Max Delbrück Medal, Berlin, Germany. 1999

Pääbo, Svante

291

Higher order mixed moment approximations for the Fokker-Planck equation in one space dimension  

E-Print Network [OSTI]

We study mixed-moment models (full zeroth moment, half higher moments) for a Fokker-Planck equation in one space dimension. Mixed-moment minimum-entropy models are known to overcome the zero net-flux problem of full-moment minimum entropy Mn models. Realizability theory for these mixed moments of arbitrary order is derived, as well as a new closure, which we refer to as Kershaw closures. They provide non-negative distribution functions combined with an analytical closure. Numerical tests are performed with standard first-order finite volume schemes and compared with a finite-difference Fokker-Planck scheme.

Florian Schneider; Graham Alldredge; Martin Frank; Axel Klar

2014-05-21T23:59:59.000Z

292

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

E-Print Network [OSTI]

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

Straube, Arthur V.

293

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

E-Print Network [OSTI]

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 equilibrium there will be no production of entropy. A non- equilibrium thermodynamic system in the stationary

de Oliveira, Mário José

294

Fokker-Planck Equation and Path Integral Representation of Fractional Ornstein-Uhlenbeck Process with Two Indices  

E-Print Network [OSTI]

This paper considers the Fokker-Planck equation and path integral formulation of the fractional Ornstein-Uhlenbeck process parametrized by two indices. The effective Fokker-Planck equation of this process is derived from the associated fractional Langevin equation. Path integral representation of the process is constructed and the basic quantities are evaluated.

C. H. Eab; S. C. Lim

2014-09-19T23:59:59.000Z

295

Intracellular Measurements of Spatial Integration and the MAX Operation in Complex Cells of the Cat Primary Visual Cortex  

E-Print Network [OSTI]

Intracellular Measurements of Spatial Integration and the MAX Operation in Complex Cells of the Cat. Intracellular measurements of spatial integration and the MAX operation in complex cells of the cat primary by a maximum operation (MAX)-like computation, as suggested by Riesenhuber and Poggio's model of object

Riesenhuber, Maximilian

296

The Singular-Value Decomposition in the Extended Max Algebra* Bart De Schutter+ and Bart De Moor*  

E-Print Network [OSTI]

numbers and the extended max algebra to define the sing&r-value decomposition of a matrix in the extendedThe Singular-Value Decomposition in the Extended Max Algebra* Bart De Schutter+ and Bart De Moor ABSTRACT First we establish a connection between the field of the real numbers and the extended max algebra

297

A summary of the Planck constant measurements using a watt balance with a superconducting solenoid at NIST  

E-Print Network [OSTI]

Researchers at the National Institute of Standards and Technology have been using a watt balance, NIST-3, to measure the Planck constant $h$ for over ten years. Two recently published values disagree by more than one standard uncertainty. The motivation for the present manuscript is twofold. First, we correct the latest published number to take into account a recently discovered systematic error in mass dissemination at the Bureau International des Poids et Mesures (BIPM). Second, we provide guidance on how to combine the two numbers into one final result. In order to adequately reflect the discrepancy, we added an additional systematic uncertainty to the published uncertainty budgets. The final value of $h$ measured with NIST-3 is $h = 6.626\\,069\\,36(37)\\times 10^{-34}\\,\\mbox{J\\,s}$. This result is $77(57) \\times 10^{-9}$ fractionally higher than $h_{\\mathrm{90}}$. Each number in parentheses gives the value of the standard uncertainty in the last two digits of the respective value and $h_{\\mathrm{90}}$ is th...

Schlamminger, S; Haddad, D; Newell, D B; Seifert, F; Chao, L S; Liu, R; Williams, E R; Pratt, J R

2015-01-01T23:59:59.000Z

298

Institute of Design Institute of Design  

E-Print Network [OSTI]

Institute of Design Institute of Design 350 N. LaSalle St. Chicago, IL 60610 312.595.4900 design The Institute of Design has continuously explored emerg- ing ideas about how design interacts with society languages and use of new media and material. The school was renamed the Institute of Design (ID) in 1944

Heller, Barbara

299

Poisson-Nernst-Planck systems for narrow tubular-like membrane and Bixiang Wang  

E-Print Network [OSTI]

membrane channels, transport of holes and electrons in semiconductors (see, e.g., [1, 2, 24, 4, 6, 7, 8, 17, 25]). In the context of ion flow through membrane channels, it is physicallyPoisson-Nernst-Planck systems for narrow tubular-like membrane channels Weishi Liu and Bixiang Wang

Liu, Weishi

300

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

E-Print Network [OSTI]

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

Peinke, Joachim

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Consistency tests for Planck and WMAP in the low multipole domain  

SciTech Connect (OSTI)

Recently, full sky maps from Planck have been made publicly available. In this paper, we do consistency tests for the three Planck CMB sky maps. We assume that the difference between two maps represents the contributions from systematics, noise, foregrounds and other sources, and that a precise representation of the Cosmic Microwave Background should be uncorrelated with it. We investigate the cross correlation in pixel space between the difference maps and the various Planck maps and find no significant correlations, in comparison to 10000 random Gaussian simulated maps. Additionally we investigate the difference map between the WMAP ILC 9 year map and the ILC 7 year map. We perform cross correlations between this difference map, and the ILC9 and ILC7, and find significant correlations only for the ILC9, at more than the 99.99% level. Likewise, a comparison between the Planck NILC map and the WMAP ILC9 map, shows a strong correlation for the ILC9 map with the difference map, also at more than the 99.99% level. Thus the ILC9 appears to be more contaminated than the ILC7, which should be taken into consideration when using WMAP maps for cosmological analyses.

Frejsel, A.; Hansen, M.; Liu, H., E-mail: frejsel@nbi.dk, E-mail: kirstejn@nbi.dk, E-mail: liuhao@nbi.dk [Niels Bohr Institute and Discovery Center, Blegdamsvej 17, 2100 Copenhagen (Denmark)

2013-06-01T23:59:59.000Z

302

Tunnel effect and symmetries for Kramers Fokker-Planck type operators  

E-Print Network [OSTI]

- values. R´esum´e Nous ´etudions des op´erateurs de type Kramers-Fokker-Planck dans la lim- ite semi are real and exponentially small, and establish the complete semiclassical asymptotics for these eigen ´etablissons leur asymp- totique semi-classique compl`ete. Contents 1 Introduction 3 2 Review of some results

Hérau, Frédéric

303

The Excellence Initiative of the German Federal Ministry of Education and Research and the German Research Foundation  

E-Print Network [OSTI]

Mikrotechnik Mainz, Max-Planck-Institute for Polymer Research, Fraunhofer-Institute for Structural Du- rability and System Reliability, Deutsches Kunststoff-Institut). The Center of Smart Interfaces focuses on phase of Smart Interfaces Experimental Interface Physics #12;Innovative Environment Workforce: 1 Research group

Haller-Dintelmann, Robert

304

Criteria for Annotation of Plant MicroRNAs Blake C. Meyers,a,1 Michael J. Axtell,b,1 Bonnie Bartel,c David P. Bartel,d David Baulcombe,e John L. Bowman,f  

E-Print Network [OSTI]

of Biology, Massachusetts Institute of Technology, Whitehead Institute, Cambridge, Massachusetts 02142 e, Tokyo 153-8902, Japan r Department of Molecular Biology, Max Planck Institute for Developmental Biology in plants and animals were spelled out by a group of leading laboratories in the small RNA field (Ambros et

Bartel, David

305

5, 10751099, 2014 Uncertainty in crop  

E-Print Network [OSTI]

Resources and Energy Directorate, Oslo, Norway 16 International Institute for Applied System Analysis, New York, USA 24 Institute for Sustainable Economic Development, Vienna, Austria 25 Max Planck of Bonn, Bonn, Germany 28 Santa Fe Institute, Santa Fe, New Mexico, USA Received: 28 July 2014 ­ Accepted

Levermann, Anders

306

Supervised Learning of Image Restoration with Convolutional Networks Viren Jain1  

E-Print Network [OSTI]

Institute of Technology, Cambridge, MA, USA 2 Howard Hughes Medical Institute, Cambridge, MA, USA 3 Biomedical Optics, Max Planck Institute for Medical Research, Heidelberg, Germany Abstract Convolutional, the images are clean enough to be used for segmentation, whereas the other approaches fail in this respect

Gabrieli, John

307

SpeeDP: A new algorithm to compute the SDP relaxations of Max ...  

E-Print Network [OSTI]

Oct 15, 2010 ... matrix A of a weighted graph G = (V,E), the Max-Cut problem calls for a ...... Further, in [21] the authors report a comparison of a matlab.

2010-10-15T23:59:59.000Z

308

An Approximation Algorithm for Max-Min Fair Allocation of Indivisible Goods  

E-Print Network [OSTI]

Saberi Abstract In this paper, we give the first approximation algorithm for the problem of max-min fair 94305. Email:{asadpour,saberi}@stanford.edu. 1 #12;1 Introduction Fair division, also known as the cake

Saberi, Amin

309

The NanoMax-TSTM three-axis stage offers an unmatched combination of  

E-Print Network [OSTI]

555 Spacer Block to Raise Optical- Axis Height to 125-mm 17 AMA 554 ©2002 MELLES GRIOT MCE 1042 03 holes threaded M2 on 20 centers dimensions: millimeters 17 MAX 302 3-axis stage MELLES GRIOT

Kik, Pieter

310

Training the Recurrent neural network by the Fuzzy Min-Max algorithm for fault prediction  

SciTech Connect (OSTI)

In this paper, we present a training technique of a Recurrent Radial Basis Function neural network for fault prediction. We use the Fuzzy Min-Max technique to initialize the k-center of the RRBF neural network. The k-means algorithm is then applied to calculate the centers that minimize the mean square error of the prediction task. The performances of the k-means algorithm are then boosted by the Fuzzy Min-Max technique.

Zemouri, Ryad [Laboratoire d'automatique, CNAM, 21 rue Pinel, 75013 Paris (France); Racoceanu, Daniel [IPAL, UMI CNRS 2955, UJF, I2R/A-STAR, NUS, 1 Fusionopolis Way, 21-01 Connexis, 138632 Singapore (Singapore); Zerhouni, Noureddine [FEMTO-ST-UMR CNRS 6174, ENSMM, UFC, UTBM, 32 Avenue de l'Observatoire, 25044 Besancon (France); Minca, Eugenia [Faculty of Electric Engineering, Valahia University, Bd. Unirii, nr. 18, 0200, Targoviste (Romania); Filip, Florin [Romanian Academy, Calea Victoriei 125, Sct. 1, Bucuresti (Romania)

2009-03-05T23:59:59.000Z

311

Institute of Design Institute of Design  

E-Print Network [OSTI]

Institute of Design Institute of Design 350 N. LaSalle St. Chicago, IL 60610 312.595.4900 main 312.595.4906 graduate study information 312.595.4901 fax design@id.iit.edu www.id.iit.edu Dean: Patrick F. Whitney The Institute of Design (ID) is defined by a legacy of experimentation joined with unique academic programs

Heller, Barbara

312

"Energetic" Theories of Culture by Max Weber (Translation)  

E-Print Network [OSTI]

and chemical bonding and all that is related to it concerning the concept of "solutions" in contrast to "com pounds," something about electrochemical problems, or something about isomerism that is to be found in the mostly so meager parts of the older... much richer conceptualization of the problem oriented above all else upon economics. So since the Institute under Waxweiler's direction has applied itself to really more worthwhile work, one can surely hope that these "energetic" reminiscences will soon...

Mikkelsen, Jon Mark; Schwartz, Charles

1984-01-01T23:59:59.000Z

313

An Analog Cellular Automaton Model of Gravitation: Planck-Scale Black Holes Randall C. O'Reilly  

E-Print Network [OSTI]

An Analog Cellular Automaton Model of Gravitation: Planck-Scale Black Holes Randall C. O by Randall C. O'Reilly, initially published online at URL listed below on 12/28/05 (Dated: December 28, 2005

O'Reilly, Randall C.

314

Una interpretaci\\'on f\\'isica de la constante de Planck  

E-Print Network [OSTI]

According to the commonly accepted interpretation of Quantum Mechanics, it is only possible to talk about the existence of elementary particles when they are detected by an experiment or by a classical measurement device. This has led to distortions with regard to the objective existence of reality, since it would be necessary an observer to materialize the elementary particle. This issue is solved when the elementary particle is placed in permanent interaction with the rest of the universe, so its existence would not depend on any intelligent observer and thus the objective range of elementary particles would be recovered. This article explores the interaction between elementary particles and a background action field of stochastic character and it is also determined that the standard deviation of the particle-background field interaction is essentially the Planck constant, since the expressions of the energy according to the Planck postulate and the momentum according to the Louis de Broglie thesis follow i...

Alvarez-Samaniego, Wilson P; Moya-Alvarez, Douglas

2013-01-01T23:59:59.000Z

315

Detectability of Planck-Scale-Induced Blurring with Gamma-Ray Bursts  

E-Print Network [OSTI]

Microscopic fluctuations inherent to the fuzziness of spacetime at the Planck scale might accumulate in wavefronts propagating a cosmological distance and lead to noticeable blurring in an image of a pointlike source. Distant quasars viewed in the optical and ultraviolet with Hubble Space Telescope (HST} may show this weakly, and if real suggests a stronger effect should be seen for Gamma-Ray Bursts (GRBs) in X-rays and gamma-rays. Those telescopes, however, operate far from their diffraction limits. A description of how Planck-scale-induced blurring could be sensed at high energy, even with cosmic rays, while still agreeing with the HST results is discussed. It predicts dilated apparent source size and inflated uncertainties in positional centroids, effectively a threshold angular accuracy restricting knowledge of source location on the sky. These outcomes are found to be consistent with an analysis of the 10 highest-redshift GRB detections reported for the Fermi satellite. Confusion with photon cascade and ...

Steinbring, Eric

2015-01-01T23:59:59.000Z

316

Vol. 167: 25-36, 1998 MARINE ECOLOGY PROGRESS SERIES  

E-Print Network [OSTI]

Gewasserphysik, Max-Planck-Strasse, D-21502 Geesthacht, Germany ABSTRACT: Macrofaunal samples were collected

Dippner, Joachim W.

317

Biogeosciences, 5, 171201, 2008 www.biogeosciences.net/5/171/2008/  

E-Print Network [OSTI]

Research, GKSS Research Center, Geesthacht, Max-Planck-Str., 21502 Geesthacht, Germany 7Center for Hydro

Stramski, Dariusz

318

ELSEVIER Atmospheric Research 39 (1995) 91-111 ATMOSPHERIC  

E-Print Network [OSTI]

Geesthacht, Institutfiir Physik, Max-Planck-Strafle, D-21502 GeesthachtGermany Received 6 April 1994

Moelders, Nicole

319

4, 34533530, 2007 Particulate organic  

E-Print Network [OSTI]

Research, GKSS Research Center, Geesthacht, Max-Planck-Str., 21502 Geesthacht, Germany 7 Center for Hydro

Paris-Sud XI, Université de

320

On the accuracy of using Fokker Planck equation in heavy ion collision  

E-Print Network [OSTI]

Application of Fokker-Planck equation to heavy quark transport in the evolving medium created in heavy ion collision is critically scrutinised. We realise that the approach introduces a moderate uncertainty in drag and diffusion coefficients culminating in huge ambiguity in the theoretical prediction of nuclear modification factor $R_{AA}$. Quantitative estimation of the error is presented by considering recent developments in this field.

Dutta, Nirupam

2015-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

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

E-Print Network [OSTI]

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.

Timashev, Serge F

2008-01-01T23:59:59.000Z

322

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

E-Print Network [OSTI]

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.

Serge F. Timashev

2008-04-17T23:59:59.000Z

323

Searching for Traces of Planck-Scale Physics with High Energy Neutrinos  

E-Print Network [OSTI]

High energy cosmic neutrino observations provide a sensitive test of Lorentz invariance violation, which may be a consequence of quantum gravity theories. We consider a class of non-renormalizable, Lorentz invariance violating operators that arise in an effective field theory description of Lorentz invariance violation in the neutrino sector inspired by Planck-scale physics and quantum gravity models. We assume a conservative generic scenario for the redshift distribution of extragalactic neutrino sources and employ Monte Carlo techniques to describe superluminal neutrino propagation, treating kinematically allowed energy losses of superluminal neutrinos caused by both vacuum pair emission and neutrino splitting. We consider EFTs with both non-renormalizable CPT-odd and non-renormalizable CPT-even operator dominance. We then compare the spectra derived using our Monte Carlo calculations in both cases with the spectrum observed by IceCube in order to determine the implications of our results regarding Planck-scale physics. We find that if the drop off in the neutrino flux above ~2 PeV is caused by Planck scale physics, rather than by a limiting energy in the source emission, a potentially significant pileup effect would be produced just below the drop off energy in the case of CPT-even operator dominance. However, such a clear drop off effect would not be observed if the CPT-odd, CPT-violating term dominates.

Floyd W. Stecker; Sean T. Scully; Stefano Liberati; David Mattingly

2015-02-09T23:59:59.000Z

324

Towards more realistic Ion Cyclotron Resonance Heating Fokker-Planck modelling  

SciTech Connect (OSTI)

Recent theoretical work allows accounting for a number of effects previously not or not fully accounted for but potentially playing an important role to understand the wave-particle interaction underlying Ion Cyclotron Resonance Heating. In [1] a semi-analytical method was proposed to evaluate the dielectric response of a plasma to electromagnetic waves in the ion cyclotron domain of frequencies accounting for drift orbit effects in an axisymmetric tokamak. It relies on subdividing the orbit into elementary segments in which the integrations can be performed analytically or by tabulation. Using the coefficients evaluated using this semi-analytical method, a 3-D Fokker-Planck code is being developed. The underlying equations and their implementation, as well as some results of this new 3-D Fokker-Planck code are briefly presented. The adopted numerical resolution technique relies on a subdivision of the integration domain in tetrahedrons. This specific shape of the elementary volumes allows imposing the boundary conditions along curved surfaces - in particular the 'bi-local' conditions across the curved trapped/passing boundary connecting one trapped to two passing orbits - elegantly. Results are presented of Fokker-Planck modelling accounting for the actual electric field wave structure, particle orbits and tokamak geometry. A discussion is also provided on the feasibility of further upgrading the description.

Van Eester, D. [Laboratory for Plasma Physics, Association 'EURATOM - Belgian State', Koninklijke Militaire School - Ecole Royale Militaire, Trilateral Euregio Cluster, Brussels (Belgium)

2006-11-30T23:59:59.000Z

325

The Simultaneous Medicina-Planck Experiment (SiMPlE): data acquisition, reduction and first results  

E-Print Network [OSTI]

The Simultaneous Medicina-{\\it Planck} Experiment (SiMPlE) is aimed at observing a selected sample of 263 extragalactic and Galactic sources with the Medicina 32-m single dish radio telescope in the same epoch as the Planck satellite observations. The data acquired with a frequency coverage down to 5 GHz, also combined with Planck at frequencies above 30 GHz, will constitute a useful reference catalogue of bright sources over the whole Northern hemisphere. Furthermore, source observations performed in different epochs and comparison with other catalogues allow the investigation of source variabilities on different timescales. In this work, we describe the sample selection, the on-going data acquisition campaign, the data reduction procedures, the developed tools, and the comparison with other data-sets. We present the data at 5 and 8.3 GHz for the SiMPlE Northern Sample consisting of 79 sources with $\\delta \\geq 45^\\circ$ selected in our catalogue and observed during the first 6 months of the project. A first...

Procopio, P; Righini, S; Zanichelli, A; Ricciardi, S; Libardi, P; Burigana, C; Cuttaia, F; Mack, K -H; Terenzi, L; Villa, F; Bonavera, L; Morgante, G; Trigilio, C; Trombetti, T; Umana, G

2011-01-01T23:59:59.000Z

326

Petroleum Institute Scholarly Publications  

E-Print Network [OSTI]

Abu Dhabi The Petroleum Institute Scholarly Publications January 1st ­ December 31st 2007 #12;The Petroleum Institute Scholarly Publications January 1st ­ December 31st 2007 v #12;- 2 - Scholarly Publications 2007 | The Petroleum Institute #12;- 3 - Scholarly Publications 2007 | The Petroleum Institute

327

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

328

Using a MaxEnt Classifier for the Automatic Content Scoring of Free-Text Responses  

SciTech Connect (OSTI)

Criticisms against multiple-choice item assessments in the USA have prompted researchers and organizations to move towards constructed-response (free-text) items. Constructed-response (CR) items pose many challenges to the education community - one of which is that they are expensive to score by humans. At the same time, there has been widespread movement towards computer-based assessment and hence, assessment organizations are competing to develop automatic content scoring engines for such items types - which we view as a textual entailment task. This paper describes how MaxEnt Modeling is used to help solve the task. MaxEnt has been used in many natural language tasks but this is the first application of the MaxEnt approach to textual entailment and automatic content scoring.

Sukkarieh, Jana Z. [Educational Testing Service, Rosedale Road, Princeton NJ 08541 (United States)

2011-03-14T23:59:59.000Z

329

DIABETES, OBESITY AND METABOLISM INSTITUTE  

E-Print Network [OSTI]

DIABETES, OBESITY AND METABOLISM INSTITUTE AT NORTHWESTERN MEDICINE THE INSTITUTES AT NORTHWESTERN MEDICINE #12;THE INSTITUTES AT NORTHWESTERN MEDICINE DIABETES, OBESITY AND METABOLISM INSTITUTE AT NORTHWESTERN MEDICINE "As we launch the Diabetes, Obesity and Metabolism Institute at Northwestern Medicine, I

Engman, David M.

330

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]

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.

Asger G. Gasanalizade; Ramin A. Hasanalizade

2015-02-20T23:59:59.000Z

331

Direct observations of nitric oxide produced by energetic electron precipitation in1 to the Antarctic middle atmosphere2  

E-Print Network [OSTI]

Observation, Finnish Meteorological Institute, Helsinki, Finland.11 5 Max Planck Institut für Solar System (EEP) from the Earth's magnetosphere than by solar protons [Randall et al.,43 2005]. However, it is unclear which electron energy range is most important for44 stratospheric chemistry. At auroral

Otago, University of

332

State of the Arctic Coast 2010 Scientific Review and Outlook  

E-Print Network [OSTI]

International Permafrost Association Published by: Helmholtz-Zentrum Geesthacht LOICZ International Project Office Institute of Coastal Research Max-Planck-Strasse 1 D-21502 Geesthacht, Germany April 2011 The Land and financially supported by the Institute of Coastal Research, at the Helmholtz-Zentrum Geesthacht, Germany

Douglas, Thomas A.

333

3, 24652497, 2003 Nudged GCM tracer  

E-Print Network [OSTI]

et al. Title Page Abstract Introduction Conclusions References Tables Figures Back Close Full Screen, The Netherlands 2 Space Research Organisation of the Netherlands (SRON), Utrecht, The Netherlands 3 Royal Netherlands Meteorological Institute (KNMI), De Bilt, The Netherlands 4 Max Planck Institut f¨ur Chemie (MPI

Paris-Sud XI, Université de

334

Physics Issues in the Design of Low Aspect-Ratio, High-, Quasi-Axisymmetric Stellarators  

E-Print Network [OSTI]

, Lausanne, Switzerland 5 Max Planck Institute for Plasma Physics,Greifswald, Germany 6 Kurchatov InstitutePhysics Issues in the Design of Low Aspect-Ratio, High-, Quasi-Axisymmetric Stellarators M Princeton Plasma Physics Laboratory, Princeton, NJ 08543 USA 2 Oak Ridge National Laboratory, Oak Ridge, TN

Lin, Zhihong

335

Integrability and disorder in mesoscopic systems: Application to orbital magnetism  

E-Print Network [OSTI]

komplexer Systeme, 01187 Dresden, Germany Denis Ullmoa) Bell Laboratories, Lucent Technologies, 1D-265, 600 Institut fu¨r Physik, Memminger Strasse. 6, 86135 Augsburg, Germany and Max-Planck-Institut fu¨r Physik functions. We dem- onstrate that the anomalously large zero-field susceptibility characteristic of clean

Ullmo, Denis

336

Atmos. Chem. Phys., 10, 93199331, 2010 www.atmos-chem-phys.net/10/9319/2010/  

E-Print Network [OSTI]

Biogeochemistry Department, Max Planck Institute for Chemistry, Mainz, Germany *present address: Institute of Sciences of Ukraine, Kharkov, Ukraine ***present address: Cordis Corporation, Analytical Technology, Spring burning), a transition period, and the onset of the wet season (clean conditions). In the present study

Meskhidze, Nicholas

337

Modeling Max-Min Fairness for Elastic Flows in Telecommunication Alain Dupuisa, Fabrice Guillemina and Philippe Robertb  

E-Print Network [OSTI]

r0 allocated to some other data ow r0 such that r0 r. Max-min fairness can be formulated in terms1 Modeling Max-Min Fairness for Elastic Flows in Telecommunication Networks Alain Dupuisa, Fabrice Guillemina and Philippe Robertb aFrance Telecom R&D, 2, Avenue Pierre Marzin, 22300 Lannion France b

Guillemin, Fabrice

338

Understanding the Link Between Bicyclists and Light Rail Survey Results from Bicycle Riders on MAX in Portland, Oregon  

E-Print Network [OSTI]

Understanding the Link Between Bicyclists and Light Rail Survey Results from Bicycle Riders on MAX Introduction 1 Portland Bicycle Master Plan, Section V 2 History of Bicycles on MAX 3 Benefits of the Bicycle is a bicycle friendly city. In 1995 and 1998, Bicycling Magazine named Portland the best city for bicycling

Bertini, Robert L.

339

Institute for Materials Science  

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

Institute for Material Science Who we are and what we do 2:23 Institute for Materials Science: Alexander V. Balatsky IMS is an interdisciplinary research and educational center...

340

Petroleum Institute Scholarly Publications  

E-Print Network [OSTI]

Abu Dhabi The Petroleum Institute Scholarly Publications 2008 #12.. AAkkgguunn Petroleum Engineering SS.. MMoorraadd Petroleum Geosciences RR.. NNuunnnn &&SS indicate Petroleum Institute faculty who are attached to the program shown. Every effort has been made

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

Prediction of Protein Subcellular Multi-locations with a Min-Max Modular  

E-Print Network [OSTI]

-location problem. In addition, there are a large portion of proteins lack the information like GO and FunPrediction of Protein Subcellular Multi-locations with a Min-Max Modular Support Vector Machine subcellular multi-locations of proteins with machine learning techniques is a challenging problem

Lu, Bao-Liang

342

Contribution aux CISG de Frdric Mougeot Centre Max Weber UMR 5283 frederic.mougeot@gmail.com  

E-Print Network [OSTI]

travail infirmier en psychiatrie. Rsum de l'article L'introduction des outils de gestion l1 Contribution aux CISG de Frdric Mougeot Centre Max Weber UMR 5283 frederic.mougeot@gmail.com * quoi tient la mesure ? Engagement dans le travail et oprations de codifications. Le cas du

Paris-Sud XI, Universit de

343

CONDENSATION OF HOMOMORPHISM SPACES KLAUS LUX, MAX NEUNHOFFER, AND FELIX NOESKE  

E-Print Network [OSTI]

CONDENSATION OF HOMOMORPHISM SPACES KLAUS LUX, MAX NEUNH¨OFFER, AND FELIX NOESKE Abstract. We present an efficient algorithm for the condensation of homo- morphism spaces. This provides an improvement is a special case of what has become known as "condensation". The precise connection is as follows: Let F

St Andrews, University of

344

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

E-Print Network [OSTI]

of multiple energy harvesting sources including solar, wind, thermal, and vibration, each with a different as the operating lifetime. Unfortunately, Fig. 1. Photo of AmbiMax Hardware with a Solar Panel, Wind Generator power efficiently. As a result, they must use a much larger solar panel than necessary to yield the same

Chou, Pai H.

345

DARK MATTER AND DARK ENERGY AS EFFECTS OF QUANTUM GRAVITY Max I. Fomitchev1  

E-Print Network [OSTI]

DARK MATTER AND DARK ENERGY AS EFFECTS OF QUANTUM GRAVITY Max I. Fomitchev1 Submitted March 12th of high matter density expected in the early Universe I show that primordial inflation and dark energy (i , 2004 ABSTRACT I present a theory of quantum gravity based on the principle of gravitational energy

Giles, C. Lee

346

High Speed Max-Log-MAP Turbo SISO Decoder Implementation Using Branch Metric Normalization  

E-Print Network [OSTI]

High Speed Max-Log-MAP Turbo SISO Decoder Implementation Using Branch Metric Normalization J. H.Erdogan@ee.ed.ac.uk, Tughrul.Arslan@ee.ed.ac.uk Abstract The authors present a turbo soft-in soft-out (SISO) decoder based. The turbo decoder with the proposed technique has been synthesized to evaluate its power consumption

Arslan, Tughrul

347

Virtual Test Tubes: A New Methodology for Computing Max Garzon, Evan Drumwright  

E-Print Network [OSTI]

with conventional solid-state based computers. Here, we explore an alter- native approach to exploiting and complexity, comparing it with the standard symbolic-based solid-state approach. It is becoming increasinglyVirtual Test Tubes: A New Methodology for Computing Max Garzon, Evan Drumwright Computer Science

Deaton, Russell J.

348

Bayesian Learning via Stochastic Gradient Langevin Dynamics Max Welling welling@ics.uci.edu  

E-Print Network [OSTI]

Bayesian Learning via Stochastic Gradient Langevin Dynamics Max Welling welling@ics.uci.edu D. Bren on iterative learning from small mini-batches. By adding the right amount of noise to a standard stochastic" and collects sam- ples after it has been surpassed. We apply the method to three models: a mixture of Gaussians

Kaski, Samuel

349

Defining Development Standards for Reusable User Interface Max Mulawa, Rich Picking and Vic Grout  

E-Print Network [OSTI]

for standard aware development. · Constraints on API of the component. · Documentation structure. · IntegrationDefining Development Standards for Reusable User Interface Components Max Mulawa, Rich Picking.NET user-interface components. This standard aims to assess the quality of implemented components

Grout, Vic

350

Queue-Length Proportional and Max-Min Fair Bandwidth Allocation for Best Effort Flows  

E-Print Network [OSTI]

and fairness principles. In this paper, we propose sequential and parallel algorithms to allocate bandwidth the max-min fairness principle, which maximizes bandwidth utilization and maintains fairness among flows. We first formulate the problem based on the allocation criterion and fairness principle. Then, we

Pan, Deng

351

Social science in forestry Paul Tabbush, Liz O'Brien, Max Hislop and Suzanne Martin  

E-Print Network [OSTI]

Social science in forestry Paul Tabbush, Liz O'Brien, Max Hislop and Suzanne Martin The Social on the idea that sustainable forestry, derived from the 1993 Helsinki Conference, is the result of economic development that is positive in its implications for the environment and for society (Forestry Commission

352

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

353

Copper: An Essential Micronutrient for Beef Cattle Max Irsik DVM, MAB  

E-Print Network [OSTI]

Copper: An Essential Micronutrient for Beef Cattle Max Irsik DVM, MAB Beef Cattle Extension Veterinarian University of Florid College of Veterinary Medicine Throughout the world copper deficiency limits of phosphorous, copper deficiency is the most sever mineral limitation to grazing livestock throughout extensive

Watson, Craig A.

354

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

355

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

E-Print Network [OSTI]

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

Lu, Bao-Liang

356

An Object-Oriented Method for ASCET Max Fuchs and Dieter Nazareth  

E-Print Network [OSTI]

98MF19 BMW-ROOM An Object-Oriented Method for ASCET Max Fuchs and Dieter Nazareth BMW AG, 80788 Munich Maximilian.Fuchs,Dieter.Nazareth@bmw.de Dirk Daniel and Bernhard Rumpe Department of Computer kitchen without a cooking book. Plans to employ the tool for BMW vehicle software sparked off demand

357

Extremal shot noises, heavy tails and max-stable random fields.  

E-Print Network [OSTI]

Extremal shot noises, heavy tails and max-stable random fields. Cl´ement Dombry May 31, 2010 Abstract We consider the extremal shot noise defined by M(y) = sup{mh(y - x); (x, m) }, where. Extremal shot noises naturally appear in extreme value theory as a model for spatial extremes and serve

Paris-Sud XI, Université de

358

OIL & GAS INSTITUTE Introduction  

E-Print Network [OSTI]

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

Mottram, Nigel

359

The Institute of Petroleum  

E-Print Network [OSTI]

The Institute of Petroleum Engineering The Institute of Petroleum Engineering (IPE) is a world leading, specialised centre in research, training and teaching, with the largest petroleum engineering and teaching. Our vision is to be the international institute of choice for research and teaching in petroleum

Painter, Kevin

360

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

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

INSTITUTE OF BIOMEDICAL ENGINEERING  

E-Print Network [OSTI]

INSTITUTE OF BIOMEDICAL ENGINEERING Innovation,Translation, Impact University College London Gower Street London WC1E 6BT UK www.ibme.ucl.ac.uk DesignbyHype!hype.co.uk UCL Institute of Biomedical Engineering #12;Innovating MedTech The Institute of Biomedical Engineering (IBME) provides a much-needed focus

Saunders, Mark

362

Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters  

E-Print Network [OSTI]

The Planck satellite is right now measuring with unprecedented accuracy the primary Background CMB anisotropies. The Standard Model of the Universe (including inflation) provides the context to analyze the CMB and other data. The Planck performance for r, the tensor to scalar ratio related to primordial B mode polarization, will depend on the quality of the data analysis. The Ginsburg Landau approach to inflation allows to take high benefit of the CMB data. The fourth degree double well inflaton potential gives an excellent fit to the current CMB+LSS data. We evaluate the Planck precision to the recovery of cosmological parameters within a reasonable toy model for residuals of systematic effects of instrumental and astrophysical origin based on publicly available information.We use and test two relevant models: the LambdaCDMr model, i.e. the standard LambdaCDM model augmented by r, and the LambdaCDMrT model, where the scalar spectral index, n_s, and r are related through the theoretical `banana-shaped' curve r = r(n_s) coming from the double-well inflaton potential. In the latter case, r = r(n_s) is imposed as a hard constraint in the MCMC data analysis. We take into account the white noise sensitivity of Planck in the 70, 100 and 143 GHz channels as well as the residuals from systematics errors and foregrounds. Foreground residuals turn to affect only the cosmological parameters sensitive to the B modes. The best value for r in the presence of residuals turns to be about r simeq 0.04 for both the LambdaCDMr and the LambdaCDMrT models. We compute the B mode detection probability by the most sensitive HFI-143 channel. At the level of foreground residual equal to 30% of our toy model only a 68% CL detection of r is very likely. For a 95% CL detection the level of foreground residual should be reduced to 10% or lower of the adopted toy model (ABRIDGED).

C. Burigana; C. Destri; H. J. de Vega; A. Gruppuso; N. Mandolesi; P. Natoli; N. G. Sanchez

2010-09-19T23:59:59.000Z

363

The Geometric Calibration of the Planck satellite using Solar System Objects  

E-Print Network [OSTI]

The geometric calibration of the Planck satellite using the planetary transits is investigated, together with the reconstruction of any offsets from the nominal layout of the focal plane. The methods presented here may be applied to a single focal plane transit of a planet, to find the values of the geometric-calibration parameters at the epoch of the transit or all the transits over the course of the mission. The pointing requirements are easily met, with the pointing reconstruction being dominated by the errors due to the star tracker.

D. L. Harrison; F. van Leeuwen

2005-10-19T23:59:59.000Z

364

Institutional Change for Sustainability | Department of Energy  

Broader source: Energy.gov (indexed) [DOE]

Institutional Change for Sustainability Institutional Change for Sustainability Institutional Change Continuous Improvement Cycle Institutional Change Continuous Improvement Cycle...

365

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

E-Print Network [OSTI]

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.

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

2014-10-17T23:59:59.000Z

366

Planck 2015 results. IV. Low Frequency Instrument beams and window functions  

E-Print Network [OSTI]

This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. The in-flight assessment of the LFI main beams relies on measurements performed during observations of Jupiter. By stacking data from seven Jupiter transits, the main beam profiles are measured down to -25 dB at 30 and 44 GHz, and down to -30 dB at 70 GHz. The agreement between the simulated beams and the measured beams is confirmed to be better than 1% at each LFI frequency band (within the 20 dB contour from the peak, the rms values are: 0.1% at 30 and 70 GHz; 0.2% at 44 GHz). Simulated polarized beams are used for the computation of the effective beam window functions. The error budget for the window functions is estimated fro...

Ade, P A R; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; 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; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, 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-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versill, 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; Keihnen, E; Keskitalo, R; Kiiveri, K; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lhteenmki, 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-Vrnle, M; Lindholm, V; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; 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; Nrgaard-Nielsen, H U; Novikov, D; Novikov, I; Paci, F; Pagano, L; Paoletti, D; Partridge, B; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Pierpaoli, E; Pietrobon, D; Pointecouteau, E; Polenta, G; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rebolo, R; Reinecke, M; Remazeilles, M; Renzi, A; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubio-Martn, 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; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; 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; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

367

Deposit Description (for FIS, max 30 characters) Outd $ PSU ID/Acct #, Name(Last, First, MI), or other comments Cards $  

E-Print Network [OSTI]

Cash $ Deposit Description (for FIS, max 30 characters) Outd $ Checks $ PSU ID/Acct #, Name documentation attached. Must equal 0: PSU Miscellaneous Deposit Form Cash $ Deposit Description (for FIS, max 30 Deposit Form Cash $ Deposit Description (for FIS, max 30 characters) Outd $ Checks $ PSU ID/Acct #, Name

Caughman, John

368

156 IEEE JOURNAL ON SELECTED AREAS IN COMMUNICATIONS, VOL. 27, NO. 2, FEBRUARY 2009 Scheduling in IEEE 802.16e Mobile WiMAX  

E-Print Network [OSTI]

in IEEE 802.16e Mobile WiMAX Networks: Key Issues and a Survey Chakchai So-In, Student Member, IEEE, Raj times. IEEE 802.16e based WiMAX networks promise the best available quality of experience for mobile data service users. Unlike wireless LANs, WiMAX networks incorporate several quality of service (Qo

Jain, Raj

369

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

E-Print Network [OSTI]

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.

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

2015-01-01T23:59:59.000Z

370

INSTITUTE OF COMPUTER SCIENCE  

E-Print Network [OSTI]

Institute of Computer Science, Academy of Sciences of the Czech Republic. Pod vodrenskou v 2, 182 07 Prague 8, Czech Republic. phone: (+420)266052083...

371

INSTITUTE OF COMPUTER SCIENCE  

E-Print Network [OSTI]

Institute of Computer Science, Academy of Sciences of the Czech Republic. Pod vodrenskou v 2, 182 07 Prague 8, Czech Republic. phone: (+4202) 6884244...

372

INSTITUTE COLLOQUIA AND SEMINARS  

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

National Laboratory, Berkeley, California Production of Transactinide Elements in Cold Fusion Reactions at LBNL February 20 Mr. Thomas Henry, Cyclotron Institute, Texas A&M...

373

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...

374

Edison Electric Institute Update  

Broader source: Energy.gov [DOE]

Presentationgiven at the Fall 2011 Federal Utility Partnership Working Group (FUPWG) meetingdiscusses the Edison Electric Institute (EEI) and the current electricity landscape.

375

Michigan Institute Science and  

E-Print Network [OSTI]

Michigan Institute for Plasma Science and Engineering Seminar Onset of Fast Magnetic Reconnection's magnetosphere, and solar flares. These observations place strong constraints on theory, which must explain

Shyy, Wei

376

Michigan Institute Plasma Science  

E-Print Network [OSTI]

Michigan Institute Plasma Science and Engineering Seminar Neutral Atom Imaging of the Terrestrial re- search includes ion heating in the solar corona, electric double layers, magne- tosphere neutral

Shyy, Wei

377

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 Office of InspectorConcentrating SolarElectric Coop,SaveWhiskey Flatshydro Home Waterstructuredtext in "Max

378

Property:OpenEI/UtilityRate/EnergyRateStructure/Tier4Max | 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 CenterFranconia, Virginia: Energy ResourcesLoadingPenobscotInformation Max Jump to: navigation, search This is a property of type

379

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 CenterFranconia, Virginia: Energy ResourcesLoadingPenobscotInformation Max Jump to: navigation, search This is a

380

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 CenterFranconia, Virginia: Energy ResourcesLoadingPenobscotInformation Max Jump to: navigation, search This is

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

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

E-Print Network [OSTI]

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.

Bikash R Dinda; Sumit Kumar; Anjan A. Sen

2014-10-21T23:59:59.000Z

382

The effect of a spatially varying Galactic spectral index on the maximum entropy reconstruction of Planck Surveyor satellite data  

E-Print Network [OSTI]

We study the effect of Galactic foregrounds with spatially varying spectral indices on analysis of simulated data from the Planck Satellite. We also briefly mention the effect the extra-galactic point sources have on the data analysis and summarise the most recent constraints on Galactic emission at GHz frequencies.

A. W. Jones; M. P. Hobson; P. Mukherjee; A. N. Lasenby

1998-10-15T23:59:59.000Z

383

Ford-Pfenning Quantum Inequalities(QI) in the Natario Warp Drive Spacetime using the Planck Length Scale.  

E-Print Network [OSTI]

Ford-Pfenning Quantum Inequalities(QI) in the Natario Warp Drive Spacetime using the Planck Length Warp Drives are solutions of the Einstein Field Equations that allows superluminal travel within drive discovered in 1994 and the Natario warp drive discovered in 2001. However as stated by both

Paris-Sud XI, Université de

384

Piezoelectric Micro/Nano-Pillars for Energy Harvesting & Medical Ultrasound Applications Max Lifson, Dartmouth College, SURF 2010 Fellow  

E-Print Network [OSTI]

Piezoelectric Micro/Nano-Pillars for Energy Harvesting & Medical Ultrasound Applications Max Lifson these pillars are actually hollow nanotubes, the purpose of this study is to verify a process that can be used

Li, Mo

385

Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data  

E-Print Network [OSTI]

We present a data analysis pipeline for CMB polarization experiments, running from multi-frequency maps to the power spectra. We focus mainly on component separation and, for the first time, we work out the covariance matrix accounting for errors associated to the separation itself. This allows us to propagate such errors and evaluate their contributions to the uncertainties on the final products.The pipeline is optimized for intermediate and small scales, but could be easily extended to lower multipoles. We exploit realistic simulations of the sky, tailored for the Planck mission. The component separation is achieved by exploiting the Correlated Component Analysis in the harmonic domain, that we demonstrate to be superior to the real-space application (Bonaldi et al. 2006). We present two techniques to estimate the uncertainties on the spectral parameters of the separated components. The component separation errors are then propagated by means of Monte Carlo simulations to obtain the corresponding contributi...

Ricciardi, S; Natoli, P; Polenta, G; Baccigalupi, C; Salerno, E; Kayabol, K; Bedini, L; De Zotti, G; 10.1111/j.1365-2966.2010.16819.x

2010-01-01T23:59:59.000Z

386

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

SciTech Connect (OSTI)

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.

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

2007-04-18T23:59:59.000Z

387

No-Scale F-SU(5) in the Light of LHC, Planck and XENON  

E-Print Network [OSTI]

We take stock of the No-Scale F-SU(5) model's experimental status and prospects in the light of results from LHC, Planck, and XENON100. Given that no conclusive evidence for light Supersymmetry (SUSY) has emerged from the 7, 8 TeV collider searches, the present work is focused on exploring and clarifying the precise nature of the high-mass cutoff enforced on this model at the point where the stau and neutralino mass degeneracy becomes so tight that cold dark matter relic density observations cannot be satisfied. This hard upper boundary on the model's mass scale constitutes a top-down theoretical mandate for a comparatively light (and testable) SUSY spectrum which does not excessively stress natural resolution of the gauge hierarchy problem. The overlap between the resulting model boundaries and the expected sensitivities of the future 14 TeV LHC and XENON 1-Ton direct detection SUSY / dark matter experiments is described.

Tianjun Li; James A. Maxin; Dimitri V. Nanopoulos; Joel W. Walker

2013-09-17T23:59:59.000Z

388

Normalization conventions for Newton's constant and the Planck scale in arbitrary spacetime dimension  

E-Print Network [OSTI]

We calculate, in d spacetime dimensions, the relationship between the coefficient 1/K^2 of the Einstein-Hilbert term in the action of general relativity and the coefficient G_N of the force law that results from the Newtonian limit of general relativity. The result is K^2=2[(d-2)/(d-3)]Vol(S^[d-2])G_N, where Vol(S^n) is the volume of the unit n-sphere. While the d=4 case is an elementary calculation in any general relativity text, the arbitrary case presented here is slightly less well known. We discuss the relevance of this result for the definition of the so-called "reduced Planck mass" and comment very briefly on the implications for brane world models. [abstract abridged

Sean P. Robinson

2006-09-17T23:59:59.000Z

389

Hypersharp Resonant Capture of Neutrinos as a Laboratory Probe of the Planck Length  

E-Print Network [OSTI]

The 18.6 keV antineutrino line from 2-body decay of 3H in crystals can be emitted with natural width because of motional averaging by lattice vibrations despite the very long lifetime of 3H and contrary to commonly held views of linewidths in such a case. It can be resonantly captured in 3He with geometrical cross section sigma ~10-17 cm2. Using its hypersharp sensitivity DELTAE/E ~10-29 and the method of time-filtered resonance, the basic energy width ~10-24 eV expected of the 3H state can be measured to test if ultimate nuclear widths are limited by the Planck length rather than time-energy uncertainty.

R. S. Raghavan

2009-03-04T23:59:59.000Z

390

Simultaneous Planck, Swift, and Fermi observations of X-ray and gamma-ray selected blazars  

E-Print Network [OSTI]

We present simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard X-ray, and gamma-ray bands. Our unique data set has allowed us to demonstrate that the selection method strongly influences the results, producing biases that cannot be ignored. Almost all the BL Lac objects have been detected by Fermi-LAT, whereas ~40% of the flat-spectrum radio quasars (FSRQs) in the radio, soft X-ray, and hard X-ray selected samples are still below the gamma-ray detection limit even after integrating 27 months of Fermi-LAT data. The radio to sub-mm spectral slope of blazars is quite flat up to ~70GHz, above which it steepens to ~-0.65. BL Lacs have significantly flatter spectra than FSRQs at higher frequencies. The distribution of the rest-frame synchrotron peak frequency (\

Giommi, P; Lahteenmaki, A; Thompson, D J; Capalbi, M; Cutini, S; Gasparrini, D; Gonzalez-Nuevo, J; Leon-Tavares, J; Lopez-Caniego, M; Mazziotta, M N; Monte, C; Perri, M; Raino, S; Tosti, G; Tramacere, A; Verrecchia, F; Aller, H D; Aller, M F; Angelakis, E; Bastieri, D; Berdyugin, A; Bonaldi, A; Bonavera, L; Burigana, C; Burrows, D N; Buson, S; Cavazzuti, E; Chincarini, G; Colafrancesco, S; Costamante, L; Cuttaia, F; D'Ammando, F; de Zotti, G; Frailis, M; Fuhrmann, L; Galeotta, S; Gargano, F; Gehrels, N; Giglietto, N; Giordano, F; Giroletti, M; Keihanen, E; King, O; Krichbaum, T P; Lasenby, A; Lavonen, N; Lawrence, C R; Leto, C; Lindfors, E; Mandolesi, N; Massardi, M; Max-Moerbeck, W; Michelson, P F; Mingaliev, M; Natoli, P; Nestoras, I; Nieppola, E; Nilsson, K; Partridge, B; Pavlidou, V; Pearson, T J; Procopio, P; Rachen, J P; Readhead, A; Reeves, R; Reimer, A; Reinthal, R; Ricciardi, S; Richards, J; Riquelme, D; Saarinen, J; Sajina, A; Sandri, M; Savolainen, P; Sievers, A; Sillanpaa, A; Sotnikova, Y; Stevenson, M; Tagliaferri, G; Takalo, L; Tammi, J; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tornikoski, M; Trigilio, C; Turunen, M; Umana, G; Ungerechts, H; Villa, F; Wu, J; Zacchei, A; Zensus, J A; Zhou, X

2011-01-01T23:59:59.000Z

391

Studies of parallel algorithms for the solution of a Fokker-Planck equation  

SciTech Connect (OSTI)

The study of laser-created plasmas often requires the use of a kinetic model rather than a hydrodynamic one. This model change occurs, for example, in the hot spot formation in an ICF experiment or during the relaxation of colliding plasmas. When the gradients scalelengths or the size of a given system are not small compared to the characteristic mean-free-path, we have to deal with non-equilibrium situations, which can be described by the distribution functions of every species in the system. We present here a numerical method in plane or spherical 1-D geometry, for the solution of a Fokker-Planck equation that describes the evolution of stich functions in the phase space. The size and the time scale of kinetic simulations require the use of Massively Parallel Computers (MPP). We have adopted a message-passing strategy using Parallel Virtual Machine (PVM).

Deck, D. [Los Alamos National Lab., NM (United States); Samba, G. [CEA/CEL-V, Villeneuve St. Georges (France). Dept. de Mathematiques Appliquees

1995-11-01T23:59:59.000Z

392

Constraints on the extensions to the base $?$CDM model from BICEP2, Planck and WMAP  

E-Print Network [OSTI]

Recently Background Imaging of Cosmic Extragalactic Polarization (B2) discovered the relic gravitational waves at $7.0\\sigma$ confidence level. However, the other cosmic microwave background (CMB) data, for example Planck data released in 2013 (P13), prefer a much smaller amplitude of the primordial gravitational waves spectrum if a power-law spectrum of adiabatic scalar perturbations is assumed in the six-parameter $\\Lambda$CDM cosmology. In this paper, we explore whether the $w$CDM model and the running spectral index can relax the tension between B2 and other CMB data. In particular, we find that a positive running of running of spectral index is preferred at $1.7\\sigma$ level from the combination of B2, P13 and WMAP Polarization data.

Cheng Cheng; Qing-Guo Huang; Wen Zhao

2014-05-02T23:59:59.000Z

393

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

SciTech Connect (OSTI)

The Planck satellite will observe the full sky at nine frequencies from 30 to 857 GHz. Temperature and polarization frequency maps made from these observations are prime deliverables of the Planck mission. The goal of this paper is to examine the effects of four realistic instrument systematics in the 30 GHz frequency maps: non-axially-symmetric beams, sample integration, sorption cooler noise, and pointing errors. They simulated one year long observations of four 30 GHz detectors. The simulated timestreams contained CMB, foreground component (both galactic and extra-galactic), instrument nolise (correlated and white), and the four instrument systematic effects. They made maps from the timelines and examined the magnitudes of the systematics effects in the maps and their angular power spectra. They also compared the maps of different mapmaking codes to see how they performed. They used five mapmaking codes (two destripers and three optimal codes). None of their mapmaking codes makes an attempt to deconvolve the beam from its output map. Therefore all our maps had similar smoothing due to beams and sample integration. This is a complicated smoothing, because every map pixel has its own effective beam. Temperature to polarization cross-coupling due to beam mismatch causes a detectable bias in the TE spectrum of the CMB map. The effects of cooler noise and pointing errors did not appear to be major concerns for the 30 GHz channel. The only essential difference found so far between mapmaking codes that affects accuracy (in terms of residual RMS) is baseline length. All optimal codes give essentially indistiguishable results. A destriper gives the same result as the optimal codes when the baseline is set short enough (Madam). For longer baselines destripers (Springtide and Madam) require less computing resources but deliver a noisier map.

The Planck CTP Working Group; Ashdown, M.A.J.; Baccigalupi, C.; Bartlett, J.G.; Borrill, J.; Cantalupo, C.; de Gasperis, G.; Gorski, K.M.; Hivon, E.; Huffenberger, K.; Keihanen, E.; Keskitalo, R.; Kisner, T.; Hurki-Suonio, H.; Lawrence, C.R.; Natoli, P.; Poutanen, T.; Prezeau, G.; Reinecke, M.; Rocha, G.; Sandri, M.; Stompor, R..; Villa, F.; Wandelt, B.; de Troia, G.

2008-06-19T23:59:59.000Z

394

Planck-scale phenomenology with anti-de Sitter momentum space  

E-Print Network [OSTI]

We investigate the anti-de Sitter (AdS) counterpart to the well studied de Sitter (dS) model for energy-momentum space, viz "$\\kappa$-momentum space" space (with a structure based on the properties of the $\\kappa$-Poincar\\'e Hopf algebra). On the basis of previous preliminary results one might expect the two models to be "dual": dS exhibiting an invariant maximal spatial momentum but unbounded energy, AdS a maximal energy but unbounded momentum. If that were the case AdS momentum space could be used to implement a principle of maximal Planck-scale energy, just as several studies use dS momentum space to postulate of maximal Planck-scale spatial momentum. However several unexpected features are uncovered in this paper, which limit the scope of the expected duality, and interestingly they take different forms in different coordinatizations of AdS momentum space. "Cosmological" AdS coordinates mimic the dS construction used for $\\kappa$-momentum space, and produce a Carrol limit in the ultraviolet. However, unlike the $\\kappa$-momentum space, the boundary of the covered patch breaks Lorentz invariance, thereby introducing a preferred frame. In "horospherical" coordinates we achieve full consistency with frame independence as far as boost transformations are concerned, but find that rotational symmetry is broken, leading to an anisotropic model for the speed of light. Finally, in "static" coordinates we find a way of deforming relativistic transformations that successfully enforces frame invariance and isotropy, and produces a Carrol limit in the ultraviolet. However, the phenomenological implications appear to be too weak for any realistic chance of detection. Our results are also relevant for a long-standing debate on whether or not coordinate redefinitions in momentum space lead to physically equivalent theories: our three proposals are evidently physically inequivalent (abridged)

Michele Arzano; Giulia Gubitosi; Joao Magueijo; Giovanni Amelino-Camelia

2014-12-05T23:59:59.000Z

395

National Institutes of Health National Institute of Mental Health  

E-Print Network [OSTI]

National Institutes of Health National Institute of Mental Health Department of Health and HumanNational Institute of Mental Health Division of Intramural Research Programs http://intramural.nimh.nih.gov/ [NIMH of Fellowship Training] National Institutes of Health National Institute of Mental Health Department of Health

Baker, Chris I.

396

J A H R E S B E R I C H T | A N N U A L R E P O R T bericht des Prsidenten  

E-Print Network [OSTI]

J A H R E S B E R I C H T | A N N U A L R E P O R T 2 0 0 9 #12;2 bericht des Präsidenten Lese an Umweltveränderungen kOOPeratiOnsPrOgramme Partnergruppen Max Planck Fellows Kooperation mit der Fraunhofer-Gesellschaft Tandemprojekte Institutsübergreifende Forschungsinitiativen nachwuchsFörderung Minerva-Programm Max

Falge, Eva

397

~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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched5 Industrial Carbon CaptureFY08Intermittent3,19963xinyufu Ames17 TheStudy of3511MANUAL

398

Use of Institutional Controls  

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

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.

2003-04-09T23:59:59.000Z

399

Critical Materials Institute  

ScienceCinema (OSTI)

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.

Alex King

2013-06-05T23:59:59.000Z

400

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

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401

INSTITUTE COLLOQUIA AND SEMINARS  

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

April 16 M. Sanchez-Vega and V. E. Jacob, Cyclotron Institute, Texas A&M University Test of the Unitarity of the CKM Matrix via Superallowed + decay. April 23 Dr. Subrata...

402

Institutional Change Process for Sustainability  

Broader source: Energy.gov [DOE]

For establishing institutional change in a Federal agency to achieve sustainability or other energy efficiency goals, follow the five-step institutional change process. In accordance with the...

403

Strategies for Achieving Institutional Change  

Broader source: Energy.gov [DOE]

Many strategiesincluding those derived from Institutional Change Principlesmay be used to effect institutional change in support of energy and sustainability objectives.

404

Quaternary Science Reviews 22 (2003) 659671 Coupling of the hemispheres in observations and simulations of  

E-Print Network [OSTI]

and simulations of glacial climate change A. Schmittnera, *, O.A. Saenkob , A.J. Weaverb a Max-Planck-Institut f of Victoria, P.O. Box 3055, Stn CSC, Victoria, BC, Canada, V8W 3P6 Received 26 June 2002; accepted 9 September 2002 Abstract We combine reconstructions, climate model simulations and a conceptual model of glacial

Schmittner, Andreas

405

The effect of expertise on the quality of forest standards implementation: The case of FSC forest certification in Russia  

E-Print Network [OSTI]

certification in Russia Olga Maletz a, , Maria Tysiachniouk b,1 a Max Planck Institute for the Study, Office 301, St. Petersburg 191040, Russia a b s t r a c ta r t i c l e i n f o Keywords: Expertise in the forestry sector. Specifically we analyze the experience of two large forest companies in Russia

406

Garching 11th May 2010 Annual Network Meeting  

E-Print Network [OSTI]

Garching 11th May 2010 RoPACS Annual Network Meeting Michele Cappetta Max Planck Institut fr extraterrestrische Physik #12;Outline M. Cappetta, RoPACS Annual Network Meeting, Garching 11th May 2010 The project from HRS @ HET R=60000 M. Cappetta, RoPACS Annual Network Meeting, Garching 11th May 2010 #12;HD195019

Pinfield, David J.

407

Ann. Geophys., 25, 171190, 2007 www.ann-geophys.net/25/171/2007/  

E-Print Network [OSTI]

Finnish Meteorological Institute, 11010 Helsinki, Finland 3Centre d'Etude Spatiale des Rayonnements, Systeme Solaire, Toulouse, France 4Max Planck Institue for Solar System Research, Katlenburg as "nose-like" structures, due to their appearance when represented in energy-time spectrograms, character

Paris-Sud XI, Université de

408

Atmos. Chem. Phys., 3, 14611475, 2003 www.atmos-chem-phys.org/acp/3/1461/ Atmospheric  

E-Print Network [OSTI]

Atmos. Chem. Phys., 3, 14611475, 2003 www.atmos-chem-phys.org/acp/3/1461/ Atmospheric Chemistry, L. Lange1, and J. Lelieveld1 1Max Planck Institute for Chemistry, Mainz, Germany 2German Weather (Andreae and Merlet, 2001). Increased use of gasoline and other hydrocarbon products has caused enhanced

Meskhidze, Nicholas

409

Inhomogeneous soliton ratchets under two ac forces Luis Morales-Molina  

E-Print Network [OSTI]

Inhomogeneous soliton ratchets under two ac forces Luis Morales-Molina Max-Planck Institut fr; published 10 April 2006 We extend our previous work on soliton ratchet devices L. Morales-Molina et al., Eur, as proposed for particle ratchets by Savele'v et al. Europhys. Lett. 67, 179 2004 ; Phys. Rev. E 70, 066109

Snchez, Angel "Anxo"

410

A&A manuscript no. (will be inserted by hand later)  

E-Print Network [OSTI]

Max­Planck­Institut f¨ur extraterrestrische Physik, Postfach 1603, D--85740 Garching, Germany 3 ISO for the grating sections are ??=ffi?? ¸ 10000. Any remaining errors in the wavelength scale are dominated is described in Schaeidt et al (1996). Pre­flight the wavelength calibration of the two grat­ ing sections

411

A&A manuscript no. (will be inserted by hand later)  

E-Print Network [OSTI]

source in Orion M.Pohl Max­Planck­Institut f?ur extraterrestrische Physik, Postfach 1603, 85740 Garching and Dermer 1995). In the next section I will show that the observed emission from the Orion region can

Pohl, Martin Karl Wilhelm

412

Influence of tissue conductivity anisotropy on EEG/MEG field and return current computation in a realistic head model  

E-Print Network [OSTI]

brain using potential differences and/or magnetic fluxes measured non- invasively directly from the head in a realistic head model: A simulation and visualization study using high-resolution finite element modeling C 3493, Salt Lake City, UT 84112, USA c Max Planck Institute for Human Cognitive and Brain Sciences

Utah, University of

413

Potential of metabolomics as a functional genomics tool  

E-Print Network [OSTI]

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

Wurtele, Eve Syrkin

414

Comparative Microbial Genomics group CenterforBiologicalSequenceanalysisDepartmentofSystemsBiology,TechnicalUniversityofDenmark  

E-Print Network [OSTI]

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

Ussery, David W.

415

Project funded by the European Union under the 7th Framework Programme  

E-Print Network [OSTI]

Project cost: 4,287,529 Project funding: 3,424,534 Max-Planck-Institut für biologische Kybernetik #12Project funded by the European Union under the 7th Framework Programme http://www.mycopter.eu my a Personal Aerial Transportation System (PATS) #12;http://www.mycopter.eu Rationale for the project Money

416

PHILOSOPHICALMAGAZINEB, 1994, zyxwvutVOL.69, No. 4, 655-669 Plan-view and profile imaging of sulphided platinum particles  

E-Print Network [OSTI]

of sulphided platinum particles By M. A. GRIBELWK~,P. J. F. HARRIS$and J. L. HUTCHISON Department of Materials}faceting of the particles(Harris 1986b).These faceted crystallites provide almost ideal candidates for surface work on specimens of this type (Jefferson and Harris 1988, t Present address: Max-Planck-Institut fur

Harris, Peter J F

417

Detection of cosmic -rays using a heliostat field: the case of F. Arqueros1  

E-Print Network [OSTI]

Fisicas. Universidad Complutense. E-28040 Madrid. Spain 2 CIEMAT-Departamento de Energias renovables. Plataforma Solar de Almeria. E-04080 Almeria. Spain 3 Max-Planck Institute f¨ur Physik. D-80805 M¨unchen. Germany Abstract. Gamma-Ray telescopes based on a solar plant are able to accurately measure the spatial

418

Introduction to special section on the Phoenix Mission: Landing Site Characterization Experiments, Mission Overviews, and  

E-Print Network [OSTI]

braking strategy. After a safe landing, twin fan-like solar panels are unfurled and provide the energy lander with a science payload inherited from MPL and 2001 instruments gives significant advantages, University of Ottawa, Ottawa, Ontario, Canada. 10 Max Planck Institute for Solar System Research, Katlenburg

Duck, Thomas J.

419

erlangen graduate school in advanced optical technologies  

E-Print Network [OSTI]

to the SAOT. The SAOT provides an interdisciplinary research and education programme in which innovation Centre (BLZ) · Fraunhofer Institute for Integrated Systems and Device Technology (IISB) · Max Planck framework for scientific enterprise with important scope for innovation at the inter- faces between

Fiebig, Peter

420

Wolfgang Ketterle Education Pre-diploma (Vordiplom), Physics, University of Heidelberg, Germany, 1978  

E-Print Network [OSTI]

Wolfgang Ketterle Education · Pre-diploma (Vordiplom), Physics, University of Heidelberg, Germany, Germany, 1982. · Ph.D., Physics, Ludwig-Maximilians University of Munich and Max-Planck Institute for Quantum Optics, Garching, Germany, 1986. Employment 1982-88 Research assistant (1982-85) and staff

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

The 32nd International Electric Propulsion Conference, Wiesbaden, Germany September 11 15, 2011  

E-Print Network [OSTI]

The 32nd International Electric Propulsion Conference, Wiesbaden, Germany September 11 ­ 15, 2011 1 Electric Propulsion Conference, Wiesbaden · Germany September 11 ­ 15, 2011 K. Matyash1 , Max-Planck-Institut für Plasmaphysik, EURATOM Association, Greifswald, D-17491, Germany R. Schneider2 , Greifswald

422

ORIGINAL RESEARCH ARTICLE published: 21 June 2012  

E-Print Network [OSTI]

Laugerette3 , Anna Wiencis3 , Xavier Grosmaitre2 and Jean-Pierre Montmayeur1,3 * 1 Chemosensory Perception, Max Planck Institute for Chemical Ecology, Germany Reviewed by: Monika Stengl, Universität Kassel, Chemosensory Perception, Unités Mixtes de Recherche, Centre des Sciences du Goût, 9E Boulevard J. D'Arc, 21000

Paris-Sud XI, Université de

423

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014 The Hawk-I UDS for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK 3 Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA, SA 4 Max-Planck-Institut fur extraterrestrische Physik

Faraon, Andrei

424

Mathematical Biology 3 Jurgen Jost  

E-Print Network [OSTI]

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

Arnold, Anton

425

Plasticity of the human brain " We never use the same brain twice" Arno Villringer and Burkhard Pleger  

E-Print Network [OSTI]

Plasticity of the human brain " We never use the same brain twice" Arno Villringer and Burkhard Pleger Max Planck Institute for Human Brain and Cognitive Sciences, Leipzig Summary With the advent of noninvasive neuroimaging the human brain has become accessible for invivo

426

1International Conference on Resource Efficiency in Interorganizational Networks, Pauliner Church, Gttingen, 2013 International Conference on Resource Efficiency  

E-Print Network [OSTI]

Academy of Sciences · German Primate Center · German Aerospace Center (DLR) Max Planck Institutes · for Biophysical Chemistry · for Dynamics and Self-Organization · for Experimental Medicine · for Solar System resources has increased significantly in recent years ­ mainly towards energy crops Wouldn't it be better

Wardetzky, Max

427

Astronomy & Astrophysics manuscript no. (will be inserted by hand later)  

E-Print Network [OSTI]

using as a reference those of other WC8 stars in the solar neighbourhood as well as those of WR 135 collected at the German-Spanish Astronomical Centre, Calar Alto, operated by the Max-Planck- Institut f to the energy budget and chemical enrichment of their parent galaxy. Through their stellar winds, they enrich

Comerón, Fernando

428

ATHAM manual Draft Version 9.4.02 Christiane Textor H igh Resolution  

E-Print Network [OSTI]

3 has been at German Climate Computing Center, Hamburg, Germany 4 Max-Planck-Institute for Chemistry Overview Purpose of the model Simulation of high energy plumes with high gradients in momentum and Crutzen, 1998). Radiation Absorption and scattering of terrestrial and solar radiation On-line delta

de Gispert, Adrià

429

Solvable Model of Spiral Wave Chimeras Erik A. Martens  

E-Print Network [OSTI]

Solvable Model of Spiral Wave Chimeras Erik A. Martens Max Planck Institute for Dynamics and Self. Here we provide the first analytical description of such a spiral wave chimera, and use perturbation.65.+b Keywords: chimera states, Kuramoto model, nonlocal coupling, spiral waves, reaction

Laing, Carlo R.

430

Proton MR Spectroscopy at 7 Tesla in the Macaque monkey J. Pfeuffer1  

E-Print Network [OSTI]

Proton MR Spectroscopy at 7 Tesla in the Macaque monkey J. Pfeuffer1 , C. Juchem1 , H. Merkle2 , N was demonstrated to provide significant sensitivity and resolution gains at high magnetic field [1,2]. MR imaging. K. Logothetis1 1 Max Planck Institute for biological Cybernetics, Tuebingen, D, Germany, 2 LFMI, NIH

Jegelka, Stefanie

431

Functional MR imaging of the awake monkey in a novel vertical large-bore 7 Tesla setup J. Pfeuffer1  

E-Print Network [OSTI]

Functional MR imaging of the awake monkey in a novel vertical large-bore 7 Tesla setup J. Pfeuffer1 , J. Pauls1 , M. Augath1 , T. Steudel1 , H. Merkle2 , N. K. Logothetis1 1 Max Planck InstituteMRI results in the awake trained monkey (Macaca mulatta) using a novel vertical 7T/60cm MR system are reported

Jegelka, Stefanie

432

Localized 1H MR Spectroscopy in the alert monkey at 7 Tesla J. Pfeuffer1  

E-Print Network [OSTI]

Localized 1H MR Spectroscopy in the alert monkey at 7 Tesla J. Pfeuffer1 , C. Juchem1 , H. Merkle2-voxel 1 H MRS in the alert monkey using a 7 T MR system with a vertical bore. Typically , N. K. Logothetis1 1 Department Physiology of Cognitive Processes, Max Planck Institute

Jegelka, Stefanie

433

Project funded by the European Union under the 7th Framework Programme  

E-Print Network [OSTI]

for vehicle automation and control Social and technological impact of a PATS 27/06/2011 5Heinrich Bülthoff, Max Planck Institute for Biological Cybernetics Automation of aerial vehicles PAVs should behavior of vehicles Automation of aerial vehicles PAVs should be autonomous to a very high degree

434

Atmos. Chem. Phys., 7, 211222, 2007 www.atmos-chem-phys.net/7/211/2007/  

E-Print Network [OSTI]

and the influence of sulfuric acid M. Ehn1, T. Pet¨aj¨a1, H. Aufmhoff2, P. Aalto1, K. H¨ameri1,3, F. Arnold2, A properties of ultrafine aerosol particles in the boreal forest: diurnal variation, solubility 64, 00014 University of Helsinki, Finland 2Max-Planck Institute for Nuclear Physics (MPIK

Boyer, Edmond

435

Biogeosciences, 11, 12151259, 2014 www.biogeosciences.net/11/1215/2014/  

E-Print Network [OSTI]

, B. Wehrli15, and F. Wenzhöfer2,3 1Helmholtz Zentrum Geesthacht Center for Materials and Coastal Research, Max-Planck Str. 1, 21502 Geesthacht, Germany 2Alfred Wegener Institute Helmholtz Center for Polar U1987, Perth, WA 6845, Australia fpresent address: Helmholtz Zentrum Geesthacht Center for Materials

Wehrli, Bernhard

436

Supporting Information: Nanoparticle Tension Probes Patterned at the Nanoscale  

E-Print Network [OSTI]

was obtained from a Nanopure water purification system with a UV sterilization unit and showed a resistivity and Biosystems, Max Planck Institute for Intelligent Systems, Stuttgart, Germany Corresponding Author: k%), cytochalasin D ( 98%) were purchased from Sigma-Aldrich (St. Louis, MO) and used without further purification

Salaita, Khalid

437

fur Mathematik in den Naturwissenschaften  

E-Print Network [OSTI]

in networks by Eckehard Olbrich, Thomas Kahle, Nils Bertschinger, Nihat Ay, and J¨urgen Jost Preprint no.: 81 in networks Eckehard Olbrich · Thomas Kahle · Nils Bertschinger · Nihat Ay · J¨urgen Jost Received: date · Nihat Ay · J¨urgen Jost Max Planck Institute for Mathematics in the Sciences, Leipzig, Germany Nihat Ay

438

The Astrophysical Journal Letters, 709:L88L93, 2010 January 20 doi:10.1088/2041-8205/709/1/L88 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

SOLAR WIND OBSERVED BY THE EUV IMAGING SPECTROMETER ON BOARD HINODE Hui Tian1 , Chuanyi Tu1 , Eckart Beijing, China; tianhui924@gmail.com 2 Max-Planck-Institut f¨ur Sonnensystemforschung, 37191 Katlenburg of the solar wind is one of the most important unresolved problems in space and solar physics. We report here

439

Gorur D, Rasmussen CE. Dirichlet process Gaussian mixture models: Choice of the base distribution. JOURNAL OF COMPUTER SCIENCE AND TECHNOLOGY 25(4): 615626 July 2010/DOI 10.1007/s11390-010-1051-1  

E-Print Network [OSTI]

G¨or¨ur D, Rasmussen CE. Dirichlet process Gaussian mixture models: Choice of the base distribution Rasmussen2,3 1 Gatsby Computational Neuroscience Unit, University College London, London WC1N 3AR, U.K. 2 Department of Engineering, University of Cambridge, Cambridge CB2 1PZ, U.K. 3 Max Planck Institute

Edinburgh, University of

440

Eidgenossische Technische Hochschule  

E-Print Network [OSTI]

and stochastic elliptic PDEs B.N. Khoromskij and C. Schwab Research Report No. 2010-04 February 2010 Seminar f-Structured Galerkin Approximation of parametric and stochastic Elliptic PDEs Boris N. Khoromskij Max-Planck-Institut f Schwab Seminar for Applied Mathematics ETH Z¨urich, Switzerland; schwab@sam.math.ethz.ch February 4, 2010

Lang, Annika

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Physics Basis for High-Beta, Low-Aspect-Ratio Stellarator Experiments G. H. Neilson, A. H. Reiman, M. C. Zarnstorff, A. Brooks, G.-Y. Fu, R. J. Goldston, L.-P. Ku,  

E-Print Network [OSTI]

Physics Basis for High-Beta, Low-Aspect-Ratio Stellarator Experiments G. H. Neilson, A. H. Reiman, C. Nuehrenberg Max-Planck-Institute for Plasma Physics, D-17491 Greifswald, Germany High-beta, low and are insensitive to changes in beta. Coil configurations have been calculated that reconstruct these plasma

442

Prevalence of Small-scale Jets from the Network Structures of the Solar Transition Region and  

E-Print Network [OSTI]

furnace model Funnels from networks Tu et al. 2005 #12;Implication for solar wind origin (II) · Mass lossPrevalence of Small-scale Jets from the Network Structures of the Solar Transition Region-Smithsonian Center for Astrophysics 2Lockheed Martin Solar and Astrophysics Laboratory 3Max Planck Institute

443

Mon. Not. R. Astron. Soc. 000, 116 (2013) Printed 5 September 2013 (MN LATEX style file v2.2) The Bifurcated Age-Metallicity Relation of Milky Way  

E-Print Network [OSTI]

-38205 La Laguna, Tenerif 3Dept. of Physics & Astronomy, University of Victoria, P.O. Box 3055, Victoria, B.C., V8W 3P6, Canada, 4Max-Planck-Institut f¨ur extraterrestrische Accepted 2013 August 14

444

November 01, 2012 CURRICULUM VITAE  

E-Print Network [OSTI]

of Idaho 2008 Kavli Foundation Fellow, National Academy of Sciences - Alexander von Humboldt Stiftung 2008, PLoS Genetics 2012-2015 Scientific Advisory Committee, Max Planck Institute for Chemical Ecology 2011-2012 Vice President, American Society of Naturalists 2010 Scientific Advisory Committee, Uppsala Centre

Hoekstra, Hopi E.

445

February 2013 CURRICULUM VITAE  

E-Print Network [OSTI]

of Idaho 2008 Kavli Foundation Fellow, National Academy of Sciences - Alexander von Humboldt Stiftung 2008S Genetics 2012-2015 Scientific Advisory Committee, Max Planck Institute for Chemical Ecology 2011-2012 Vice President, American Society of Naturalists 2010 Scientific Advisory Committee, Uppsala Centre

Hoekstra, Hopi E.

446

The Landscape of the Traveling Salesman Problem Peter F. Stadler y  

E-Print Network [OSTI]

The Landscape of the Traveling Salesman Problem Peter F. Stadler y Max Planck Institut f The landscapes of Traveling Salesman Problems are investigated by ran­ dom walk techniques. The autocorrelation functions for different metrics on the space of tours are calculated. The landscape turns out to be AR(1

Stadler, Peter F.

447

Nonlinear alternating current responses of dipolar fluids J. P. Huang  

E-Print Network [OSTI]

Nonlinear alternating current responses of dipolar fluids J. P. Huang Max Planck Institute Mechanics Group, Laboratory of Computational Engineering, Helsinki University of Technology, P. O. Box 9203-dependent nonlinear dielectric increment of dipolar fluids in nonpolar fluids is often mea- sured by using

Huang, Ji-Ping

448

MORTEN H. CHRISTIANSEN Department of Psychology  

E-Print Network [OSTI]

Phone: (607) 255-3834 (dept) Fax: (607) 255-8433 Email: christiansen@cornell.edu Departmental web page for Psycholinguistics, Nijmegen, the Netherlands. 2009 6-week visit at the Max Planck Institute for Psycholinguistics, Nijmegen, the Netherlands. 2007 9-week sabbatical visit in the Department of Developmental and Comparative

449

The Astrophysical Journal, 676: L81L84, 2008 March 20 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.  

E-Print Network [OSTI]

in magnetic shear and the requirement to release magnetic energy to power 1 Center for Solar Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314. 3 Max-Planck-Institut fu the flare in a local area close to the flaring magnetic polarity inversion line. Two measures

450

Robustness and flexibility in compact quasiaxial stellarators: Global ideal magnetohydrodynamic stability and energetic particle transport  

E-Print Network [OSTI]

stability and energetic particle transport M. H. Redia) Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543 A. Diallob) University of Montana, Missoula, Montana 59801 W. A Physics Laboratory, Princeton University, Princeton, New Jersey 08543 C. Nuhrenberg Max Planck Institut

451

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein  

E-Print Network [OSTI]

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein: Some new applications and new-4000 Roskilde, Denmark 2 Department of Biological Physics, E¨otv¨os Lor´and University (ELTE), H-1117 Budapest, Hungary 3 Max Planck Institute for the Physics of Complex Systems, N¨othnitzer Strasse 38, D

452

Atmos. Chem. Phys., 9, 47174728, 2009 www.atmos-chem-phys.net/9/4717/2009/  

E-Print Network [OSTI]

- lutant which has a profound impact on the environment. Its origin is mostly anthropogenic (almost 90¨are, Oberpfaffenhofen, 82234 Wessling, Germany 2Max-Planck Institute for Nuclear Physics, (MPIK), Atmospheric Physics. This favors the formation of clouds and impacts the cloud droplet sedimentation life- time. In this way

Meskhidze, Nicholas

453

Surface Science 430 (1999) L515L520 www.elsevier.nl/locate/susc Surface Science Letters  

E-Print Network [OSTI]

of Science and Technology, 790-784 Pohang, South Korea b Fritz-Haber-Institut der Max-Planck-Gesellschaft, Faradayweg 4-6, 14195 Berlin-Dahlem, Germany Received 14 October 1998; accepted for publication 11 January. This substrate was chosen since the clean W(001)* Corresponding author. Fax: +82-562-279-3099. E-mail address

454

High-Capacity Hydrogen Storage in Metal-Free Organic Molecular Crystals  

E-Print Network [OSTI]

Scheffler1 1 Fritz-Haber-Institut der Max-Planck-Gesellschaft, Faradayweg 4-6, 14195 Berlin, Germany 2 Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831-6032, USA #12;Hydrogen is an appealing energy carrier for renewable and clean energy [1]. The inten- sive

455

Interaction between hydrogen molecules and metallofullerenes Mina Yoon,1,2,3,a  

E-Print Network [OSTI]

and Zhenyu Zhang1,3 1 Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA 2 Fritz-Haber-Institut der Max-Planck-Gesellschaft, 14195 Berlin, Germany 3 Department have been made in exploring hydrogen as a potential energy carrier for efficient, clean, and renewable

456

Point Defect Configurations of Supersaturated Au Atoms Inside Si  

E-Print Network [OSTI]

, Dhananjay Kumar,, Sokrates T. Pantelides,,# and Stephen J. Pennycook,# Materials Science and Technology Di, Spain, Max Planck Institute of Microstructure Physics, Weinberg 2, 06120 Halle, Germany, and Department of stable silicides in the Au-Si phase diagram suggests growth of clean Si nanowires might be possible

Pennycook, Steve

457

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

E-Print Network [OSTI]

, 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, refineries, etc.) 0911 0914 0924 121 084 Consumption by mining industry Consumption by biogas plants

Meskhidze, Nicholas

458

Function follows dynamics: state-dependency of directed functional influences  

E-Print Network [OSTI]

Function follows dynamics: state-dependency of directed functional influences Demian Battaglia of computations must Demian Battaglia Max Planck Institute for Dynamics and Selforganization and Bernstein Center@nld.ds.mpg.de. 1 #12;2 Demian Battaglia be performed in a way dependent from external context and internal brain

Battaglia, Demian

459

Synchronous Chaos and Broad Band Gamma Rhythm in a Minimal Multi-Layer Model of Primary Visual Cortex  

E-Print Network [OSTI]

Cortex Demian Battaglia1,2 *, David Hansel3,4 1 Max Planck Institute for Dynamics and Self to develop chaos when coupled by sufficiently strong excitation. Citation: Battaglia D, Hansel D (2011 Copyright: 2011 Battaglia and Hansel. This is an open-access article distributed under the terms

Battaglia, Demian

460

PodBase: Transparent storage management for personal devices  

E-Print Network [OSTI]

PodBase: Transparent storage management for personal devices Ansley Post Petr Kuznetsov PeterBase, a system that automatically manages the data and storage across a household's personal devices and frees Druschel Max Planck Institute for Software Systems Rice University 1. INTRODUCTION Personal electronic

Druschel, Peter

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461

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

SciTech Connect (OSTI)

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.

Desroches, Louis-Benoit; Garbesi, Karina

2011-07-20T23:59:59.000Z

462

AVTA: 2013 Ford C-MAX HEV Testing Results | Department of Energy  

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

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 Delicious Rank EERE:YearRound-Up fromDepartment of Energy 601Department of Energy Toyota Prius PHEVofMalibuMAX

463

AVTA: 2013 Ford C-Max Energi PHEV Testing Results | Department of Energy  

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

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 Delicious Rank EERE:YearRound-Up fromDepartment of Energy 601Department of Energy Toyota PriusMax Energi PHEV

464

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

E-Print Network [OSTI]

Within ten nearby (d 450 pc) Gould Belt molecular clouds we evaluate statistically the relative orientation between the magnetic field 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...

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; Benot, A; Benoit-Lvy, 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; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, T A; Eriksen, H K; Falgarone, E; Ferrire, K; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Guillet, V; Harrison, D L; Helou, G; Henrot-Versill, S; Hernndez-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; Keihnen, 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-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Miville-Deschnes, 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; Rubio-Martn, 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

2015-01-01T23:59:59.000Z

465

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

E-Print Network [OSTI]

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.

Toru Miyazawa

2011-12-26T23:59:59.000Z

466

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

E-Print Network [OSTI]

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.

Toru Miyazawa

2011-12-26T23:59:59.000Z

467

The effects of two levels of water vapor pressure on localized sweat rate in high fit males running at 50% VO? Max  

E-Print Network [OSTI]

, workload and VO& Max by correlative methods. Procedures Twelve male volunteers were selected as subjects from a Physical Education class at Texas A&M University. The criterion for selection -1 . -1 as a subject was a VO Max greater than 57 ml kg min.... Schvartz et al. (70) found subjects with high VO Max values (mean of 60. 1 ml kg min ) to respond better to heat than those with 1 medium and low Y02 Max values (means of 47. 7 and 35. 6 ml ~ kg ' n", . n respectively) with lower heart rates...

Sockler, James Michael

2012-06-07T23:59:59.000Z

468

Using BBN in cosmological parameter extraction from CMB: a forecast for Planck  

E-Print Network [OSTI]

Data from future high-precision Cosmic Microwave Background (CMB) measurements will be sensitive to the primordial Helium abundance $Y_p$. At the same time, this parameter can be predicted from Big Bang Nucleosynthesis (BBN) as a function of the baryon and radiation densities, as well as a neutrino chemical potential. We suggest to use this information to impose a self-consistent BBN prior on $Y_p$ and determine its impact on parameter inference from simulated Planck data. We find that this approach can significantly improve bounds on cosmological parameters compared to an analysis which treats $Y_p$ as a free parameter, if the neutrino chemical potential is taken to vanish. We demonstrate that fixing the Helium fraction to an arbitrary value can seriously bias parameter estimates. Under the assumption of degenerate BBN (i.e., letting the neutrino chemical potential $\\xi$ vary), the BBN prior's constraining power is somewhat weakened, but nevertheless allows us to constrain $\\xi$ with an accuracy that rivals bounds inferred from present data on light element abundances.

Jan Hamann; Julien Lesgourgues; Gianpiero Mangano

2008-03-05T23:59:59.000Z

469

Self-Consistent Fokker-Planck Treatment Of Particle Distributions in Astrophysical Plasmas  

E-Print Network [OSTI]

High-energy, multi-component plasmas in which pair creation and annihilation, lepton-lepton scattering, lepton-proton scattering, and Comptonization all contribute to establishing the particle and photon distributions, are present in a broad range of compact astrophysical objects. Earlier work has included much of the microphysics needed to account for electron-photon and electron-proton interactions, but little has been done to handle the redistribution of the particles as a result of their Coulomb interaction with themselves in an arbitrary case. Our goal here is to use a Fokker-Planck approach in order to develop a fully self-consistent theory for the interaction of arbitrarily distributed particles and radiation to arrive at an accurate representation of the high-energy plasma in these sources. We conduct several tests representative of two dominant segments of parameter space and discuss physical implications of the non-Maxwellian distribution function. Approximate analytical forms for the electron distribution in the case of strongly non-Maxwellian plasmas are given.

Sergei Nayakshin; Fulvio Melia

1997-05-03T23:59:59.000Z

470

Detection of Quasar Feedback from the Thermal Sunyaev-Zel'dovich Effect in Planck  

E-Print Network [OSTI]

Poorly understood feedback processes associated with highly-luminous black hole accretion in quasars may dramatically affect the properties of their host galaxies. We search for the effect of quasar feedback on surrounding gas using Planck maps of the thermal Sunyaev-Zel'dovich effect (tSZ). By stacking tSZ Compton-y maps centered on the locations of 26,686 spectroscopic quasars from the Sloan Digital Sky Survey, we detect a strong but unresolved tSZ Compton-y signal at >5 sigma significance that likely originates from a combination of virialized halo atmosphere gas and quasar feedback effects. We show that the feedback contribution to our detected quasar tSZ signal is likely to dominate over virialized halo gas by isolating the feedback tSZ component for high- and low-redshift quasars. We find that this quasar tSZ signal also scales with black hole mass and bolometric luminosity, all consistent with general expectations of quasar feedback. We estimate the mean angularly-integrated Compton-y of quasars at z~1...

Ruan, John J; Anderson, Scott F

2015-01-01T23:59:59.000Z

471

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

E-Print Network [OSTI]

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.

Haidar Sheikhahmadi; Soheyla Ghorbani; Khaled Saaidi

2015-02-18T23:59:59.000Z

472

Neutrinos help reconcile Planck measurements with both Early and Local Universe  

E-Print Network [OSTI]

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.

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

2014-09-17T23:59:59.000Z

473

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

E-Print Network [OSTI]

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...

Adam, R; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, 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; Dsert, F -X; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, 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-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versill, 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; Keihnen, 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-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, 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; Nrgaard-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; Przeau, 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; Sauv, 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

2015-01-01T23:59:59.000Z

474

INSTITUTE ON ASSETS & SOCIAL POLICY  

E-Print Network [OSTI]

INSTITUTE ON ASSETS & SOCIAL POLICY LIVING LONGER ON LESS IN MASSACHUSETTS: THE NEW ECONOMIC (IN)SECURITY OF SENIORS Tatjana Meschede Laura Sullivan Thomas Shapiro #12;About the Institute on Assets and Social Policy The Institute on Assets and Social Policy (IASP), a research institute at the Heller School for Social Policy

Snider, Barry B.

475

ENERGY INSTITUTE WILLOWCREEK  

E-Print Network [OSTI]

WISCONSIN ENERGY INSTITUTE WILLOWCREEK 1918 MARSH UNIVERSITY BAY LAKE MENDOTA CLASS OF LOT #65 LOT. TEACHER SCIENCES EDUCATIONAL BAYLISS DAVIS GRAINGER CHADBOURNE HALL HALL BARNARD MUSIC HALLLAW HALL NORTH EDUCATION HALL SCIENCE RADIO & ENGR. LABWATER SCIENCE OF LIMNOLOGY HASLER LAB RAMPS PARKING MADISON CITY

Liblit, Ben

476

Michigan Institute Science and  

E-Print Network [OSTI]

. Kaita's present research interests focus on plasma-surface interactions and the use of liquid metalsMichigan Institute for Plasma Science and Engineering Seminar Up Against the Wall: Liquid Lithium for the Chamber Technology Challenge in Fusion Energy Dr. Robert Kaita Princeton Plasma Physics Laboratory 3:00 pm

Shyy, Wei

477

Cancer Research Beckman Institute  

E-Print Network [OSTI]

Cancer Research Beckman Institute FOR ADVANCED SCIENCE AND TECHNOLOGY #12;T The medical and scientific worlds have known for many years that in order to truly understand and treat cancer, the fight has and cancerous tumors have to first be visualized at the smallest scales possible, and then treated in the most

Illinois at Urbana-Champaign, University of

478

Institute for ADVANCED STUDY  

E-Print Network [OSTI]

to the Institute's Trustees, dated June 6, 1930. Newark, New Jersey. It is fiindamental in our purpose, and our energetic objects in the Universe? To answer these questions, astronomers and astrophysicists use paper, Adassadnisetts HYMAN BASS Adrain Professor of Mathematics, Cohimbia University Neiv York, New York RICHARD B

479

Michigan Institute Science and  

E-Print Network [OSTI]

Michigan Institute for Plasma Science and Engineering Seminar Universal Magnetic Structures Prof. Mark Moldwin Dept. of Atmospheric, Oceanic and Space Sciences University of Michigan Thursday, 19 Nov and provide examples on how thinking about discrete structures can add to our understanding of the solar

Shyy, Wei

480

Effect of microstructure anisotropy on the deformation of MAX polycrystals studied by in-situ compression combined with neutron diffraction  

SciTech Connect (OSTI)

In situ compression tests combined with neutron diffraction were performed on Ti{sub 2}AlN MAX polycrystals with lamellar anisotropic microstructure: the diffraction peak evolution (position and profile) with applied stress reveals that lamellar grains parallel to compression axis remain elastic while lamellar grains perpendicular to compression plastify, both families being subjected to strong variations of heterogeneous strains (types II and III). We demonstrate that this behavior originates from the complex response of the very anisotropic lamellar microstructure and explains the observation of reversible hysteretic loops when cycling MAX polycrystals even in the elastic regime.

Guitton, A.; Joulain, A.; Thilly, L., E-mail: ludovic.thilly@univ-poitiers.fr [Institut Pprime, CNRS-University of Poitiers-ENSMA, SP2MI, 86962 Futuroscope (France); Van Petegem, S.; Tromas, C.; Van Swygenhoven, H. [Materials Science and Simulations, NUM/ASQ, CH5232 Villigen PSI (Switzerland)

2014-06-16T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
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481

return 2i + 1 Max-heap property is A[Parent(i)] A[i] for  

E-Print Network [OSTI]

[Parent(i)] A[i] for every node i other than the root. Max-Heapify(A, i) l Left(i) r Right(i) if l heap1 Heapsort Parent(i) return i/2 Left(i) return 2i Right(i) return 2i + 1 Max-heap property is A-size[A] and A[l] > A[i] then largest l else largest i if r heap-size[A] and A[r] > A[largest] then largest r

Bylander, Tom

482

Home About Thomson Reuters Press Room Contact Us ScienceWatch Home  

E-Print Network [OSTI]

: Max Planck Inst Extraterr Phys, Postfach 1603, D-85740 Garching, Germany. Max Planck Inst Extraterr of the interstellar dust, radiation, and magnetic fields, and improved particle and nuclear cross-section data

Moskalenko, Igor V.

483

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

E-Print Network [OSTI]

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

D'Andrea, Fabio

484

String theoretic QCD axions in the light of PLANCK and BICEP2  

E-Print Network [OSTI]

The QCD axion solving the strong CP problem may originate from antisymmetric tensor gauge fields in compactified string theory, with a decay constant around the GUT scale. Such possibility appears to be ruled out now by the detection of tensor modes by BICEP2 and the PLANCK constraints on isocurvature density perturbations. A more interesting and still viable possibility is that the string theoretic QCD axion is charged under an anomalous U(1)_A gauge symmetry. In such case, the axion decay constant can be much lower than the GUT scale if moduli are stabilized near the point of vanishing Fayet-Illiopoulos term, and U(1)_A-charged matter fields get a vacuum value far below the GUT scale due to a tachyonic SUSY breaking scalar mass. We examine the symmetry breaking pattern of such models during the inflationary epoch with the Hubble expansion rate 10^{14} GeV, and identify the range of the QCD axion decay constant, as well as the corresponding relic axion abundance, consistent with known cosmological constraints. In addition to the case that the PQ symmetry is restored during inflation, there are other viable scenarios, including that the PQ symmetry is broken during inflation at high scales around 10^{16}-10^{17} GeV due to a large Hubble-induced tachyonic scalar mass from the U(1)_A D-term, while the present axion scale is in the range 10^{9}-5\\times 10^{13} GeV, where the present value larger than 10^{12} GeV requires a fine-tuning of the axion misalignment angle. We also discuss the implications of our results for the size of SUSY breaking soft masses.

Kiwoon Choi; Kwang Sik Jeong; Min-Seok Seo

2014-07-21T23:59:59.000Z

485

Homogenization of the Poisson-Nernst-Planck Equations for Ion Transport in Charged Porous Media  

E-Print Network [OSTI]

Effective Poisson-Nernst-Planck (PNP) equations are derived for macroscopic ion transport in charged porous media under periodic fluid flow by an asymptotic multi-scale expansion with drift. The microscopic setting is a two-component periodic composite consisting of a dilute electrolyte continuum (described by standard PNP equations) and a continuous dielectric matrix, which is impermeable to the ions and carries a given surface charge. Four new features arise in the upscaled equations: (i) the effective ionic diffusivities and mobilities become tensors, related to the microstructure; (ii) the effective permittivity is also a tensor, depending on the electrolyte/matrix permittivity ratio and the ratio of the Debye screening length to the macroscopic length of the porous medium; (iii) the microscopic fluidic convection is replaced by a diffusion-dispersion correction in the effective diffusion tensor; and (iv) the surface charge per volume appears as a continuous "background charge density", as in classical membrane models. The coefficient tensors in the upscaled PNP equations can be calculated from periodic reference cell problems. For an insulating solid matrix, all gradients are corrected by the same tensor, and the Einstein relation holds at the macroscopic scale, which is not generally the case for a polarizable matrix, unless the permittivity and electric field are suitably defined. In the limit of thin double layers, Poisson's equation is replaced by macroscopic electroneutrality (balancing ionic and surface charges). The general form of the macroscopic PNP equations may also hold for concentrated solution theories, based on the local-density and mean-field approximations. These results have broad applicability to ion transport in porous electrodes, separators, membranes, ion-exchange resins, soils, porous rocks, and biological tissues.

Markus Schmuck; Martin Z. Bazant

2014-07-14T23:59:59.000Z

486

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

E-Print Network [OSTI]

The Planck satellite will observe the full sky at nine frequencies from 30 to 857 GHz. The goal of this paper is to examine the effects of four realistic instrument systematics in the 30 GHz frequency maps: non-axially-symmetric beams, sample integration, sorption cooler noise, and pointing errors. We simulated one year long observations of four 30 GHz detectors. The simulated timestreams contained CMB, foreground components (both galactic and extra-galactic), instrument noise (correlated and white), and the four instrument systematic effects. We made maps from the timelines and examined the magnitudes of the systematics effects in the maps and their angular power spectra. We also compared the maps of different mapmaking codes to see how they performed. We used five mapmaking codes (two destripers and three optimal codes). None of our mapmaking codes makes an attempt to deconvolve the beam from its output map. Therefore all our maps had similar smoothing due to beams and sample integration. Temperature to polarization cross-coupling due to beam mismatch causes a detectable bias in the TE spectrum of the CMB map. The effects of cooler noise and pointing errors did not appear to be major concerns for the 30 GHz channel. The only essential difference found so far between mapmaking codes that affects accuracy (in terms of residual RMS) is baseline length. All optimal codes give essentially indistinguishable results. A destriper gives the same result as the optimal codes when the baseline is set short enough. For longer baselines destripers require less computing resources but deliver a noisier map.

M. A. J. Ashdown; C. Baccigalupi; J. G. Bartlett; J. Borrill; C. Cantalupo; G. de Gasperis; G. de Troia; K. M. Gorski; E. Hivon; K. Huffenberger; E. Keihanen; R. Keskitalo; T. Kisner; H. Kurki-Suonio; C. R. Lawrence; P. Natoli; T. Poutanen; G. Prezeau; M. Reinecke; G. Rocha; M. Sandri; R. Stompor; F. Villa; B. Wandelt

2009-04-09T23:59:59.000Z

487

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

SciTech Connect (OSTI)

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.

Telle, Rainer [Institut fuer Gesteinshuettenkunde (Mineral Engineering), Chair of Ceramics and Refractory Materials, RWTH Aachen, Mauerstrasse 5, D-52056 Aachen (Germany)]. E-mail: telle@ghi.rwth-aachen.de; Momozawa, Ai [Institut fuer Gesteinshuettenkunde (Mineral Engineering), Chair of Ceramics and Refractory Materials, RWTH Aachen, Mauerstrasse 5, D-52056 Aachen (Germany); Music, Denis [Materials Chemistry, RWTH Aachen (Germany); Schneider, Jochen M. [Materials Chemistry, RWTH Aachen (Germany)

2006-09-15T23:59:59.000Z

488

Transportation Institutional Plan  

SciTech Connect (OSTI)

This Institutional Plan is divided into three chapters. Chapter 1 provides background information, discusses the purposes of the Plan and the policy guidance for establishing the transportation system, and describes the projected system and the plans for its integrated development. Chapter 2 discusses the major participants who must interact to build the system. Chapter 3 suggests mechanisms for interaction that will foster wide participation in program planning and implementation and provides a framework for managing and resolving the issues related to development and operation of the transportation system. A list of acronyms and a glossary are included for the reader's convenience. Also included in this Plan are four appendices. Of particular importance is Appendix A, which includes detailed discussion of specific transportation issues. Appendices B, C, and D provide supporting material to assist the reader in understanding the roles of the involved institutions.

Not Available

1986-08-01T23:59:59.000Z

489

Formation of a High Coverage (3 3) NO Phase on Pd(111) at Elevated Pressures: Interplay between Kinetic and Thermodynamic Accessibility  

E-Print Network [OSTI]

Max-Planck-Gesellschaft, Faradayweg 4-6, D-14195 Berlin, Germany, Laboratoire de Chimie, UMR CNRS 5182

Goodman, Wayne

490

Curriculum vitae Bernd Knll  

E-Print Network [OSTI]

Curriculum vitae Bernd Knöll Schulbildung 1985 ­ 1992 Max-Planck-Gymnasium Gro?-Umstadt Zivildienst

Ulm, Universität

491

E-Print Network 3.0 - abfallhaltung von natuerlicher Sample Search...  

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

Universitt Hamburg Summary: Prof. Dr. Hans von Storch GKSS-Forschungszentrum Geesthacht Max-Planck-Strae 21502 Geesthacht Prof. Dr... - - - - - - - - - - - - - - - - - -...

492

Matthias Zahn1,2 , Ralf Weisse1  

E-Print Network [OSTI]

for Coastal Research, MaxPlanckStr.1, 21502 Geesthacht, Germany #12;Outline: · Introduction · Reconstruction

Zahn, Matthias

493

Remote Sens. 2014, 6, 4190-4216; doi:10.3390/rs6054190 remote sensing  

E-Print Network [OSTI]

Brockmann Consult, Max-Planck-Str. 2, 21502 Geesthacht, Germany; E-Mails: tom.block@brockmann-consult.de (T

Myneni, Ranga B.

494

meteorological synthesizing centre -east Convention on Long-Range Transboundary Air Pollution  

E-Print Network [OSTI]

of Hydrophysics Max-Planck-Strasse 1 D-21502 Geesthacht GERMANY tel: 49 41 52871847; fax: 49 41 52871888 e

495

Atmos. Chem. Phys., 11, 47794787, 2011 www.atmos-chem-phys.net/11/4779/2011/  

E-Print Network [OSTI]

, Stellenbosch 7599, South Africa 3GKSS Forschungszentrum Geesthacht GmbH, Max-Planck-Strasse, 21502 Geesthacht

Meskhidze, Nicholas

496

J A H R E S B E R I C H T | A N N U A L R E P O R T Vorwort des Prsidenten  

E-Print Network [OSTI]

2 0 1 0 J A H R E S B E R I C H T | A N N U A L R E P O R T #12;Vorwort des Präsidenten Lese, soziale Interaktion und Solidarität kooPerationsProgramme Partnergruppen Max Planck Center Max Planck Forschungsinitiativen nachwuchsFörderung Minerva-Programm Max-Planck-Forschungsgruppen International Max Planck Research

Falge, Eva

497

Analysis, Modification, and Implementation (AMI) of Scheduling Algorithm for the IEEE 802.116e (Mobile WiMAX)  

E-Print Network [OSTI]

Mobile WiMAX (Worldwide Interoperability for Microwave Access) is being touted as the most promising and potential broadband wireless technology. And the popularity rate has been surging to newer heights as the knowledge-backed service era unfolds steadily. Especially Mobile WiMAX is being projected as a real and strategic boon for developing counties such as India due to its wireless coverage acreage is phenomenally high. Mobile WiMAX has spurred tremendous interest from operators seeking to deploy high-performance yet cost-effective broadband wireless networks. The IEEE 802.16e standard based Mobile WiMAX system will be investigated for the purpose of Quality of Service provisioning. As a technical challenge, radio resource management will be primarily considered and main is the costly spectrum and the increasingly more demanding applications with ever growing number of subscribers. It is necessary to provide Quality of Service (QoS) guaranteed with different characteristics. As a possible solution the sche...

Ravichandiran, C; Vaidhyanathan, V

2010-01-01T23:59:59.000Z

498

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

SciTech Connect (OSTI)

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).

Puttagunta, S.; Shapiro, C.

2012-04-01T23:59:59.000Z

499

Structure of pre-Supervisory Committee Meeting (PRE-SCM) report: Abstract of work to date (250 words max)  

E-Print Network [OSTI]

Appendix B Structure of pre-Supervisory Committee Meeting (PRE-SCM) report: Abstract of work to date (250 words max) An abstract of the work to date, providing general background and explaining how the work fits in the field of your project. This abstract can be very similar to the one submitted

Woodgett, Jim

500

Sustainable Development Research Institute fonds  

E-Print Network [OSTI]

Sustainable Development Research Institute fonds Compiled by Erwin Wodarczak and Melanie Hardbattle Projects series Sous-fonds Description o "Women and Sustainable Development: Canadian Perspectives (UBC Library catalogue) #12;Fonds Description Sustainable Development Research Institute fonds. 1985

Handy, Todd C.