Rainer Held > Guest Researcher - Max-Planck Institute for Solid...
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Rainer Held Guest Researcher - Max-Planck Institute for Solid State Research heldrain@gmail.com Formerly a member of the Schlom Group, he joined the Max-Planck Institute for Solid ...
Paul Blom: Research Director, Max Planck Institute for Polymer Research |
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Center for Energy Efficient Materials Paul Blom: Research Director, Max Planck Institute for Polymer Research Jan 22, 2014 | 2:00 PM - 3:00 PM Paul Blom Research Director, Max Planck Institute for Polymer Research Transport and Recombination in Polymer:fullerene bulk Heterojunction Solar Cells January 22, 2014 | 2:00pm | ESB 2001 Faculty host: Thuc Quyen-Nguyen >>>Video and Slides available after the presentation* Abstract In solar cells, free charge carriers can recombine both via
Princeton, Max Planck Society launch new research center for plasma physics
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| Princeton Plasma Physics Lab Princeton, Max Planck Society launch new research center for plasma physics By John Greenwald March 30, 2012 Tweet Widget Google Plus One Share on Facebook (From left to right) Princeton University Professor of Astrophysical Sciences James Stone, Princeton University President Shirley M. Tilghman, Princeton University Dean for Research A. J. Stewart Smith, Max Planck Society President Peter Gruss, and Consul General of the Federal Republic of Germany in New
Dedicated Max-Planck beamline for the in situ investigation of interfaces and thin films
Stierle, A.; Steinhaeuser, A.; Ruehm, A.; Renner, F.U.; Weigel, R.; Kasper, N.; Dosch, H.
2004-12-01
A dedicated beamline for the Max-Planck-Institut fuer Metallforschung was recently taken into operation at the Angstroemquelle Karlsruhe (ANKA). Here we describe the layout of the beamline optics and the experimental end-station, consisting of a heavy duty multiple circle diffractometer. For both a new design was realized, combining a maximum flexibility in the beam properties [white, pink (focused) monochromatic, energy range 6-20 keV] with a special diffractometer for heavy sample environments up to 500 kg, that can be run in different geometrical modes. In addition the angular-reciprocal space transformations for the diffractometer in use are derived, which allows an operation of the instrument in the convenient six circle mode. As an example, results from surface x-ray diffraction on a Cu{sub 3}Au(111) single crystal are presented.
Deporcel, Lilian
2001-04-02
The XXVI SLAC Summer Institute on Particle Physics was held from August 3 to August 14, 1998. The topic, ''Gravity--from the Hubble Length to the Planck Length,'' brought together 179 physicists from 13 countries. The lectures in this volume cover the seven-day school portion of the Institute, which took us from the largest scales of the cosmos, to the Planck length at which gravity might be unified with the other forces of nature. Lectures by Robert Wagoner, Clifford Will, and Lynn Cominsky explored the embedding of gravity into general relativity and the confrontation of this idea with experiments in the laboratory and astrophysical settings. Avishai Deckel discussed observations and implications of the large-scale structure of the universe, and Tony Tyson presented the gravitational lensing effect and its use in the ongoing search for signatures of the unseen matter of the cosmos. The hunt for the wave nature of gravity was presented by Sam Finn and Peter Saulson, and Joe Polchinski showed us what gravity might look like in the quantum limit at the Planck scale. The lectures were followed by afternoon discussion sessions, where students could further pursue questions and topics with the day's lecturers. The Institute concluded with a three-day topical conference covering recent developments in theory and experiment from around the world of elementary particle physics and cosmology; its proceedings are also presented in this volume.
None
2011-10-06
Planck 2010 From the Planck Scale to the ElectroWeak Scale The conference will be the twelfth one in a series of meetings on physics beyond the Standard Model, organized jointly by several European groups: Bonn, CERN, Ecole Polytechnique, ICTP, Madrid, Oxford, Padua, Pisa, SISSA and Warsaw as part of activities in the framework of the European network UNILHC.Topics to be discussed: Supersymmetry Supergravity & string phenomenology Extra dimensions Electroweak symmetry breaking LHC and Tevatron Physics Collider physics Flavor & neutrinos physics Astroparticle & cosmology Gravity & holography Strongly coupled physics & CFT Registration: registration will be open until May 1st. Registration fees amount to 150 CHF and cover the cost of the coffee breaks and the social dinner. Payment has to be made online. The deadline for registration has been postponed to May 7th. However, after May 3th, we shall not accept any talk request any more. The meeting will be partly supported by ° the Marie Curie Initial Training Network "UNILHC" PITN-GA-2009-23792, ° the ERC Advanced Grant "MassTeV" 226371, ° and the CERN-TH unit.
2010-06-02
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
2011-10-06
Planck 2010 From the Planck Scale to the ElectroWeak Scale The conference will be the twelfth one in a series of meetings on physics beyond the Standard Model, organized jointly by several European groups: Bonn, CERN, Ecole Polytechnique, ICTP, Madrid, Oxford, Padua, Pisa, SISSA and Warsaw as part of activities in the framework of the European network UNILHC.Topics to be discussed: Supersymmetry Supergravity & string phenomenology Extra dimensions Electroweak symmetry breaking LHC and Tevatron Physics Collider physics Flavor & neutrinos physics Astroparticle & cosmology Gravity & holography Strongly coupled physics & CFT Registration: registration will be open until May 1st. Registration fees amount to 150 CHF and cover the cost of the coffee breaks and the social dinner. Payment has to be made online. The deadline for registration has been postponed to May 7th. However, after May 3th, we shall not accept any talk request any more. The meeting will be partly supported by the Marie Curie Initial Training Network "UNILHC" PITN-GA-2009-23792, the ERC Advanced Grant "MassTeV" 226371, and the CERN-TH unit.
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Max Schulze June 9, 2015 Extreme unicycling The unicycle that Los Alamos student intern Max Schulze and his brother had given their dad for Father's Day in 2005 did not get much use until Schulze tried it and got hooked. Today, he is a three-time unicycling world champion, with world wins in New Zealand in 2010, Italy in 2012 and Canada in 2014. "My main competitive unicycling event is 'trials,'" Schulze explains, "which requires riders to navigate technically challenging obstacle
Populations Voss, R.; /Garching, Max Planck Inst., MPE; Ajello...
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study the populations of X-ray sources in the Milky Way in the 15-55 keV band using a deep survey with the BAT instrument aboard the Swift observatory. We present the logN-logS...
Princeton, Max Planck Society launch new research center for...
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General of the Federal Republic of Germany in New York Busso von Alvensleben meet to ... General of the Federal Republic of Germany in New York Busso von Alvensleben meet to ...
The Planck Surveyor mission: astrophysical prospects
De Zotti, Gianfranco; Toffolatti, Luigi Toffolatti, Luigi Partridge, R. Bruce
1999-05-01
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{close_quote}s impact on the study of their properties and, on the other side, to what extent foreground contamination may affect Planck{close_quote}s ability to accurately determine cosmological parameters. Planck{close_quote}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{close_quote}s ability to measure the cosmological signals. Even measurements of polarization of the primordial Cosmic Microwave background fluctuations appear to be feasible. {copyright} {ital 1999 American Institute of Physics.}
Giant Protease TPP II's Structure, Mechanism Uncovered
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of California, Berkeley, and the Max Planck Institute of Biochemistry combined ... J. Peters, and W. Baumeister (Max Planck Institute of Biochemistry); P.J. Walian ...
A collaboration bears fruit as W7-X celebrates first research...
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and Andreas Langenberg, of the Max Planck Institute, in front of the housing for ... and Andreas Langenberg, of the Max Planck Institute, in front of the housing for ...
A collaboration bears fruit as W7-X celebrates first research...
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Gallery: PPPL physicist Novimir Pablant and Andreas Langenberg, of the Max Planck ... (Photo by Photo by Scott MassidaMax Planck Institute ) PPPL physicist Novimir ...
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)
Planck constraints on monodromy inflation
Easther, Richard; Flauger, Raphael E-mail: flauger@ias.edu
2014-02-01
We use data from the nominal Planck mission to constrain modulations in the primordial power spectrum associated with monodromy inflation. The largest improvement in fit relative to the unmodulated model has Δχ{sup 2} ≈ 10 and we find no evidence for a primordial signal, in contrast to a previous analysis of the WMAP9 dataset, for which Δχ{sup 2} ≈ 20. The Planck and WMAP9 results are broadly consistent on angular scales where they are expected to agree as far as best-fit values are concerned. However, even on these scales the significance of the signal is reduced in Planck relative to WMAP, and is consistent with a fit to the ''noise'' associated with cosmic variance. Our results motivate both a detailed comparison between the two experiments and a more careful study of the theoretical predictions of monodromy inflation.
Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site
Summary Max Total Units *If All Splits, No Rack Units **If Only FW, AC Splits 1000 52 28 28 2000 87 59 35 3000 61 33 15 4000 61 33 15 Totals 261 153 93 ***Costs $1,957,500.00 $1,147,500.00 $697,500.00 Notes: added several refrigerants removed bins from analysis removed R-22 from list 1000lb, no Glycol, CO2 or ammonia Seawater R-404A only * includes seawater units ** no seawater units included *** Costs = (total units) X (estimate of $7500 per unit) 1000lb, air cooled split systems, fresh water
Primordial power spectrum from Planck
Hazra, Dhiraj Kumar; Shafieloo, Arman; Souradeep, Tarun E-mail: arman@apctp.org
2014-11-01
Using modified Richardson-Lucy algorithm we reconstruct the primordial power spectrum (PPS) from Planck Cosmic Microwave Background (CMB) temperature anisotropy data. In our analysis we use different combinations of angular power spectra from Planck to reconstruct the shape of the primordial power spectrum and locate possible features. Performing an extensive error analysis we found the dip near ℓ ∼ 750–850 represents the most prominent feature in the data. Feature near ℓ ∼ 1800–2000 is detectable with high confidence only in 217 GHz spectrum and is apparently consequence of a small systematic as described in the revised Planck 2013 papers. Fixing the background cosmological parameters and the foreground nuisance parameters to their best fit baseline values, we report that the best fit power law primordial power spectrum is consistent with the reconstructed form of the PPS at 2σ C.L. of the estimated errors (apart from the local features mentioned above). As a consistency test, we found the reconstructed primordial power spectrum from Planck temperature data can also substantially improve the fit to WMAP-9 angular power spectrum data (with respect to power-law form of the PPS) allowing an overall amplitude shift of ∼ 2.5%. In this context low-ℓ and 100 GHz spectrum from Planck which have proper overlap in the multipole range with WMAP data found to be completely consistent with WMAP-9 (allowing amplitude shift). As another important result of our analysis we do report the evidence of gravitational lensing through the reconstruction analysis. Finally we present two smooth form of the PPS containing only the important features. These smooth forms of PPS can provide significant improvements in fitting the data (with respect to the power law PPS) and can be helpful to give hints for inflationary model building.
Planck Surveyor On Its Way to Orbit
Borrill, Julian
2013-05-29
An Ariane 5 rocket carried the Planck Surveyor and a companion satellite into space May 14, 2009 from the European Space Agency (ESA) base on the northwest coast of South America. Once in orbit beyond the moon, Planck will produce the most accurate measurements ever made of the relic radiation from the big bang, plus the largest set of CMB data ever recorded. Berkeley Labs long and continuing involvement with Planck began when George Smoot of the Physics Division proposed Plancks progenitor to ESA and continues with preparations for ongoing data analysis for the U.S. Planck team at NERSC, led by Julian Borrill, co-leader of the Computational Cosmology Center.
Planck Surveyor On Its Way to Orbit
None
2010-01-08
An Ariane 5 rocket carried the Planck Surveyor and a companion satellite into space May 14, 2009 from the European Space Agency (ESA) base on the northwest coast of South America. Once in orbit beyond the moon, Planck will produce the most accurate measurements ever made of the relic radiation from the big bang, plus the largest set of CMB data ever recorded. Berkeley Labs long and continuing involvement with Planck began when George Smoot of the Physics Division proposed Plancks progenitor to ESA and continues with preparations for ongoing data analysis for the U.S. Planck team at NERSC, led by Julian Borrill, co-leader of the Computational Cosmology Center
Khler potentials for Planck inflation
Roest, Diederik; Scalisi, Marco; Zavala, Ivonne E-mail: m.scalisi@rug.nl
2013-11-01
We assess which Khler potentials in supergravity lead to viable single-field inflationary models that are consistent with Planck. We highlight the role of symmetries, such as shift, Heisenberg and supersymmetry, in these constructions. Also the connections to string theory are pointed out. Finally, we discuss a supergravity model for arbitrary inflationary potentials that is suitable for open string inflation and generalise it to the case of closed string inflation. Our model includes the recently discussed supergravity reformulation of the Starobinsky model of inflation as well as an interesting alternative with comparable predictions.
Higher order Fokker-Planck operators
Pomraning, G.C.
1996-11-01
If the scattering interaction in linear particle transport problems is highly peaked about zero momentum transfer, a common and often useful approximation is the replacement of the integral scattering operator with the differential Fokker-Planck operator. This operator involves a first derivative in energy and second derivatives in angle. In this paper, higher order Fokker-Planck scattering operators are derived, involving higher derivatives in both energy and angle. The applicability of these higher order differential operators to representative scattering kernels is discussed. It is shown that, depending upon the details of the scattering kernel in the integral operator, higher order Fokker-Planck approximations may or may not be valid. Even the classic low-order Fokker-Planck operator fails as an approximation for certain highly peaked scattering kernels. In particular, no Fokker-Planck operator is a valid approximation for scattering involving the widely used Henyey-Greenstein scattering kernel.
Unfolding with Maxed and Gravel.
Energy Science and Technology Software Center (OSTI)
2004-07-12
Version: 00 UMG (Unfolding with MAXED and GRAVEL) is a package of seven programs written for the analysis of data measured with spectrometers that require the use of unfolding techniques. See the developers website for information on training courses http://www.ptb.de/en/org/6/utc2006/intro.htm. The program MAXED applies the maximum entropy principle to the unfolding problem, and the program GRAVEL uses a modified SAND-II algorithm to do the unfolding. There are two versions of each: MXD_FC33 and GRV_FC33 formore » few-channel unfolding (e.g., Bonner sphere spectrometers) and MXD-MC33 and GRV_MC33 for multi-channel unfolding (e.g., NE-213). The program IQU can be used to calculate integral quantities for both MAXED and GRAVEL solution spectra and, in the case of MAXED solutions, it can also be used to calculate the uncertainty in these values as well as the uncertainty in the solution spectrum. The uncertainty calculation is handled in the following way: given a solution spectrum generated by MAXED, the program IQU considers variations in the measured data and in the default spectrum and uses standard methods to do sensitivity analysis and uncertainty propagation. There are two versions: IQU_FC33 for few channel unfolding and IQU_MC33 for multi-channel unfolding. The program UMGPlot can be used to display the results from the unfolding programs MAXED and GRAVEL in graphical form in a quick and easy way.« less
PPPL, Princeton University physicists join German Chancellor...
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the Wendelstein 7-X. (Photo by the Max Planck Institute for Plasma Physics) An image of ... plasma. (Photo courtesy of the Max Planck Institute for Plasma Physics) (Photo by ...
Supercomputer Helps Model 3D Map of Adolescent Universe
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The new study, led by Khee-Gan Lee and his team at the Max Planck Institute for Astronomy ... Read the news release from Max Planck Institute for Astronomy here. About NERSC and ...
Max Ambiental S A | Open Energy Information
Ambiental S A Jump to: navigation, search Name: Max Ambiental S.A. Place: Sao Paulo, Brazil Zip: 01452-938 Sector: Carbon Product: Max Ambiental is a company involved in the...
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MaxWest Environmental Systems Jump to: navigation, search Name: MaxWest Environmental Systems Place: Houston, Texas Zip: 77057 Product: MaxWest Environmental Systems designs,...
Zhang, D.S.; Wei, G.W.; Kouri, D.J.; Hoffman, D.K.
1997-03-01
The distributed approximating functional method is applied to the solution of the Fokker{endash}Planck equations. The present approach is limited to the standard eigenfunction expansion method. Three typical examples, a Lorentz Fokker{endash}Planck equation, a bistable diffusion model and a Henon{endash}Heiles two-dimensional anharmonic resonating system, are considered in the present numerical testing. All results are in excellent agreement with those of established methods in the field. It is found that the distributed approximating functional method yields the accuracy of a spectral method but with a local method{close_quote}s simplicity and flexibility for the eigenvalue problems arising from the Fokker{endash}Planck equations. {copyright} {ital 1997 American Institute of Physics.}
Supersymmetric Fokker-Planck strict isospectrality
Rosu, H.C.
1997-08-01
I report a study of the nonstationary one-dimensional Fokker-Planck solutions by means of the strictly isospectral method of supersymmetric quantum mechanics. The main conclusion is that this technique can lead to a space-dependent (modulational) damping of the spatial part of the nonstationary Fokker-Planck solutions, which I call strictly isospectral damping. At the same time, using an additive decomposition of the nonstationary solutions suggested by the strictly isospectral procedure and by an argument of Englefield [J. Stat. Phys. {bold 52}, 369 (1988)], they can be normalized and thus turned into physical solutions, i.e., Fokker-Planck probability densities. There might be applications to many physical processes during their transient period. {copyright} {ital 1997} {ital The American Physical Society}
Axion hot dark matter bounds after Planck
Archidiacono, Maria; Hannestad, Steen; Mirizzi, Alessandro; Raffelt, Georg; Wong, Yvonne Y.Y. E-mail: sth@phys.au.dk E-mail: raffelt@mpp.mpg.de
2013-10-01
We use cosmological observations in the post-Planck era to derive limits on thermally produced cosmological axions. In the early universe such axions contribute to the radiation density and later to the hot dark matter fraction. We find an upper limit m{sub a} < 0.67 eV at 95% C.L. after marginalising over the unknown neutrino masses, using CMB temperature and polarisation data from Planck and WMAP respectively, the halo matter power spectrum extracted from SDSS-DR7, and the local Hubble expansion rate H{sub 0} released by the Carnegie Hubble Program based on a recalibration of the Hubble Space Telescope Key Project sample. Leaving out the local H{sub 0} measurement relaxes the limit somewhat to 0.86 eV, while Planck+WMAP alone constrain the axion mass to 1.01 eV, the first time an upper limit on m{sub a} has been obtained from CMB data alone. Our axion limit is therefore not very sensitive to the tension between the Planck-inferred H{sub 0} and the locally measured value. This is in contrast with the upper limit on the neutrino mass sum, which we find here to range from ? m{sub ?} < 0.27 eV at 95% C.L. combining all of the aforementioned observations, to 0.84 eV from CMB data alone.
Probing the Planck Scale with Proton Decay
Harnik, Roni; Larson, Daniel T.; Murayama, Hitoshi; Thormeier, Marc
2004-04-28
We advocate the idea that proton decay may probe physics at the Planck scale instead of the GUT scale. This is possible because supersymmetric theories have dimension-5 operators that can induce proton decay at dangerous rates, even with R-parity conservation. These operators are expected to be suppressed by the same physics that explains the fermion masses and mixings. We present a thorough analysis of nucleon partial lifetimes in models with a string-inspired anomalous U(1)_X family symmetry which is responsible for the fermionic mass spectrum as well as forbidding R-parity violating interactions. Protons and neutrons can decay via R-parity conserving non-renormalizable superpotential terms that are suppressed by the Planck scale and powers of the Cabibbo angle. Many of the models naturally lead to nucleon decay near present limits without any reference to grand unification.
Does Planck really rule out monomial inflation?
Enqvist, Kari; Kar?iauskas, Mindaugas E-mail: mindaugas.karciauskas@helsinki.fi
2014-02-01
We consider the modifications of monomial chaotic inflation models due to radiative corrections induced by inflaton couplings to bosons and/or fermions necessary for reheating. To the lowest order, ignoring gravitational corrections and treating the inflaton as a classical background field, they are of the Coleman-Weinberg type and parametrized by the renormalization scale ?. In cosmology, there are not enough measurements to fix ? so that we end up with a family of models, each having a slightly different slope of the potential. We demonstrate by explicit calculation that within the family of chaotic ?{sup 2} models, some may be ruled out by Planck whereas some remain perfectly viable. In contrast, radiative corrections do not seem to help chaotic ?{sup 4} models to meet the Planck constraints.
Max Tech and Beyond Design Competition
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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...
SolarMax Inc | Open Energy Information
Korea (Republic) Zip: 445-912 Sector: Solar Product: Manufacturer and engineer of solar heating systems and boilers. References: SolarMax Inc1 This article is a stub. You...
This is likely due to users not understanding the meaning of "Max kWh"--often I see things like: "300, 700, 1000" (derived from "first 300, next 700, greater than 1000") which...
Adjoint Fokker-Planck equation and runaway electron dynamics...
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This content will become publicly available on January 13, 2017 Title: Adjoint Fokker-Planck equation and runaway electron dynamics Authors: Liu, Chang 1 ; Brennan, Dylan P. 1 ...
Fokker-Planck equation in mirror research
Post, R.F.
1983-08-11
Open confinement systems based on the magnetic mirror principle depend on the maintenance of particle distributions that may deviate substantially from Maxwellian distributions. Mirror research has therefore from the beginning relied on theoretical predictions of non-equilibrium rate processes obtained from solutions to the Fokker-Planck equation. The F-P equation plays three roles: Design of experiments, creation of classical standards against which to compare experiment, and predictions concerning mirror based fusion power systems. Analytical and computational approaches to solving the F-P equation for mirror systems will be reviewed, together with results and examples that apply to specific mirror systems, such as the tandem mirror.
Electroweak matching conditions for top pair production at threshold...
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Authors: Hoang, Andre H. ; Reisser, Christoph J. 1 + Show Author Affiliations Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Munich ...
Renormalization group analysis in nonrelativistic QCD for colored...
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Authors: Hoang, Andre H. ; Ruiz-Femenia, Pedro 1 + Show Author Affiliations Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Munich ...
Heavy pair production currents with general quantum numbers in...
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Authors: Hoang, Andre H. ; Ruiz-Femenia, Pedro 1 + Show Author Affiliations Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Munich ...
Opacity of iron, nickel, and copper plasmas in the x-ray wavelength...
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2 more ; Max-Planck-Institut fuer Quantenoptik, D-85748 Garching 3 ; Institute of Nuclear Fusion, Universidad Politecnica de Madrid, Spain and Laboratoire d'Optique...
The best inflationary models after Planck
Martin, Jrme; Vennin, Vincent; Ringeval, Christophe; Trotta, Roberto E-mail: christophe.ringeval@uclouvain.be E-mail: vennin@iap.fr
2014-03-01
We compute the Bayesian evidence and complexity of 193 slow-roll single-field models of inflation using the Planck 2013 Cosmic Microwave Background data, with the aim of establishing which models are favoured from a Bayesian perspective. Our calculations employ a new numerical pipeline interfacing an inflationary effective likelihood with the slow-roll library ASPIC and the nested sampling algorithm MultiNest. The models considered represent a complete and systematic scan of the entire landscape of inflationary scenarios proposed so far. Our analysis singles out the most probable models (from an Occam's razor point of view) that are compatible with Planck data, while ruling out with very strong evidence 34% of the models considered. We identify 26% of the models that are favoured by the Bayesian evidence, corresponding to 15 different potential shapes. If the Bayesian complexity is included in the analysis, only 9% of the models are preferred, corresponding to only 9 different potential shapes. These shapes are all of the plateau type.
Quantum Gravity corrections and entropy at the Planck time
Basilakos, Spyros; Vagenas, Elias C.; Das, Saurya E-mail: saurya.das@uleth.ca
2010-09-01
We investigate the effects of Quantum Gravity on the Planck era of the universe. In particular, using different versions of the Generalized Uncertainty Principle and under specific conditions we find that the main Planck quantities such as the Planck time, length, mass and energy become larger by a factor of order 10?10{sup 4} compared to those quantities which result from the Heisenberg Uncertainty Principle. However, we prove that the dimensionless entropy enclosed in the cosmological horizon at the Planck time remains unchanged. These results, though preliminary, indicate that we should anticipate modifications in the set-up of cosmology since changes in the Planck era will be inherited even to the late universe through the framework of Quantum Gravity (or Quantum Field Theory) which utilizes the Planck scale as a fundamental one. More importantly, these corrections will not affect the entropic content of the universe at the Planck time which is a crucial element for one of the basic principles of Quantum Gravity named Holographic Principle.
The Atacama Cosmology Telescope: cross correlation with Planck maps
Louis, Thibaut; Calabrese, Erminia; Dunkley, Joanna; Næss, Sigurd; Addison, Graeme E.; Hincks, Adam D.; Hasselfield, Matthew; Hlozek, Renée; Bond, J. Richard; Hajian, Amir; Das, Sudeep; Devlin, Mark J.; Dünner, Rolando; Infante, Leopoldo; Gralla, Megan; Marriage, Tobias A.; Huffenberger, Kevin; Kosowsky, Arthur; Moodley, Kavilan; Niemack, Michael D.; and others
2014-07-01
We present the temperature power spectrum of the Cosmic Microwave Background obtained by cross-correlating maps from the Atacama Cosmology Telescope (ACT) at 148 and 218 GHz with maps from the Planck satellite at 143 and 217 GHz, in two overlapping regions covering 592 square degrees. We find excellent agreement between the two datasets at both frequencies, quantified using the variance of the residuals between the ACT power spectra and the ACT × Planck cross-spectra. We use these cross-correlations to measure the calibration of the ACT data at 148 and 218 GHz relative to Planck, to 0.7% and 2% precision respectively. We find no evidence for anisotropy in the calibration parameter. We compare the Planck 353 GHz power spectrum with the measured amplitudes of dust and cosmic infrared background (CIB) of ACT data at 148 and 218 GHz. We also compare planet and point source measurements from the two experiments.
Fokker-Planck approximation of monoenergetic transport processes
Boergers, C.; Larsen, E.W.
1994-12-31
For transport problems with highly forward-peaked scattering, the transport equation is often approximated by the Fokker-Planck equation or, if large-angle scattering is deemed sufficiently important, by the Boltzmann-Fokker-Planck equation. In this paper, we state a simple, necessary, and sufficient condition for the validity of the simpler Fokker-Planck approximation for monoenergetic particle transport. We also show that for screened Rutherford scattering, the Fokker-Planck approximation is only marginally valid and is inaccurate unless the scattering is extremely forward peaked. (The same is true for more sophisticated models of elastic scattering of charged particles. In this paper, we restrict ourselves to screened Rutherford scattering for simplicity). More details on the results presented here will be given in forthcoming publications.
Signatures of Planck corrections in a spiralling axion inflation model
McDonald, John
2015-05-08
The minimal sub-Planckian axion inflation model accounts for a large scalar-to-tensor ratio via a spiralling trajectory in the field space of a complex field Φ. Here we consider how the predictions of the model are modified by Planck scale-suppressed corrections. In the absence of Planck corrections the model is equivalent to a ϕ{sup 4/3} chaotic inflation model. Planck corrections become important when the dimensionless coupling ξ of |Φ|{sup 2} to the topological charge density of the strongly-coupled gauge sector FF{sup ~} satisfies ξ∼1. For values of |Φ| which allow the Planck corrections to be understood via an expansion in powers of |Φ|{sup 2}/M{sub Pl}{sup 2}, we show that their effect is to produce a significant modification of the tensor-to-scalar ratio from its ϕ{sup 4/3} chaotic inflation value without strongly modifying the spectral index. In addition, to leading order in |Φ|{sup 2}/M{sub Pl}{sup 2}, the Planck modifications of n{sub s} and r satisfy a consistency relation, Δn{sub s}=−Δr/16. Observation of these modifications and their correlation would allow the model to be distinguished from a simple ϕ{sup 4/3} chaotic inflation model and would also provide a signature for the influence of leading-order Planck corrections.
Gauge-flation confronted with Planck
Namba, Ryo; Dimastrogiovanni, Emanuela; Peloso, Marco E-mail: ema@physics.umn.edu
2013-11-01
Gauge-flation is a recently proposed model in which inflation is driven solely by a non-Abelian gauge field thanks to a specific higher order derivative operator. The nature of the operator is such that it does not introduce ghosts. We compute the cosmological scalar and tensor perturbations for this model, improving over an existing computation. We then confront these results with the Planck data. The model is characterized by the quantity ??g{sup 2}Q{sup 2}/H{sup 2} (where g is the gauge coupling constant, Q the vector vev, and H the Hubble rate). For ? < 2, the scalar perturbations show a strong tachyonic instability. In the stable region, the scalar power spectrum n{sub s} is too low at small ?, while the tensor-to-scalar ratio r is too high at large ?. No value of ? leads to acceptable values for n{sub s} and r, and so the model is ruled out by the CMB data. The same behavior with ? was obtained in Chromo-natural inflation, a model in which inflation is driven by a pseudo-scalar coupled to a non-Abelian gauge field. When the pseudo-scalar can be integrated out, one recovers the model of Gauge-flation plus corrections. It was shown that this identification is very accurate at the background level, but differences emerged in the literature concerning the perturbations of the two models. On the contrary, our results show that the analogy between the two models continues to be accurate also at the perturbative level.
Ji-Woong Lee | Center for Gas SeparationsRelevant to Clean Energy...
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Max-Planck Institut fuer Kohlenforschung, Germany BSc and MSc in Chemistry, Sungkyunkwan University, Korea EFRC research: We are currently developing a methodology for a...
Using powerful computers, physicists uncover mechanism that stabilizes...
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The research was supported by the DOE Office of Science. The team, which included scientists from General Atomics and the Max Planck Institute for Plasma Physics, performed ...
COLLOQUIUM: Wendelstein 7-X: Highlights from the First Operational...
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COLLOQUIUM: Wendelstein 7-X: Highlights from the First Operational Phase of the New Optimized Stellarator Dr. Oliver P. Ford Max-Planck Institut fr Plasmaphysik, Greifswald...
Verification of the ideal magnetohydrodynamic response at rational...
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New Jersey 08543, USA Max-Planck-Institut fr Plasmaphysik, Greifswald 17491, Germany Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA Publication Date:...
X-ray and neutron scattering studies of the complex compounds...
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Presented 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, ...
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(Univ. of Michigan); and B.J Kim (Argonne National Laboratory, Univ. of Michigan, and Max Planck Institute for Solid State Research). Research funding: National Science...
Dubilier, Nicole
2014-03-19
Nicole Dubilier of the Max Planck Institute speaks at the 9th Annual Genomics of Energy & Environment Meeting on March 20, 2014 in Walnut Creek, Calif.
Stimulated X-Ray Emission for Spectroscopy | Stanford Synchrotron...
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Room 108A Speaker: Clemens Weninger, Max Planck Institute for the Physics of Complex Systems Program Description The recent advance of x-ray free electron lasers (XFELs)...
Neutron Damage and MAX Phase Ternary Compounds
Barsoum, Michael; Hoffman, Elizabeth; Sindelar, Robert; Garcua-Duaz, Brenda; Kohse, Gordon
2014-06-17
The Demands of Gen IV nuclear power plants for long service life under neutron radiation at high temperature are severe. Advanced materials that would withstand high temperatures (up to 1000+ C) to high doses in a neutron field would be ideal for reactor internal structures and would add to the long service life and reliability of the reactors. The objective of this work is to investigate the response 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.
A generalized Fokker-Planck model applied to beam transport
Prinja, A.K.; Pomraning, G.C.
1998-12-31
In this paper the authors consider a generalized Fokker-Planck (GFP) model for the transport of charged-particle beams, when scattering is not sufficiently forward peaked for the well-known Fokker-Planck (FP) approximation to hold. This approximation is strictly valid in the limit that the total scattering cross section {sigma}{sub s} {r_arrow} {infinity} and the mean cosine of scattering {bar {mu}} {r_arrow} 1. When scattering is not sufficiently forward peaked, higher order Fokker-Planck expansions, restricted to differential cross sections that fall off sufficiently rapidly, can be developed. For instance, the Henyey-Greenstein differential cross section does not possess an FP limit at all, while the screened Rutherford cross section satisfies the FP limit only marginally, and its higher order FP limits do not exist. For cross sections that fall off faster than screened Rutherford, including the exponential phase function, higher order truncations exist.
Statistical measures of Planck scale signal correlations in interferometers
Hogan, Craig J.; Kwon, Ohkyung
2015-06-22
A model-independent statistical framework is presented to interpret data from systems where the mean time derivative of positional cross correlation between world lines, a measure of spreading in a quantum geometrical wave function, is measured with a precision smaller than the Planck time. The framework provides a general way to constrain possible departures from perfect independence of classical world lines, associated with Planck scale bounds on positional information. A parametrized candidate set of possible correlation functions is shown to be consistent with the known causal structure of the classical geometry measured by an apparatus, and the holographic scaling of information suggested by gravity. Frequency-domain power spectra are derived that can be compared with interferometer data. As a result, simple projections of sensitivity for specific experimental set-ups suggests that measurements will directly yield constraints on a universal time derivative of the correlation function, and thereby confirm or rule out a class of Planck scale departures from classical geometry.
SolarMax Technology Inc | Open Energy Information
Technology Inc Jump to: navigation, search Name: SolarMax Technology Inc Place: City of Industry, California Zip: 91745 Product: PV module maker and residential and commercial PV...
Incorporating the min-max mesh optimization method within the...
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Incorporating the min-max mesh optimization method within the Target-Matrix Paradigm. ... Country of Publication: United States Language: English Word Cloud More Like This Full ...
Incorporating the min-max mesh optimization method within the...
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Title: Incorporating the min-max mesh optimization method within the Target-Matrix ... Country of Publication: United States Language: English Word Cloud More Like This Full ...
AVTA: 2013 Ford C-MAX HEV Testing Results
Office of Energy Efficiency and Renewable Energy (EERE)
VTO's National Laboratories have tested and collected both dynamometer and fleet data for the Ford C-MAX HEV (a hybrid electric vehicle).
The MAX facility for CFD code validation
Lomperski, S.; Merzari, E.; Obabko, A.; Pointer, W. D.; Fischer, P.
2012-07-01
ANL has recently completed construction of a fluid dynamics test facility devised to provide validation data for CFD simulation tools used to evaluate various aspects of nuclear power plant design and safety. Experiments with the facility involve mixing air jets within a 1x1x1.7m long glass tank at atmospheric pressure. A particle image velocimetry system measures flow velocity and turbulence quantities within the tank while a high-speed infrared camera records temperatures across the tank lid. The tandem of high fidelity thermal and turbulence data is particularly useful for benchmarking transient heat transfer phenomena such as thermal striping. This paper describes the MAX facility, preliminary data obtained during shakedown tests, and the results of companion CFD calculations employing RANS-based Star-CCM+ and large eddy simulations with Nek 5000. (authors)
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Infrastructure :: News :: Related sites National Nanotechnology Initiative Nano Technology Industries Advanced Materials Research Institute Institute of Physics Max-Planck Institute for Kohlenforschung The institute of nanotechnology Nanotechnology Now Nanotechnology - Education Nanojournals Chancellor's Distinguished Lectureship Series
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Related Sites National Nanotechnology Initiative Nano Technology Industries Advanced Materials Research Institute Institute of Physics Max-Planck Institute for Kohlenforschung The institute of nanotechnology Nanotechnology Now Nanotechnology - Education Nanojournals Chancellor's Distinguished Lectureship Series Patent Analytics and Patent Searching
Resurrecting power law inflation in the light of Planck results
Unnikrishnan, Sanil; Sahni, Varun E-mail: varun@iucaa.ernet.in
2013-10-01
It is well known that a canonical scalar field with an exponential potential can drive power law inflation (PLI). However, the tensor-to-scalar ratio in such models turns out to be larger than the stringent limit set by recent Planck results. We propose a new model of power law inflation for which the scalar spectra index, the tensor-to-scalar ratio and the non-gaussianity parameter f{sub N{sub L}{sup equil}} are in excellent agreement with Planck results. Inflation, in this model, is driven by a non-canonical scalar field with an inverse power law potential. The Lagrangian for our model is structurally similar to that of a canonical scalar field and has a power law form for the kinetic term. A simple extension of our model resolves the graceful exit problem which usually afflicts models of power law inflation.
Equilibrium Distribution of Heavy Quarks in Fokker-Planck Dynamics
Walton, D. Brian; Rafelski, Johann
2000-01-03
We obtain an explicit generalization, within Fokker-Planck dynamics, of Einstein's relation between drag, diffusion, and the equilibrium distribution for a spatially homogeneous system, considering both the transverse and longitudinal diffusion for dimension n>1 . We provide a complete characterization of the equilibrium distribution in terms of the drag and diffusion transport coefficients. We apply this analysis to charm quark dynamics in a thermal quark-gluon plasma for the case of collisional equilibration. (c) 1999 The American Physical Society.
University of Maryland Wins Max Tech and Beyond Competition for
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Ultra-Efficient Clothes Dryer | Department of Energy University of Maryland Wins Max Tech and Beyond Competition for Ultra-Efficient Clothes Dryer University of Maryland Wins Max Tech and Beyond Competition for Ultra-Efficient Clothes Dryer September 10, 2013 - 12:00pm Addthis The Energy Department announced today that the University of Maryland won the second annual Max Tech and Beyond design competition for ultra-low energy use appliances and equipment for the second year in a row. The
Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated...
Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated Refrigerant Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated Refrigerant Information flow ...
Zhejiang Max Solar Energy Co Ltd | Open Energy Information
Solar Energy Co Ltd Jump to: navigation, search Name: Zhejiang Max Solar Energy Co Ltd Place: Huzhou, Zhejiang Province, China Zip: 313009 Product: A Zhejiang-based PV module...
Subkilovolt response of Kodak T max XUV film
Dittmore, C.; Stoering, J.P. ); Gullikson, E. )
1990-02-08
A calibration of Kodak T max 100 XUV film at six x-ray energies ranging from 0.27 keV to 1.49 keV has been concluded. The primary purpose was to compare the sensitivity of this film to that of Kodak type 101-07 XUV film in order to appraise the feasibility of replacing the type 101-07 film with the type T max 100 film. In addition to being considerably less expensive, the T max 100 film is less disposed to abrasion from handling. A secondary objective was to provide a base for further response measurements should the T max 100 film prove to be an acceptable substitute for the type 101-07 film. 10 figs., 2 tabs.
NERSC User Group 2013 Big Bang, Big Data, Big Iron Planck Satellite...
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complementarity to astrophysical probes - Perlmutter, Riess & Schmidt (2011) What is Dark Energy? (Planck + DESBigBOSSLSSTEuclid) What is Inflation? (CMBpol + LHC) NERSC User ...
A fractional Fokker-Planck model for anomalous diffusion
Anderson, Johan; Kim, Eun-jin; Moradi, Sara
2014-12-15
In this paper, we present a study of anomalous diffusion using a Fokker-Planck description with fractional velocity derivatives. The distribution functions are found using numerical means for varying degree of fractionality of the stable Lévy distribution. The statistical properties of the distribution functions are assessed by a generalized normalized expectation measure and entropy in terms of Tsallis statistical mechanics. We find that the ratio of the generalized entropy and expectation is increasing with decreasing fractionality towards the well known so-called sub-diffusive domain, indicating a self-organising behavior.
The observational status of Galileon gravity after Planck
Barreira, Alexandre; Li, Baojiu; Baugh, Carlton M.; Pascoli, Silvia E-mail: baojiu.li@durham.ac.uk E-mail: silvia.pascoli@durham.ac.uk
2014-08-01
We use the latest CMB data from Planck, together with BAO measurements, to constrain the full parameter space of Galileon gravity. We constrain separately the three main branches of the theory known as the Cubic, Quartic and Quintic models, and find that all yield a very good fit to these data. Unlike in ?CDM, the Galileon model constraints are compatible with local determinations of the Hubble parameter and predict nonzero neutrino masses at over 5? significance. We also identify that the low l part of the CMB lensing spectrum may be able to distinguish between ?CDM and Galileon models. In the Cubic model, the lensing potential deepens at late times on sub-horizon scales, which is at odds with the current observational suggestion of a positive ISW effect. Compared to ?CDM, the Quartic and Quintic models predict less ISW power in the low l region of the CMB temperature spectrum, and as such are slightly preferred by the Planck data. We illustrate that residual local modifications to gravity in the Quartic and Quintic models may render the Cubic model as the only branch of Galileon gravity that passes Solar System tests.
The interactional foundations of MaxEnt: Open questions
Harr, Michael S.
2014-12-05
One of the simplest and potentially most useful techniques to be developed in the 20{sup th} century, a century noted for an ever more mathematically sophisticated formulation of the sciences, is that of maximising the entropy of a system in order to generate a descriptive, stochastic model of that system in closed form, often abbreviated to MaxEnt. The extension of MaxEnt to systems beyond the physics from which it originated is hampered by the fact that the microscopic physical interactions that are not justified or justifiable within the MaxEnt framework need to be falsifiably evaluated in each new field of application. It is not obvious that such justification exists for many systems in which the interactions are not directly based on physics. For example what is the justification for the use of MaxEnt in biology, climate modelling or economics? Is it simply a useful heuristic or is there some deeper connection with the foundations of some systems? Without further critical examination of the microscopic foundations that give rise to the success of the MaxEnt principle it is difficult to motivate the use of such techniques in other fields except through theoretically an practically unsatisfying analogical arguments. This article briefly presents the basis of MaxEnt principles as originally introduced in statistical mechanics in the Jaynes form, the Tsallis form and the Rnyi form. Several different applications are introduced including that of ecological diversity where maximising the different diversity measures is equivalent to maximising different entropic functionals.
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A lending program begins with a financial institution that procures the funds they lend from a number of other sources.
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Institute Engineering Institute Multidisciplinary engineering research that integrates advanced modeling and simulations, novel sensing systems and new developments in information technology. May 14, 2013 Los Alamos Research Park Los Alamos Research Park, the home of Engineering Institute Contact Institute Director Charles Farrar (505) 665-0860 Email UCSD EI Director Michael Todd (858) 534-5951 Executive Administrator Ellie Vigil (505) 667-2818 Email Administrative Assistant Rebecca Duran (505)
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Institute Seaborg Institute The institute provides a primary mechanism for fostering cooperation and collaboration in actinide science among the national laboratories, university campuses, and the national and international actinide science community. Contact Director Albert Migliori (505) 663-5627 Email Deputy Director Franz Freibert (505) 667-6879 Email Professional Staff Assistant Susan Ramsay (505) 665-0858 Email actinide The Seaborg Institute at Los Alamos integrates research programs,
Generalized Fokker-Planck Approximations of Particle Transport with Highly Forward-Peaked Scattering
Leakeas, Christopher L.; Larsen, Edward W.
2001-03-15
The Fokker-Planck equation is often used to approximate the description of particle transport processes with highly forward-peaked scattering. Pomraning has shown that if the physical scattering kernel is sufficiently dominated by small-angle scattering, then the Fokker-Planck equation is an asymptotic approximation to the linear Boltzmann equation. However, most physically-meaningful scattering kernels contain a sufficient amount of large-angle scattering that the asymptotic criterion is not met. Thus, in many physical problems, solutions of the Fokker-Planck equation are substantially in error. In this paper, Pomraning's asymptotic results are generalized and a new generalized Fokker-Planck (GFP) theory that robustly incorporates large-angle scattering is developed. Numerical experiments demonstrate that the resulting GFP equations are much more accurate than the standard Fokker-Planck equation.
Probing Planck scale physics with IceCube
Anchordoqui, Luis A.; Goldberg, Haim; Gonzalez-Garcia, M.C.; Halzen, Francis; Hooper, Dan; Sarkar, Subir; Weiler, Thomas J.
2005-09-15
Neutrino oscillations can be affected by decoherence induced e.g. by Planck scale suppressed interactions with the space-time foam predicted in some approaches to quantum gravity. We study the prospects for observing such effects at IceCube, using the likely flux of TeV antineutrinos from the Cygnus spiral arm. We formulate the statistical analysis for evaluating the sensitivity to quantum decoherence in the presence of the background from atmospheric neutrinos, as well as from plausible cosmic neutrino sources. We demonstrate that IceCube will improve the sensitivity to decoherence effects of O(E{sup 2}/M{sub Pl}) by 17 orders of magnitude over present limits and, moreover, that it can probe decoherence effects of O(E{sup 3}/M{sub Pl}{sup 2}) which are well beyond the reach of other experiments.
Planck-Size Black Hole Remnants as Dark Matter
Chen, P
2004-09-13
While there exist various candidates, the nature of dark matter remains unresolved. Recently it was argued that the generalized uncertainty principle (GUP) may prevent a black hole from evaporating completely, and as a result there should exist a Planck-size black hole remnant (BHR) at the end of its evaporation. If a sufficient amount of small black holes can be produced in the early universe, then the resultant BHRs can be an interesting candidate for DM. We demonstrate that this is indeed the case for the hybrid inflation model. By assuming BHR as DM, our notion imposes a constraint on the hybrid inflation potential. We show that such a constraint is not so fine-tuned. Possible observational signatures are briefly discussed.
Inflation with a Planck-scale frequency cutoff
Niemeyer, Jens C.
2001-06-15
The implementation of a Planck-scale high frequency and short wavelength cutoff in quantum theories on expanding backgrounds may have potentially nontrivial implications, such as the breaking of local Lorentz invariance and the existence of a yet unknown mechanism for the creation of vacuum modes. In scenarios where inflation begins close to the cutoff scale, these effects could have observable consequences as trans-Planckian modes are redshifted to cosmological scales. In close analogy with similar studies of Hawking radiation, a simple theory of a minimally coupled scalar field in de Sitter space is studied, with a high frequency cutoff imposed by a nonlinear dispersion relation. Under certain conditions the model predicts deviations from the standard inflationary scenario. We also comment on the difficulties in generalizing fluid models of Hawking radiation to cosmological space-times.
Standard big bang nucleosynthesis and primordial CNO abundances after Planck
Coc, Alain [Centre de Sciences Nuclaires et de Sciences de la Matire (CSNSM), CNRS/IN2P3, Universit Paris Sud 11, UMR 8609, Btiment 104, F91405 Orsay Campus (France); Uzan, Jean-Philippe; Vangioni, Elisabeth, E-mail: coc@csnsm.in2p3.fr, E-mail: uzan@iap.fr, E-mail: vangioni@iap.fr [Institut d'Astrophysique de Paris, UMR-7095 du CNRS, Universit Pierre et Marie Curie, 98 bis bd Arago, 75014 Paris (France)
2014-10-01
Primordial or big bang nucleosynthesis (BBN) is one of the three historical strong evidences for the big bang model. The recent results by the Planck satellite mission have slightly changed the estimate of the baryonic density compared to the previous WMAP analysis. This article updates the BBN predictions for the light elements using the cosmological parameters determined by Planck, as well as an improvement of the nuclear network and new spectroscopic observations. There is a slight lowering of the primordial Li/H abundance, however, this lithium value still remains typically 3 times larger than its observed spectroscopic abundance in halo stars of the Galaxy. According to the importance of this ''lithium problem{sup ,} we trace the small changes in its BBN calculated abundance following updates of the baryonic density, neutron lifetime and networks. In addition, for the first time, we provide confidence limits for the production of {sup 6}Li, {sup 9}Be, {sup 11}B and CNO, resulting from our extensive Monte Carlo calculation with our extended network. A specific focus is cast on CNO primordial production. Considering uncertainties on the nuclear rates around the CNO formation, we obtain CNO/H?(5-30)10{sup -15}. We further improve this estimate by analyzing correlations between yields and reaction rates and identified new influential reaction rates. These uncertain rates, if simultaneously varied could lead to a significant increase of CNO production: CNO/H?10{sup -13}. This result is important for the study of population III star formation during the dark ages.
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upon completion of their graduate degrees Over the last seven years, 150 students from 50 academic institutions have participated in the summer school and sixteen such TSM's have...
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Education Opportunities » Engineering Institute Engineering Institute Engineering dynamics that include flight, vibration isolation for precision manufacturing, earthquake engineering, blast loading, signal processing, and experimental model analysis. Contact Leader, Los Alamos Charles Farrar Email Leader, UCSD Michael Todd Email Los Alamos Program Administrator Jutta Kayser (505) 663-5649 Email Administrative Assistant Stacy Baker (505) 663-5233 Email Collaboration for conducting
High temperature ion irradiation effects in MAX phase ceramics
DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)
Clark, D. W.; Zinkle, Steven J.; Patel, Maulik K.; Parish, Chad M.
2015-12-24
The family of layered carbides and nitrides known as MAX phase ceramics combine many attractive properties of both ceramics and metals due to their nanolaminate crystal structure and are promising potential candidates for application in future nuclear reactors. This research examines the effects of energetic heavy ion (5.8 MeV Ni) irradiations on polycrystalline samples of Ti3SiC2, Ti3AlC2, and Ti2AlC. The irradiation conditions consisted of midrange ion doses between 10 and 30 displacements per atom at temperatures of 400 and 700⁰C, conditions relevant to application in future nuclear reactors and a relatively un-explored regime for this new class of materials. Followingmore » irradiation, a comprehensive analysis of radiation response properties was compiled using grazing incidence X-ray diffraction (XRD), nanoindentation, scanning electron microcopy (SEM), and transmission electron microscopy (TEM). In all cases, XRD and TEM analyses confirm the materials remain fully crystalline although the intense atomic collisions induce significant damage and disorder into the layered crystalline lattice. X-ray diffraction and nanoindentation show this damage is manifest in anisotropic swelling and hardening at all conditions and in all materials, with the aluminum based MAX phase exhibiting significantly more damage than their silicon counterpart. In all three materials there is little damage dependence on dose, suggesting saturation of radiation damage at levels below 10 displacements per atom, and significantly less retained damage at higher temperatures, suggesting radiation defect annealing. SEM surface analysis showed significant grain boundary cracking and loss of damage tolerance properties in the aluminum-based MAX phase irradiated at 400⁰C, but not in the silicon counterpart. TEM analysis of select samples suggest that interstitials are highly mobile while vacancies are immobile and that all three materials are in the so-called point defect swelling regime
max walltime for "low" queue is increased to 24 hrs on Hopper
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max walltime for low queue is increased to 24 hrs on Hopper max walltime for low queue is increased to 24 hrs on Hopper May 31, 2012 by Helen He (0 Comments) We have increased the...
WPPI GreenMax-Scheller Residence: Near Zero Energy Monitoring Summary
2010-11-19
This report describes results of GreenMax 2 monitoring project referred to as the GreenMax Net Zero Home, a demonstration home that can provide a wealth of information for the building community.
An implicit energy-conservative 2D Fokker-Planck algorithm -- 1. Difference scheme
Chacon, L.; Barnes, D.C.; Knoll, D.A.; Miley, G.H.
2000-01-20
Numerical energy conservation in Fokker-Planck problems requires the energy moment of the Fokker-Planck equation to cancel exactly. However, standard discretization techniques not only do not observe this requirement (thus precluding exact energy conservation), but they also demand very refined meshes to keep the energy error under control. In this paper, a new difference scheme for multidimensional Fokker-Planck problems that improves the numerical cancellation of the energy moment is proposed. Crucial to this new development is the reformulation of the friction term in the Fokker-Planck collision operator takes the form of a double divergence operating on a tensor, which is suitable for particle and energy conservative differencing. Numerical results show that the new discretization scheme improves the cancellation of the energy moment integral over standard approaches by at least an order of magnitude.
Hogan, Craig
2010-01-08
Classical spacetime and quantum mass-energy form the basis of all of physics. They become inconsistent at the Planck scale, 5.4 times 10^{-44} seconds, which may signify a need for reconciliation in a unified theory. Although proposals for unified theories exist, a direct experimental probe of this scale, 16 orders of magnitude above Tevatron energy, has seemed hopelessly out of reach. However in a particular interpretation of holographic unified theories, derived from black hole evaporation physics, a world assembled out of Planck-scale waves displays effects of unification with a new kind of uncertainty in position at the Planck diffraction scale, the geometric mean of the Planck length and the apparatus size. In this case a new phenomenon may measurable, an indeterminacy of spacetime position that appears as noise in interferometers. The colloquium will discuss the theory of the effect, and our plans to build a holographic interferometer at Fermilab to measure it.
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Software Download and Data Sets First name * Last name * Email address * Institution * Software & Data Set Selection (Select one or more) SHMTools Software (0.20.0 Beta) mFUSE ...
Possible cosmogenic neutrino constraints on Planck-scale Lorentz violation
Mattingly, David M.; Maccione, Luca; Galaverni, Matteo; Liberati, Stefano; Sigl, Günter E-mail: luca.maccione@desy.de E-mail: liberati@sissa.it
2010-02-01
We study, within an effective field theory framework, O(E{sup 2}M{sub Pl}{sup 2}) Planck-scale suppressed Lorentz invariance violation (LV) effects in the neutrino sector, whose size we parameterize by a dimensionless parameter η{sub ν}. We find deviations from predictions of Lorentz invariant physics in the cosmogenic neutrino spectrum. For positive O(1) coefficients no neutrino will survive above 10{sup 19}eV. The existence of this cutoff generates a bump in the neutrino spectrum at energies of 10{sup 17}eV. Although at present no constraint can be cast, as current experiments do not have enough sensitivity to detect ultra-high-energy neutrinos, we show that experiments in construction or being planned have the potential to cast limits as strong as η{sub ν}∼<10{sup −4} on the neutrino LV parameter, depending on how LV is distributed among neutrino mass states. Constraints on η{sub ν} < 0 can in principle be obtained with this strategy, but they require a more detailed modeling of how LV affects the neutrino sector.
The Planck aether model for a unified theory of elementary particles
Winterberg, F. )
1994-06-01
A dense assembly of an equal number of two kinds of Planck masses, one having positive and the other one negative kinetic energy, described by a nonrelativistic nonlinear Heisenberg equation with pointlike interactions, is proposed as a model for a unified theory of elementary particles. The dense assembly of Planck masses leads to a vortex field below the Planck scale having the form of a vortex lattice, which can propagate two types of waves, one having the property of Maxwell's electromagnetic and the other one the property of Einstein's gravitational waves. The waves have a cutoff at a wavelength equal to the vortex lattice constant about [approximately] 10[sup 3] times larger than the Planck length, reproducing the GUT scale of elementary particle physics. The vortex lattice has a resonance energy leading to two kinds of quasiparticles, both of which have the property of Dirac spinors. Depending on the resonance energy, estimated to be [approximately] 10[sup 7] times smaller than the Planck energy, the mass of one of these quasiparticles is about equal to the electron mass. The mass of the other particle is much smaller, making it a likely candidate for the much smaller neutrino mass. Larger spinor masses occur as internal excitations, with a maximum of four such excitations corresponding to a maximum of four particle families. Other vortex solutions may describe the quark-lepton symmetries of the standard model. All masses, with the exception of the Planck mass particles, are quasiparticles for which Lorentz invariance holds, with the Galilei invariance at the Planck scale dynamically broken into Lorentz invariance below this scale. The assumed equal number of Planck masses with positive and negative kinetic energy makes the cosmological constant exactly equal to zero.
Exact solutions of the Fokker-Planck equations with moving boundaries
Lo, C.F. . E-mail: cflo@phy.cuhk.edu.hk
2005-10-01
By means of time-dependent similarity transformations, we derive exact solutions of the Fokker-Planck equations with moving boundaries in the presence of: (1) a time-dependent linear force and (2) a time-dependent nonlinear force. The method of similarity transformation is simple and can be easily applied to more general Fokker-Planck equations. Furthermore, the knowledge of the exact solutions in closed form can be useful as a benchmark to test approximate numerical or analytical procedures.
Mikami, T.
2000-07-01
R. Jordan, D. Kinderlehrer, and F. Otto proposed the discrete-time approximation of the Fokker-Planck equation by the variational formulation. It is determined by the Wasserstein metric, an energy functional, and the Gibbs-Boltzmann entropy functional. In this paper we study the asymptotic behavior of the dynamical systems which describe their approximation of the Fokker-Planck equation and characterize the limit as a solution to a class of variational problems.
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Quantum Institute Quantum Institute A new research frontier awaits! Our door is open and we thrive on mutually beneficial partnerships, collaborations that drive innovations and new technologies. Contact Leader Malcolm Boshier (505) 665-8892 Email Two of LANL's most successful quantum technology initiatives: quantum cryptography and the race for quantum computer The area of quantum information, science, and technology is rapidly evolving, with important applications in the areas of quantum
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McDonald, John
2014-11-01
Planck favours a negative running of the spectral index, with the likelihood being dominated by low multipoles l?<50 and no preference for running at higher l. A negative spectral index is also necessary for the 2- Planck upper bound on the tensor-to-scalar ratio r to be consistent with values significantly larger than 0.1. Planck has also observed a hemispherical asymmetry of the CMB power spectrum, again mostly at low multipoles. Here we consider whether the physics responsible for the hemispherical asymmetry could also account for the negative running of the spectral index and the consistency of Planck with a large value of r. A negative running of the spectral index can be generated if the hemispherical asymmetry is due to a scale- and space-dependent modulation which suppresses the CMB power spectrum at low multipoles. We show that the observed hemispherical asymmetry at low l can be generated while satisfying constraints on the asymmetry at higher l and generating a negative spectral index of the right magnitude to account for the Planck observation and to allow Planck to be consistent with a large value of r.
Symmetry breaking indication for supergravity inflation in light of the Planck 2015
Li, Tianjun; Li, Zhijin; Nanopoulos, Dimitri V.
2015-09-01
Supergravity (SUGRA) theories with exact global U(1) symmetry or shift symmetry in Kähler potential provide natural frameworks for inflation. However, quadratic inflation is disfavoured by the new results on primordial tensor fluctuations from the Planck Collaboration. To be consistent with the new Planck data, we point out that the explicit symmetry breaking is needed, and study these two SUGRA inflation in detail. For SUGRA inflation with global U(1) symmetry, the symmetry breaking term leads to a trigonometric modulation on inflaton potential. Coefficient of the U(1) symmetry breaking term is of order 10{sup −2}, which is sufficient large to improve the inflationary predictions while its higher order corrections are negligible. Such models predict sizeable tensor fluctuations and highly agree with the Planck results. In particular, the model with a linear U(1) symmetry breaking term predicts the tensor-to-scalar ratio around r∼0.01 and running spectral index α{sub s}∼−0.004, which comfortably fit with the Planck observations. For SUGRA inflation with breaking shift symmetry, the inflaton potential is modulated by an exponential factor. The modulated linear and quadratic models are consistent with the Planck observations. In both types of models the tensor-to-scalar ratio can be of order 10{sup −2}, which will be tested by the near future observations.
A Generalized Fokker-Planck Model for Transport of Collimated Beams
Prinja, Anil K.; Pomraning, G.C.
2001-03-15
A generalized Fokker-Planck (GFP) model is introduced for application to the problem of the angular spreading of a broad beam of charged particles. This approach extends the classic Fokker-Planck (FP) approximation of the scattering operator to instances when the differential scattering cross section is not sufficiently forward peaked for the strict FP representation to be valid. Our previously developed (1 - {mu}){sup n}-moments method is used to construct a truncated hierarchy of moment equations from the GFP and transport equations. For slab thicknesses that are small compared to the transport mean-free-path, the scalar flux is explicitly represented as a Taylor expansion in the depth variable for different truncation orders and for different orders of the generalized Fokker-Planck expansion. Numerical results indicate that the GFP method is a viable method for dealing with larger scattering angles than are possible with the classic FP approximation.
Energy Tomorrow | Department of Energy
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2011 Serena DeBeer of Cornell University and the Max Planck Institute for Bioinorganic Chemistry, led the the team that performed crucial experiments at SLAC. Dr. DeBeer is...
Wiegel, Detlef
2011-04-25
Detlef Wiegel from the Max Planck Institute for Developmental Biology on "Next-generation genetics in plants: Evolutionary tradeoffs, immunity and speciation" on March 25, 2010 at the 5th Annual DOE JGI User Meeting
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Li Xu 1 (lixum@umich.edu), Joyce E. Penner 1 and Swen Metzger 2 1 Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan 2 Max Planck Institute for ...
PPPL engineers complete the design of Wendelstein 7-X scraper...
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finished designing a novel component for the Wendelstein 7-X (W7-X) stellarator, which recently opened at the Max Planck Institute of Plasma Physics (IPP) in Griefswald, Germany. ...
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Walter Steininger is a physicist (University of Stuttgart). He made his doctoral thesis at the Max-Planck-Institute for Material Research, Material Science, and worked as a project ...
COLLOQUIUM: W7-X Status Report | Princeton Plasma Physics Lab
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November 12, 2015, 4:15pm to 5:30pm Colloquia MBG AUDITORIUM COLLOQUIUM: W7-X Status Report Dr. Thomas Sunn Pedersen Max Planck Institute of Plasma Physics Presentation: File ...
Tests of Monte Carlo Independent Column Approximation in the...
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In this work, McICA and a stochastic cloud generator have been implemented to the Max Planck Institute for Meteorology's ECHAM5 atmospheric GCM. The impact of McICA noise on ...
From corrosion to batteries: Electrochemical interface studies...
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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 ...
Tomče Runčevski | Center for Gas SeparationsRelevant to Clean...
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University of California, Berkeley Email: runcevski@berkeley.edu Phone: 510-708-2455 PhD in Materials Chemistry, Max Planck Institute for Solid State Research and Stuttgart ...
Ji-Woong Lee | Center for Gas SeparationsRelevant to Clean Energy...
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Email: jiwoong.lee at berkeley.edu Phone: 510-643-3832 PhD in Chemistry, Max-Planck Institut fuer Kohlenforschung, Germany BSc and MSc in Chemistry, Sungkyunkwan University, ...
Markus Mezger | Center for Gas SeparationsRelevant to Clean Energy...
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Presently: Project leader, Max Planck Institute for Polymer Research, Mainz, Germany Email: mezger at mpip-mainz.mpg.de Diploma in Physics, Stuttgart University, Germany PhD in ...
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Biology Matthias Scheffler Fritz-Haber-Institut der Max-Planck-Gesellschaft, Berlin, Germany CNMS D D I I S S C C O O V V E E R R Y Y SEMINAR SERIES Abstract: Dispersive or van...
North-South non-Gaussian asymmetry in Planck CMB maps
Bernui, A.; Oliveira, A.F.; Pereira, T.S. E-mail: adhimar@unifei.edu.br
2014-10-01
We report the results of a statistical analysis performed with the four foreground-cleaned Planck maps by means of a suitably defined local-variance estimator. Our analysis shows a clear dipolar structure in Planck's variance map pointing in the direction (l,b)?(220,-32), thus consistent with the North-South asymmetry phenomenon. Surprisingly, and contrary to previous findings, removing the CMB quadrupole and octopole makes the asymmetry stronger. Our results show a maximal statistical significance, of 98.1% CL, in the scales ranging from ?=4 to ?=500. Additionally, through exhaustive analyses of the four foreground-cleaned and individual frequency Planck maps, we find unlikely that residual foregrounds could be causing this dipole variance asymmetry. Moreover, we find that the dipole gets lower amplitudes for larger masks, evidencing that most of the contribution to the variance dipole comes from a region near the galactic plane. Finally, our results are robust against different foreground cleaning procedures, different Planck masks, pixelization parameters, and the addition of inhomogeneous real noise.
The Fokker-Planck limit of a family of transport differencing methods
Anistratov, D.Y.
1998-12-31
Recently, Pomraning performed an asymptotic analysis of the Fokker-Planck (FP) limit for the analytic transport equation with a forward-peaked scattering kernel. Then, Adams and Pautz extended this analysis to the discrete ordinates transport equation and studied some difference schemes. In this paper a broad family of transport differencing methods is analyzed.
Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and...
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Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours Docket No. ...
Planck CMB anomalies: astrophysical and cosmological secondary effects and the curse of masking
Rassat, A.; Starck, J.-L.; Paykari, P.; Sureau, F.; Bobin, J. E-mail: jstarck@cea.fr E-mail: florent.sureau@cea.fr
2014-08-01
Large-scale anomalies have been reported in CMB data with both WMAP and Planck data. These could be due to foreground residuals and or systematic effects, though their confirmation with Planck data suggests they are not due to a problem in the WMAP or Planck pipelines. If these anomalies are in fact primordial, then understanding their origin is fundamental to either validate the standard model of cosmology or to explore new physics. We investigate three other possible issues: 1) the trade-off between minimising systematics due to foreground contamination (with a conservative mask) and minimising systematics due to masking, 2) astrophysical secondary effects (the kinetic Doppler quadrupole and kinetic Sunyaev-Zel'dovich effect), and 3) secondary cosmological signals (the integrated Sachs-Wolfe effect). We address the masking issue by considering new procedures that use both WMAP and Planck to produce higher quality full-sky maps using the sparsity methodology (LGMCA maps). We show the impact of masking is dominant over that of residual foregrounds, and the LGMCA full-sky maps can be used without further processing to study anomalies. We consider four official Planck PR1 and two LGMCA CMB maps. Analysis of the observed CMB maps shows that only the low quadrupole and quadrupole-octopole alignment seem significant, but that the planar octopole, Axis of Evil, mirror parity and cold spot are not significant in nearly all maps considered. After subtraction of astrophysical and cosmological secondary effects, only the low quadrupole may still be considered anomalous, meaning the significance of only one anomaly is affected by secondary effect subtraction out of six anomalies considered. In the spirit of reproducible research all reconstructed maps and codes will be made available for download here http://www.cosmostat.org/anomaliesCMB.html.
Diffusion of Ag, Au and Cs implants in MAX phase Ti3SiC2 (Journal...
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Title: Diffusion of Ag, Au and Cs implants in MAX phase Ti3SiC2 MAX phases (M: early transition metal; A: elements in group 13 or 14; X: C or N), such as titanium silicon carbide ...
ARM - Field Campaign - 2006 MAX-Mex-Megacity Aerosol eXperiment - Mexico
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City 6 MAX-Mex-Megacity Aerosol eXperiment - Mexico City ARM Data Discovery Browse Data Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : 2006 MAX-Mex-Megacity Aerosol eXperiment - Mexico City 2006.03.03 - 2006.03.28 Lead Scientist : Jeffrey Gaffney For data sets, see below. Abstract A 4-week field campaign was conducted in and downwind of Mexico City during March 2006. The Megacity Aerosol eXperiment - MEXico City (MAX-MEX)
max walltime for low queue is increased to 24 hrs on Hopper
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max walltime for low queue is increased to 24 hrs on Hopper max walltime for low queue is increased to 24 hrs on Hopper May 31, 2012 by Helen He We have increased the max walltime for the low queue on Hopper from 12 to 24 hrs. Subscribe via RSS Subscribe Browse by Date February 2013 September 2012 August 2012 May 2012 April 2012 March 2012 February 2012 January 2012 November 2011 October 2011 September 2011 August 2011 July 2011 June 2011 May 2011 April 2011 March 2011 February 2011 January 2011
runtime error message: "apsched: request exceeds max nodes, alloc"
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apsched: request exceeds max nodes, alloc" runtime error message: "apsched: request exceeds max nodes, alloc" September 12, 2014 Symptom: User jobs with single or multiple apruns in a batch script may get this runtime error. "apsched: request exceeds max nodes, alloc". This problem is intermittent, started in April, then mid July, and again since late August. Status: This problem is identified as a problem when Torque/Moab batch scheduler becomes out of sync with the
Quantum dynamics via Planck-scale-stepped action-carrying 'Graph Paths'
Chew, Geoffrey F.
2003-05-05
A divergence-free, parameter-free, path-based discrete-time quantum dynamics is designed to not only enlarge the achievements of general relativity and the standard particle model, by approximations at spacetime scales far above Planck scale while far below Hubble scale, but to allow tackling of hitherto inaccessible questions. ''Path space'' is larger than and precursor to Hilbert-space basis. The wave-function-propagating paths are action-carrying structured graphs-cubic and quartic structured vertices connected by structured ''fermionic'' or ''bosonic'' ''particle'' and ''nonparticle'' arcs. A Planck-scale path step determines the gravitational constant while controlling all graph structure. The basis of the theory's (zero-rest-mass) elementary-particle Hilbert space (which includes neither gravitons nor scalar bosons) resides in particle arcs. Nonparticle arcs within a path are responsible for energy and rest mass.
Sensitivity analysis for dose deposition in radiotherapy via a Fokker–Planck model
DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)
Barnard, Richard C.; Frank, Martin; Krycki, Kai
2016-02-09
In this paper, we study the sensitivities of electron dose calculations with respect to stopping power and transport coefficients. We focus on the application to radiotherapy simulations. We use a Fokker–Planck approximation to the Boltzmann transport equation. Equations for the sensitivities are derived by the adjoint method. The Fokker–Planck equation and its adjoint are solved numerically in slab geometry using the spherical harmonics expansion (PN) and an Harten-Lax-van Leer finite volume method. Our method is verified by comparison to finite difference approximations of the sensitivities. Finally, we present numerical results of the sensitivities for the normalized average dose deposition depthmore » with respect to the stopping power and the transport coefficients, demonstrating the increase in relative sensitivities as beam energy decreases. In conclusion, this in turn gives estimates on the uncertainty in the normalized average deposition depth, which we present.« less
An Asymptotic Study of Discretized Transport Equations in the Fokker-Planck Limit
Pautz, Shawn D.; Adams, Marvin L.
2002-01-15
Recent analyses have shown that the Fokker-Planck equation is an asymptotic limit of the transport equation given a forward-peaked scattering kernel satisfying certain constraints. Discretized transport equations in the same limit are studied, both by asymptotic analysis and by numerical testing. It is shown that spatially discretized discrete ordinates transport solutions can be accurate in this limit if and only if the scattering operator is handled in a certain nonstandard way.
Current dependence of spin torque switching rate based on Fokker-Planck approach
Taniguchi, Tomohiro Imamura, Hiroshi
2014-05-07
The spin torque switching rate of an in-plane magnetized system in the presence of an applied field is derived by solving the Fokker-Planck equation. It is found that three scaling currents are necessary to describe the current dependence of the switching rate in the low-current limit. The dependences of these scaling currents on the applied field strength are also studied.
Zhang, Jing-Fei; Geng, Jia-Jia; Zhang, Xin E-mail: gengjiajia163@163.com
2014-10-01
The detection of the B-mode polarization of the cosmic microwave background (CMB) by the BICEP2 experiment implies that the tensor-to-scalar ratio r should be involved in the base standard cosmology. In this paper, we extend the ΛCDM r+neutrino/dark radiation models by replacing the cosmological constant with the dynamical dark energy with constant w. Four neutrino plus dark energy models are considered, i.e., the wCDM r ∑ m{sub ν}, wCDM r N{sub eff}, wCDM r ∑ m{sub ν} N{sub eff}, and wCDM r N{sub eff} m{sub ν,sterile}{sup eff} models. The current observational data considered in this paper include the Planck temperature data, the WMAP 9-year polarization data, the baryon acoustic oscillation data, the Hubble constant direct measurement data, the Planck Sunyaev-Zeldovich cluster counts data, the Planck CMB lensing data, the cosmic shear data, and the BICEP2 polarization data. We test the data consistency in the four cosmological models, and then combine the consistent data sets to perform joint constraints on the models. We focus on the constraints on the parameters w, ∑ m{sub ν}, N{sub eff}, and m{sub ν,sterile}{sup eff}.
The precise time-dependent solution of the Fokker–Planck equation with anomalous diffusion
Guo, Ran; Du, Jiulin
2015-08-15
We study the time behavior of the Fokker–Planck equation in Zwanzig’s rule (the backward-Ito’s rule) based on the Langevin equation of Brownian motion with an anomalous diffusion in a complex medium. The diffusion coefficient is a function in momentum space and follows a generalized fluctuation–dissipation relation. We obtain the precise time-dependent analytical solution of the Fokker–Planck equation and at long time the solution approaches to a stationary power-law distribution in nonextensive statistics. As a test, numerically we have demonstrated the accuracy and validity of the time-dependent solution. - Highlights: • The precise time-dependent solution of the Fokker–Planck equation with anomalous diffusion is found. • The anomalous diffusion satisfies a generalized fluctuation–dissipation relation. • At long time the time-dependent solution approaches to a power-law distribution in nonextensive statistics. • Numerically we have demonstrated the accuracy and validity of the time-dependent solution.
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text in "Max kWh" fields | OpenEI Community
it should as we are trying to prevent users from writing "less than X", "greater than Y", etc. and follow the intention of the "Max kWh" field. Also there should be a warning...
Frederic Laquai Seminar: Photocurrent Generation in Low-Bandgap Polymer and
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Small Molecule Organic Solar Cells | Center for Energy Efficient Materials Frederic Laquai Seminar: Photocurrent Generation in Low-Bandgap Polymer and Small Molecule Organic Solar Cells Apr 18, 2014 | 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 Polymer and Small Molecule Organic Solar Cells April 18, 2014 | 3:30pm | Elings Hall (CNSI) 1605 Faculty host: Quyen
Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated
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Refrigerant | Department of Energy Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated Refrigerant Max Tech Electric Heat Pump Water Heater with Lower GWP Halogenated Refrigerant Information flow schematic for an integrated heat pump design model and wrapped tank model. Image credit: Oak Ridge National Laboratory. Information flow schematic for an integrated heat pump design model and wrapped tank model. Image credit: Oak Ridge National Laboratory. Information flow schematic
A joint analysis of Planck and BICEP2 B modes including dust polarization uncertainty
Mortonson, Michael J.; Seljak, Uro E-mail: useljak@berkeley.edu
2014-10-01
We analyze BICEP2 and Planck data using a model that includes CMB lensing, gravity waves, and polarized dust. Recently published Planck dust polarization maps have highlighted the difficulty of estimating the amount of dust polarization in low intensity regions, suggesting that the polarization fractions have considerable uncertainties and may be significantly higher than previous predictions. In this paper, we start by assuming nothing about the dust polarization except for the power spectrum shape, which we take to be C{sub l}{sup BB,dust}?l{sup -2.42}. The resulting joint BICEP2+Planck analysis favors solutions without gravity waves, and the upper limit on the tensor-to-scalar ratio is r<0.11, a slight improvement relative to the Planck analysis alone which gives r<0.13 (95% c.l.). The estimated amplitude of the dust polarization power spectrum agrees with expectations for this field based on both HI column density and Planck polarization measurements at 353 GHz in the BICEP2 field. Including the latter constraint on the dust spectrum amplitude in our analysis improves the limit further to r<0.09, placing strong constraints on theories of inflation (e.g., models with r>0.14 are excluded with 99.5% confidence). We address the cross-correlation analysis of BICEP2 at 150 GHz with BICEP1 at 100 GHz as a test of foreground contamination. We find that the null hypothesis of dust and lensing with 0r= gives ??{sup 2}<2 relative to the hypothesis of no dust, so the frequency analysis does not strongly favor either model over the other. We also discuss how more accurate dust polarization maps may improve our constraints. If the dust polarization is measured perfectly, the limit can reach r<0.05 (or the corresponding detection significance if the observed dust signal plus the expected lensing signal is below the BICEP2 observations), but this degrades quickly to almost no improvement if the dust calibration error is 20% or larger or if the dust maps are not
On the significance of power asymmetries in Planck CMB data at all scales
Quartin, Miguel [Instituto de Fsica, Universidade Federal do Rio de Janeiro, 21941-972, Rio de Janeiro, RJ (Brazil); Notari, Alessio, E-mail: mquartin@if.ufrj.br, E-mail: notari@ffn.ub.es [Departament de Fsica Fondamental i Institut de Cincies del Cosmos, Universitat de Barcelona, Mart i Franqus 1, E-08028 Barcelona (Spain)
2015-01-01
We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if there is any significant deviation from cosmological isotropy. We look for differences in the spectrum between two opposite hemispheres and also for dipolar modulations. We propose a new way to avoid biases due to partial-sky coverage by producing a mask symmetrized in antipodal directions, in addition to the standard smoothing procedure. We also properly take into account both Doppler and aberration effects due to our peculiar velocity and the anisotropy of the noise, since these effects induce a significant hemispherical asymmetry. We are thus able to probe scales all the way to ?=2000. After such treatment we find no evidence for significant hemispherical anomalies along any of the analyzed directions (i.e. deviations are less than 1.5? when summing over all scales). Although among the larger scales there are sometimes higher discrepancies, these are always less than 3?. We also find results on a dipolar modulation of the power spectrum. Along the hemispheres aligned with the most asymmetric direction for 2???2000 we find a 3.3? discrepancy when comparing to simulations. However, if we do not restrict ourselves to Planck's maximal asymmetry axis, which can only be known a posteriori, and compare Planck data with the modulation of simulations along their respective maximal asymmetry directions, the discrepancy goes down to less than 1? (with, again, almost 3? discrepancies in some low-? modes). We thus conclude that no significant power asymmetries seem to be present in the full data set. Interestingly, without proper removal of Doppler and aberration effects one would find spurious anomalies at high ?, between 3? and 5?. Even when considering only ?<600 we find that the boost is non-negligible and alleviates the discrepancy by roughly half-?.
Mesoscopic superposition of states with sub-Planck structures in phase space
Agarwal, G.S.; Pathak, P.K.
2004-11-01
We propose the cavity quantum electrodynamics method, using dispersive interaction between atoms and a high-quality cavity to realize the mesoscopic superposition of coherent states that would exhibit sub-Planck structures in phase space, i.e., the structures at a scale smaller than the Plank's constant (({Dirac_h}/2{pi})). These structures are direct signatures of quantum coherence and are formed as a result of interference between the two superposed cat states. In particular we focus on a superposition involving four coherent states. We show interferences in the conditional measurements involving two atoms.
Fokker-Planck Modelling of Delayed Loss of Charged Fusion Products in TFTR.
Edenstrasser, J.W.; Goloborod'ko, V.Ya.; Reznik, S.N.; Yavorskij, V.A.; Zweben, S.
1998-08-01
The results of a Fokker-Planck simulation of the ripple-induced loss of charged fusion products in the Tokamak Fusion Test Reactor (TFTR) are presented. It is shown that the main features of the measured "delayed loss" of partially thermalized fusion products, such as the differences between deuterium-deuterium and deuterium-tritium discharges, the plasma current and major radius dependencies, etc., are in satisfactory agreement with the classical collisional ripple transport mechanism. The inclusion of the inward shift of the vacuum flux surfaces turns out to be necessary for an adequate and consistent explanation of the origin of the partially thermalized fusion product loss to the bottom of TFTR.
Diffusion coefficients of Fokker-Planck equation for rotating dust grains in a fusion plasma
Bakhtiyari-Ramezani, M. Alinejad, N.; Mahmoodi, J.
2015-11-15
In the fusion devices, ions, H atoms, and H{sub 2} molecules collide with dust grains and exert stochastic torques which lead to small variations in angular momentum of the grain. By considering adsorption of the colliding particles, thermal desorption of H atoms and normal H{sub 2} molecules, and desorption of the recombined H{sub 2} molecules from the surface of an oblate spheroidal grain, we obtain diffusion coefficients of the Fokker-Planck equation for the distribution function of fluctuating angular momentum. Torque coefficients corresponding to the recombination mechanism show that the nonspherical dust grains may rotate with a suprathermal angular velocity.
COLLOQUIUM: Small-scale CMB Cosmology: ACT, Planck and Beyond | Princeton
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Plasma Physics Lab June 25, 2014, 4:00pm to 5:30pm Colloquia MBG Auditorium COLLOQUIUM: Small-scale CMB Cosmology: ACT, Planck and Beyond Dr. Renee Hlozek Princeton University Abstract: PDF icon COLL.06.25.14.pdf The Atacama Cosmology Telescope (ACT) has mapped the microwave sky to arcminute scales. We present constraints on parameters from the observations at 148 and 217 GHz respectively by ACT from three years of observations. We fit a model of primary cosmological and secondary foreground
INSTITUTE COLLOQUIA AND SEMINARS
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INSTITUTE INSTITUTE INSTITUTE INSTITUTE COLLOQUIA AND SEMINARS April 1, 2000-March 31, 2001 2000 April 4 Dr. B. Launé, Institut de Physique Nucléaire - Orsay, France GANIL: Overview and Perspectives April 11 Dr. Z. Lin, Cyclotron Institute, TAMU J/psi Absorption in Hadronic Matter April 20 Dr. R. Tribble, Texas A&M University Nuclear Astrophysics at Texas A&M April 23 Prof. S.A. Gurvitz, The Weizmann Institute of Science, Rehovot, Israel Confinement and Scaling in Deep Inelastic
Gibbs, Zachary M.; Kim, Hyun-Sik; Wang, Heng; Snyder, G. Jeffrey
2015-01-12
In characterizing thermoelectric materials, electrical and thermal transport measurements are often used to estimate electronic band structure properties such as the effective mass and band gap. The Goldsmid-Sharp band gap, E{sub g}?=?2e|S|{sub max}T{sub max}, is a tool widely employed to estimate the band gap from temperature dependent Seebeck coefficient measurements. However, significant deviations of more than a factor of two are now known to occur. We find that this is when either the majority-to-minority weighted mobility ratio (A) becomes very different from 1.0 or as the band gap (E{sub g}) becomes significantly smaller than 10 k{sub B}T. For narrow gaps (E{sub g}???6 k{sub B}T), the Maxwell-Boltzmann statistics applied by Goldsmid-Sharp break down and Fermi-Dirac statistics are required. We generate a chart that can be used to quickly estimate the expected correction to the Goldsmid-Sharp band gap depending on A and S{sub max}; however, additional errors can occur for S?
Claire E. Max, 2004 | U.S. DOE Office of Science (SC)
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Claire E. Max, 2004 The Ernest Orlando Lawrence Award Lawrence Award Home Nomination & Selection Guidelines Award Laureates 2010's 2000's 1990's 1980's 1970's 1960's Ceremony The Life of Ernest Orlando Lawrence Contact Information The Ernest Orlando Lawrence Award U.S. Department of Energy SC-2/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-2411 E: Email Us 2000's Claire E. Max, 2004 Print Text Size: A A A FeedbackShare Page Physics: For her contributions to
Self-unitarization of New Higgs Inflation and compatibility with Planck and BICEP2 data
Germani, Cristiano; Wintergerst, Nico; Watanabe, Yuki E-mail: watanabe@resceu.s.u-tokyo.ac.jp
2014-12-01
In this paper we show that the Germani-Kehagias model of Higgs inflation (or New Higgs Inflation), where the Higgs boson is kinetically non-minimally coupled to the Einstein tensor is in perfect compatibility with the latest Planck and BICEP2 data. Moreover, we show that the tension between the Planck and BICEP2 data can be relieved within the New Higgs inflation scenario by a negative running of the spectral index. Regarding the unitarity of the model, we argue that it is unitary throughout the evolution of the Universe. Weak couplings in the Higgs-Higgs and Higgs-graviton sectors are provided by a large background dependent cut-off scale during inflation. In the same regime, the W and Z gauge bosons acquire a very large mass, thus decouple. On the other hand, if they are also non-minimally coupled to the Higgs boson, their effective masses can be enormously reduced. In this case, the W and Z bosons are no longer decoupled. After inflation, the New Higgs model is well approximated by a quartic Galileon with a renormalizable potential. We argue that this can unitarily create the right conditions for inflation to eventually start.
An efficient particle FokkerPlanck algorithm for rarefied gas flows
Gorji, M. Hossein; Jenny, Patrick
2014-04-01
This paper is devoted to the algorithmic improvement and careful analysis of the FokkerPlanck kinetic model derived by Jenny et al. [1] and Gorji et al. [2]. The motivation behind the FokkerPlanck based particle methods is to gain efficiency in low Knudsen rarefied gas flow simulations, where conventional direct simulation Monte Carlo (DSMC) becomes expensive. This can be achieved due to the fact that the resulting model equations are continuous stochastic differential equations in velocity space. Accordingly, the computational particles evolve along independent stochastic paths and thus no collision needs to be calculated. Therefore the computational cost of the solution algorithm becomes independent of the Knudsen number. In the present study, different computational improvements were persuaded in order to augment the method, including an accurate time integration scheme, local time stepping and noise reduction. For assessment of the performance, gas flow around a cylinder and lid driven cavity flow were studied. Convergence rates, accuracy and computational costs were compared with respect to DSMC for a range of Knudsen numbers (from hydrodynamic regime up to above one). In all the considered cases, the model together with the proposed scheme give rise to very efficient yet accurate solution algorithms.
Jaeger, E.F.; Berry, L.A.; Batchelor, D.B.; Carter, M.D.; D'Azevedo, E.; Harvey, R.W.; Myra, J.R.; D'Ippolito, D.A.; Dumont, R.J.; Smithe, D.N.; Bonoli, P.T.; Wright, J.C.
2005-09-26
Self-consistent solutions for the wave electric field and particle distribution function are calculated for ion cyclotron heating in non-Maxwellian plasmas. The all-orders wave solver AORSA is generalized to treat non-thermal velocity distributions arising from fusion reactions, neutral beam injection, and wave driven diffusion in velocity space. Quasi-linear diffusion coefficients are derived directly from the wave electric fields and used to calculate velocity distribution functions with the CQL3D Fokker-Planck code. Self-consistent results are obtained by iterating the full-wave and Fokker-Planck solutions.
The Critical Materials Institute | Critical Materials Institute
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The Critical Materials Institute Director Alex King, Operations Manager Cynthia Feller, Jenni Brockpahler and Melinda Thach. Photo left to right: CMI Director Alex King, Operations Manager Cynthia Feller, Jenni Brockpahler and Melinda Thach. Not pictured: Carol Bergman. CMI staff phone 515-296-4500, e-mail CMIdirector@ameslab.gov 2332 Pammel Drive, 134 Wilhelm Hall, Iowa State University, Ames, IA 50011-1025 The Critical Materials Institute focuses on technologies that make better use of
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Institute » Advanced Studies Institute Science of Signatures Advanced Studies Institute Developing innovative solution strategies for problems that support the forward deployment theme of the Science of Signatures Pillar, and building skills needed for successful research program development. Contact Institute Director Charles Farrar (505) 665-0860 Email UCSD EI Director Michael Todd (858) 534-5951 Executive Administrator Ellie Vigil (505) 667-2818 Email Administrative Assistant Rebecca Duran
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5-March 31, 2006 2005 April 1 Dr. Ralf Rapp, Cyclotron Institute, Texas A&M University, College Station, Texas Thermal Field Theory and Instantons II April 8 Mr. Deqiang Sun, Cyclotron Institute, Texas A&M University, College Station, Texas Bottomonium in QGP and Heavy-Ion Collisions April 22 Dr. Ralf Rapp, Cyclotron Institute, Texas A&M University, College Station, Texas Thermal Field Theory and Instantons III May 6 Dr. Massimo Mannarelli, Massachusetts Institute of Technology,
Southern Research Institute Visit
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Southern Reaserch Engineering Capabilities Briefing 2010 Southern Research Institute Pharmaceutical and Biotechnology Research Briefing 2010 CAMD Introduction - Richard Kurtz Mary ...
Kirk, D.; et al.
2015-12-14
We measure the cross-correlation between weak lensing of galaxy images and of the cosmic microwave background (CMB). The effects of gravitational lensing on different sources will be correlated if the lensing is caused by the same mass fluctuations. We use galaxy shape measurements from 139 deg$^{2}$ of the Dark Energy Survey (DES) Science Verification data and overlapping CMB lensing from the South Pole Telescope (SPT) and Planck. The DES source galaxies have a median redshift of $z_{\\rm med} {\\sim} 0.7$, while the CMB lensing kernel is broad and peaks at $z{\\sim}2$. The resulting cross-correlation is maximally sensitive to mass fluctuations at $z{\\sim}0.44$. Assuming the Planck 2015 best-fit cosmology, the amplitude of the DES$\\times$SPT cross-power is found to be $A = 0.88 \\pm 0.30$ and that from DES$\\times$Planck to be $A = 0.86 \\pm 0.39$, where $A=1$ corresponds to the theoretical prediction. These are consistent with the expected signal and correspond to significances of $2.9 \\sigma$ and $2.2 \\sigma$ respectively. We demonstrate that our results are robust to a number of important systematic effects including the shear measurement method, estimator choice, photometric redshift uncertainty and CMB lensing systematics. Significant intrinsic alignment of galaxy shapes would increase the cross-correlation signal inferred from the data; we calculate a value of $A = 1.08 \\pm 0.36$ for DES$\\times$SPT when we correct the observations with a simple IA model. With three measurements of this cross-correlation now existing in the literature, there is not yet reliable evidence for any deviation from the expected LCDM level of cross-correlation, given the size of the statistical uncertainties and the significant impact of systematic errors, particularly IAs. We provide forecasts for the expected signal-to-noise of the combination of the five-year DES survey and SPT-3G.
Sloan, D.P.
1983-05-01
Morel (1981) has developed multigroup Legendre cross sections suitable for input to standard discrete ordinates transport codes for performing charged-particle Fokker-Planck calculations in one-dimensional slab and spherical geometries. Since the Monte Carlo neutron transport code, MORSE, uses the same multigroup cross section data that discrete ordinates codes use, it was natural to consider whether Fokker-Planck calculations could be performed with MORSE. In order to extend the unique three-dimensional forward or adjoint capability of MORSE to Fokker-Planck calculations, the MORSE code was modified to correctly treat the delta-function scattering of the energy operator, and a new set of physically acceptable cross sections was derived to model the angular operator. Morel (1979) has also developed multigroup Legendre cross sections suitable for input to standard discrete ordinates codes for performing electron Boltzmann calculations. These electron cross sections may be treated in MORSE with the same methods developed to treat the Fokker-Planck cross sections. The large magnitude of the elastic scattering cross section, however, severely increases the computation or run time. It is well-known that approximate elastic cross sections are easily obtained by applying the extended transport (or delta function) correction to the Legendre coefficients of the exact cross section. An exact method for performing the extended transport cross section correction produces cross sections which are physically acceptable. Sample calculations using electron cross sections have demonstrated this new technique to be very effective in decreasing the large magnitude of the cross sections.
Deterministic proton transport solving a one dimensional Fokker-Planck equation
Marr, D.; Prael, R.; Adams, K.; Alcouffe, R.
1997-10-01
The transport of protons through matter is characterized by many interactions which cause small deflections and slight energy losses. The few which are catastrophic or cause large angle scattering can be viewed as extinction for many applications. The transport of protons at this level of approximation can be described by a Fokker Planck Equation. This equation is solved using a deterministic multigroup differencing scheme with a highly resolved set of discrete ordinates centered around the beam direction which is adequate to properly account for deflections and energy losses due to multiple Coulomb scattering. Comparisons with LAHET for a large variety of problems ranging from 800 MeV protons on a copper step wedge to 10 GeV protons on a sandwich of material are presented. The good agreement with the Monte Carlo code shows that the solution method is robust and useful for approximate solutions of selected proton transport problems.
Inflation Induced Planck-Size Black Hole Remnants as Dark Matter
Chen, P
2004-07-06
While there exist various candidates, the identification of dark matter remains unresolved. Recently it was argued that the generalized uncertainty principle (GUP) may prevent a black hole from evaporating completely, and as a result there should exist a Planck-size BHR at the end of its evaporation. We speculate that the stability of BHR may be further protected by supersymmetry in the form of extremal black hole. If this is indeed the case and if a sufficient amount of small black holes can be produced in the early universe, then the resultant BHRs can be an interesting candidate for DM. We demonstrate that this is the case in the hybrid inflation model. By assuming BHR as DM, our notion imposes a constraint on the hybrid inflation potential. We show that such a constraint is not fine-tuned. Possible observational signatures are briefly discussed.
Higher order statistics of curvature perturbations in IFF model and its Planck constraints
Fujita, Tomohiro; Yokoyama, Shuichiro E-mail: shu@icrr.u-tokyo.ac.jp
2013-09-01
We compute the power spectrum P{sub ζ} and non-linear parameters f{sub NL} and τ{sub NL} of the curvature perturbation induced during inflation by the electromagnetic fields in the kinetic coupling model (IFF model). By using the observational result of P{sub ζ},f{sub NL} and τ{sub NL} reported by the Planck collaboration, we study the constraint on the model comprehensively. Interestingly, if the single slow-rolling inflaton is responsible for the observed P{sub ζ}, the constraint from τ{sub NL} is most stringent. We also find a general relationship between f{sub NL} and τ{sub NL} generated in this model. Even if f{sub NL} ∼ O(1), a detectable τ{sub NL} can be produced.
A High-Order Finite-Volume Algorithm for Fokker-Planck Collisions in Magnetized Plasmas
Xiong, Z; Cohen, R H; Rognlien, T D; Xu, X Q
2007-04-18
A high-order finite volume algorithm is developed for the Fokker-Planck Operator (FPO) describing Coulomb collisions in strongly magnetized plasmas. The algorithm is based on a general fourth-order reconstruction scheme for an unstructured grid in the velocity space spanned by parallel velocity and magnetic moment. The method provides density conservation and high-order-accurate evaluation of the FPO independent of the choice of the velocity coordinates. As an example, a linearized FPO in constant-of-motion coordinates, i.e. the total energy and the magnetic moment, is developed using the present algorithm combined with a cut-cell merging procedure. Numerical tests include the Spitzer thermalization problem and the return to isotropy for distributions initialized with velocity space loss cones. Utilization of the method for a nonlinear FPO is straightforward but requires evaluation of the Rosenbluth potentials.
Does the first chaotic inflation model in supergravity provide the best fit to the Planck data?
Linde, Andrei
2015-02-23
I describe the first model of chaotic inflation in supergravity, which was proposed by Goncharov and the present author in 1983. The inflaton potential of this model has a plateau-type behavior V{sub 0}(1−(8/3) e{sup −√6|ϕ|}) at large values of the inflaton field. This model predicts n{sub s}=1−(2/N)≈0.967 and r=(4/(3N{sup 2}))≈4×10{sup −4}, in good agreement with the Planck data. I propose a slight generalization of this model, which allows to describe not only inflation but also dark energy and supersymmetry breaking.
Analytical and Numerical Solutions of Generalized Fokker-Planck Equations - Final Report
Prinja, Anil K.
2000-12-31
The overall goal of this project was to develop advanced theoretical and numerical techniques to quantitatively describe the spreading of a collimated beam of charged particles in space, in angle, and in energy, as a result of small deflection, small energy transfer Coulomb collisions with the target nuclei and electrons. Such beams arise in several applications of great interest in nuclear engineering, and include electron and ion radiotherapy, ion beam modification of materials, accelerator transmutation of waste, and accelerator production of tritium, to name some important candidates. These applications present unique and difficult modeling challenges, but from the outset are amenable to the language of ''transport theory'', which is very familiar to nuclear engineers and considerably less-so to physicists and material scientists. Thus, our approach has been to adopt a fundamental description based on transport equations, but the forward peakedness associated with charged particle interactions precludes a direct application of solution methods developed for neutral particle transport. Unique problem formulations and solution techniques are necessary to describe the transport and interaction of charged particles. In particular, we have developed the Generalized Fokker-Planck (GFP) approach to describe the angular and radial spreading of a collimated beam and a renormalized transport model to describe the energy-loss straggling of an initially monoenergetic distribution. Both analytic and numerical solutions have been investigated and in particular novel finite element numerical methods have been developed. In the first phase of the project, asymptotic methods were used to develop closed form solutions to the GFP equation for different orders of expansion, and was described in a previous progress report. In this final report we present a detailed description of (i) a novel energy straggling model based on a Fokker-Planck approximation but which is adapted for a
Graduate Studies - Cyclotron Institute
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Students wishing to carry out their dissertation research at the Cyclotron Institute must be formally enrolled in the graduate program of either the Department of Physics or the Department of Chemistry, but may elect to work with any Institute faculty research advisor, irrespective of that advisor's departmental affiliation. Research programs at the Cyclotron Institute are funded by the U.S. Department of Energy, the National Science Foundation, and the Robert A. Welch Foundation. Application
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Emeritus Institute for Theoretical Condensed Matter Physics (KIT) The Exotic World of Quantum Matter: Novel States Induced by Fluctuations Tuesday, June 30, 2015 2 - 3pm MSL...
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Shanghai Jiao Tong University, Shanghai, China Probing the Nuclear Symmetry Energy with ... Jiansong Wang, Institute of Modern Physics, Lanzhou, China The Status of Hadronic Physics ...
Information Science & Technology Institute
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ISTI Information Science & Technology Institute Providing connection to program management for capability needs, as well as IS&T integration and support for mission-critical...
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Jeffrey W. Martin, Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California Ultracold Neutrons April 20 Professor J. W. Watson, Department of Physics, ...
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professor in the Woodruff School of Mechanical Engineering at Georgia Institute of Technology. She was previously a postdoctoral research fellow at the Center for Integrated...
Edison Electric Institute Update
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Presentation—given at the Fall 2011 Federal Utility Partnership Working Group (FUPWG) meeting—discusses the Edison Electric Institute (EEI) and the current electricity landscape.
Careers | Critical Materials Institute
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Careers The Critical Materials Institute at the The Ames Laboratory, a Department of Energy national laboratory affiliated with Iowa State University, offers a variety of career ...
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Hass, The Weizmann Institute, Rehovot, Israel A New Precision Measurement of the 7 Be ... Yigal Ronen, Ben Gurion University Beer-Sheva, Israel Space Travel: Science or Fiction? ...
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Raymond Moreh, Physics Department, Ben-Gurion University of the Negev, Beer-Sheva, Israel and Rensselaer Polytechnic Institute, Troy, New York Neutron Scattering of keV ...
Institute for Advanced Studies
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working on joint NMC proposals. Participation in the projects must not negatively impact partner institutions. Funding for joint projects should be through partner...
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Office of Legacy Management (LM)
- IL 30 FUSRAP Considered Sites Site: MAX ZUCKERMAN & SONS (IL.30 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: 1925 N. Kenmore Avenue , Chicago , Illinois IL.30-1 Evaluation Year: 1994 IL.30-2 Site Operations: Sample sized quantities of radioactive materials were shipped through this location; broker arranged purchases of materials for third party buyers. IL.30-2 Site Disposition: Eliminated - Potential for contamination
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Matty Greene About Us Matty Greene - Former Videographer Matty Greene Matty joined the Department of Energy as a videographer in May 2013, producing, filming and editing online video content for Energy. Prior to joining the Department of Energy, her other video pursuits included interning at the White House in the Office of Digital Strategy, where she filmed the President and First Lady, and making short films that played at festivals including South by Southwest. A native Austinite and avid
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... NNSA Headauarters. 1) For cyber security. direct assessment of NNSA contractors by NASA Ifeadquarters organizations consists of the following: a) Annual revieus of Site Office ...
Facilities - Cyclotron Institute
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The Cyclotron Institute has expanded steadily since commissioning the original cyclotron in 1967 and is currently upgrading again. The diagram to the left shows the variety of sophisticated detectors and spectrometers that enhance the Institute's capacity for nuclear research. Follow the above links for more detailed information about our facilities.
Cyclotron Institute Upgrade Project - Facilities - Cyclotron Institute
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Upgrade Overview / K150 Cyclotron / Light Ion Guide / Heavy Ion Guide / Negative Ion Source / CB-ECRIS Facility Upgrade White Paper Overview Picture of the experimental set up to measure beta-decay half-lives. On January 3, 2005 the Cyclotron Institute Upgrade Project (CIUP) began with the approval of the CIUP management plan by the Department of Energy Nuclear Physics Office. The project will extend to the first quarter of calendar year 2011. When completed, the upgraded facility will provide
James A. MacLachlan
2001-07-12
Numerical simulations of cooling processes over minutes or hours of real time are usually carried out using direct solution of the Fokker-Planck equation. However, by using scaling rules derived from that equation, it is possible to use macroparticle representations of the beam distribution. Besides having applications for cooling alone, the macroparticle approach allows combining the cooling process with other dynamical processes which are represented by area-preserving maps. A time-scaling rule derived from the Vlasov equation can be used to adjust the time step of a map-based dynamics calculation to one more suitable for combining with a macroparticle Fokker-Planck calculation. The time scaling for the Vlasov equation is also useful for substantially more rapid calculations when a macroparticle model of a conservative multiparticle system requires a large number of macroparticles to faithfully produce the collective potential or when the model must simulate a long time period.
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2-March 31, 2003 2002 April 2 Dr. Bency John, Cyclotron Institute, Texas A&M University Isoscalar Giant Resonances in 12 C April 9 Professor J. Rapaport, Ohio University, Athens, Ohio Charge Exchange Reactions and Spin Transfer Measurements 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 β + decay. April 23 Dr. Subrata Pal, Cyclotron Institute, Texas A&M University Strange Particle
Higgs vacuum stability and inflationary dynamics after BICEP2 and PLANCK dust polarisation data
Bhattacharya, Kaushik; Chakrabortty, Joydeep; Das, Suratna; Mondal, Tanmoy E-mail: joydeep@iitk.ac.in E-mail: tanmoym@prl.res.in
2014-12-01
If the recent detection of B-mode polarization of the Cosmic Microwave Background by BICEP2 observations, withstand the test of time after the release of recent PLANCK dust polarisation data, then it would surprisingly put the inflationary scale near Grand Unification scale if one considers single-field inflationary models. On the other hand, Large Hadron Collider has observed the elusive Higgs particle whose presently observed mass can lead to electroweak vacuum instability at high scale (?O(10{sup 10}) GeV). In this article, we seek for a simple particle physics model which can simultaneously keep the vacuum of the theory stable and yield high-scale inflation successfully. To serve our purpose, we extend the Standard Model of particle physics with a U(1){sub B-L} gauged symmetry which spontaneously breaks down just above the inflationary scale. Such a scenario provides a constrained parameter space where both the issues of vacuum stability and high-scale inflation can be successfully accommodated. The threshold effect on the Higgs quartic coupling due to the presence of the heavy inflaton field plays an important role in keeping the electroweak vacuum stable. Furthermore, this scenario is also capable of reheating the universe at the end of inflation. Though the issues of Dark Matter and Dark Energy, which dominate the late-time evolution of our universe, cannot be addressed within this framework, this model successfully describes the early universe dynamics according to the Big Bang model.
Constraining models of f(R) gravity with Planck and WiggleZ power spectrum data
Dossett, Jason; Parkinson, David; Hu, Bin E-mail: hu@lorentz.leidenuniv.nl
2014-03-01
In order to explain cosmic acceleration without invoking ''dark'' physics, we consider f(R) modified gravity models, which replace the standard Einstein-Hilbert action in General Relativity with a higher derivative theory. We use data from the WiggleZ Dark Energy survey to probe the formation of structure on large scales which can place tight constraints on these models. We combine the large-scale structure data with measurements of the cosmic microwave background from the Planck surveyor. After parameterizing the modification of the action using the Compton wavelength parameter B{sub 0}, we constrain this parameter using ISiTGR, assuming an initial non-informative log prior probability distribution of this cross-over scale. We find that the addition of the WiggleZ power spectrum provides the tightest constraints to date on B{sub 0} by an order of magnitude, giving log{sub 10}(B{sub 0}) < ?4.07 at 95% confidence limit. Finally, we test whether the effect of adding the lensing amplitude A{sub Lens} and the sum of the neutrino mass ?m{sub ?} is able to reconcile current tensions present in these parameters, but find f(R) gravity an inadequate explanation.
The Knotted Sky I: Planck constraints on the primordial power spectrum
Aslanyan, Grigor; Price, Layne C.; Easther, Richard; Abazajian, Kevork N. E-mail: lpri691@aucklanduni.ac.nz E-mail: r.easther@auckland.ac.nz
2014-08-01
Using the temperature data from Planck we search for departures from a power-law primordial power spectrum, employing Bayesian model-selection and posterior probabilities. We parametrize the spectrum with n knots located at arbitrary values of logk, with both linear and cubic splines. This formulation recovers both slow modulations and sharp transitions in the primordial spectrum. The power spectrum is well-fit by a featureless, power-law at wavenumbers k>10{sup -3} Mpc{sup -1}. A modulated primordial spectrum yields a better fit relative to ΛCDM at large scales, but there is no strong evidence for a departure from a power-law spectrum. Moreover, using simulated maps we show that a local feature at k ∼ 10{sup -3} Mpc{sup -1} can mimic the suppression of large-scale power. With multi-knot spectra we see only small changes in the posterior distributions for the other free parameters in the standard ΛCDM universe. Lastly, we investigate whether the hemispherical power asymmetry is explained by independent features in the primordial power spectrum in each ecliptic hemisphere, but find no significant differences between them.
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Financial Institution Lending Programs
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Financial institution loans for clean energy projects are originated and serviced through an entity other than the government, typically banks. In this case, a state or local government is not the...
Alex King
2013-06-05
Ames Laboratory Director Alex King talks about the goals of the Critical Materials Institute in diversifying the supply of critical materials, developing substitute materials, developing tools and techniques for recycling critical materials, and forecasting materials needs to avoid future shortages.
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and CEO of the New England Fuel Institute Before the U.S. Department of Energy and the Quadrennial Energy Review Task Force Public Hearing on "New England Regional ...
UNCLASSIFIED Institute for Materials ...
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PSI: the X-ray free electron laser SwissFEL and its future experimental capabilities. Biography: Prof. Dr. Jol Mesot is, since 2008, director of the Paul Scherrer Institute...
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Overview Dr. Ralf Rapp meets with his research group. At the Institute we focus on conducting basic research, educating students in accelerator-based science and technology, and providing technical capabilities for a wide variety of applications in space science, materials science, analytical procedures and nuclear medicine. Approximately 100 Institute members - scientists, engineers, technicians, support staff, graduate students and undergraduate students - are involved in these programs.
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Resources The Critical Materials Institute offers connections to resources, including: List of resources U.S. Rare Earth Magnet Patents Table Government agency contacts CMI unique facilities CMI recent presentations Photographs via Flick'r: Critical Materials Institute, The Ames Laboratory Videos from The Ames Laboratory Webinars from Colorado School of Mines To offer comments on the CMI website or to ask questions, please contact us via e-mail at CMIdirector@ameslab.gov or call 515-296-4500.
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Site Map Cyclotron Institute About K500 Beam Schedule Recent News Seminars and Colloquia Cyclotron Institute Safety (limited access) Radiation Effects Facility REU Program Research Heavy Ion Reactions Fundamental Interactions Nuclear Astrophysics Interactions of Highly Charged Ions With Matter Theoretical Nuclear Physics Nuclear Structure External Collaborations Publications Research Groups Facilities K500 Cyclotron ECR Ion Sources MARS Big Sol MDM Spectrometer NIMROD Precision On-Line Decay
Alexander, J. Iwan
2012-11-18
The vision of the Great Lakes Energy Institute is to enable the transition to advanced, sustainable energy generation, storage, distribution and utilization through coordinated research, development, and education. The Institute will place emphasis on translating leading edge research into next generation energy technology. The Institute’s research thrusts focus on coordinated research in decentralized power generation devices (e.g. fuel cells, wind turbines, solar photovoltaic devices), management of electrical power transmission and distribution, energy storage, and energy efficiency.
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INSTITUTE COLLOQUIA AND SEMINARS April 1, 2010-March 31, 2011 2010 May 11 Dr. J. J. Ressler, Lawrence Livermore National Laboratory, Livermore, California Surrogate Reactions for Nuclear Energy Application May 12 Professor Lie-Wen Chen, Institute of Nuclear, Particle Astronomy and Cosmology (INPAC) and Department of Physics, Shanghai Jiao Tong University, Shanghai, China Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions and Neutron Skin Thickness of Heavy Nuclei May 13 Professor A. R.
Max Tech and Beyond: Maximizing Appliance and Equipment Efficiency by Design
Desroches, Louis-Benoit; Garbesi, Karina
2011-07-20
It is well established that energy efficiency is most often the lowest cost approach to reducing national energy use and minimizing carbon emissions. National investments in energy efficiency to date have been highly cost-effective. The cumulative impacts (out to 2050) of residential energy efficiency standards are expected to have a benefit-to-cost ratio of 2.71:1. This project examined energy end-uses in the residential, commercial, and in some cases the industrial sectors. The scope is limited to appliances and equipment, and does not include building materials, building envelopes, and system designs. This scope is consistent with the scope of DOE's appliance standards program, although many products considered here are not currently subject to energy efficiency standards. How much energy could the United States save if the most efficient design options currently feasible were adopted universally? What design features could produce those savings? How would the savings from various technologies compare? With an eye toward identifying promising candidates and strategies for potential energy efficiency standards, the Max Tech and Beyond project aims to answer these questions. The analysis attempts to consolidate, in one document, the energy savings potential and design characteristics of best-on-market products, best-engineered products (i.e., hypothetical products produced using best-on-market components and technologies), and emerging technologies in research & development. As defined here, emerging technologies are fundamentally new and are as yet unproven in the market, although laboratory studies and/or emerging niche applications offer persuasive evidence of major energy-savings potential. The term 'max tech' is used to describe both best-engineered and emerging technologies (whichever appears to offer larger savings). Few best-on-market products currently qualify as max tech, since few apply all available best practices and components. The three primary
DOE - Office of Legacy Management -- Max Zuckerman and Sons Inc - MD 04
Office of Legacy Management (LM)
Inc - MD 04 FUSRAP Considered Sites Site: MAX ZUCKERMAN & SONS, INC. (MD.04 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Maryland Alloys Corporation MD.04-1 Location: 5245 Fairlawn Avenue , Baltimore , Maryland MD.04-2 Evaluation Year: 1994 MD.04-1 MD.04-3 Site Operations: Scrap metals broker that arranged purchases of materials for third party buyers. MD.04-2 MD.04-4 Site Disposition: Eliminated - Potential for contamination remote MD.04-3
Real-time and imaginary-time quantum hierarchal Fokker-Planck equations
Tanimura, Yoshitaka
2015-04-14
We consider a quantum mechanical system represented in phase space (referred to hereafter as “Wigner space”), coupled to a harmonic oscillator bath. We derive quantum hierarchal Fokker-Planck (QHFP) equations not only in real time but also in imaginary time, which represents an inverse temperature. This is an extension of a previous work, in which we studied a spin-boson system, to a Brownian system. It is shown that the QHFP in real time obtained from a correlated thermal equilibrium state of the total system possesses the same form as those obtained from a factorized initial state. A modified terminator for the hierarchal equations of motion is introduced to treat the non-Markovian case more efficiently. Using the imaginary-time QHFP, numerous thermodynamic quantities, including the free energy, entropy, internal energy, heat capacity, and susceptibility, can be evaluated for any potential. These equations allow us to treat non-Markovian, non-perturbative system-bath interactions at finite temperature. Through numerical integration of the real-time QHFP for a harmonic system, we obtain the equilibrium distributions, the auto-correlation function, and the first- and second-order response functions. These results are compared with analytically exact results for the same quantities. This provides a critical test of the formalism for a non-factorized thermal state and elucidates the roles of fluctuation, dissipation, non-Markovian effects, and system-bath coherence. Employing numerical solutions of the imaginary-time QHFP, we demonstrate the capability of this method to obtain thermodynamic quantities for any potential surface. It is shown that both types of QHFP equations can produce numerical results of any desired accuracy. The FORTRAN source codes that we developed, which allow for the treatment of Wigner space dynamics with any potential form (TanimuranFP15 and ImTanimuranFP15), are provided as the supplementary material.
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News August 25th, 2016 12:46 AM "Texas A&M Science - Labors of Lab." REU student Kassie Marble featured in TAMU College of Science Video July 23rd, 2016 12:46 AM The 2015-2016 Cyclotron Institute Annual Report, "Progress in Research", is now available. You may view/download the complete document and you may also browse individual articles. July 7th, 2015 1:01 AM The 2014-2015 Cyclotron Institute Annual Report, "Progress in Research", is now available. You may
Max Phase Materials And Coatings For High Temperature Heat Transfer Applications
Martinez-Rodriguez, M.; Garcia-Diaz, B.; Olson, L.; Fuentes, R.; Sindelar, R.
2015-10-19
Molten salts have been used as heat transfer fluids in a variety of applications within proposed Gen IV nuclear designs and in advanced power system such as Concentrating Solar Power (CSP). However, operating at elevated temperatures can cause corrosion in many materials. This work developed coating technologies for MAX phase materials on Haynes-230 and characterized the corrosion of the coatings in the presence of commercial MgCl_{2}-KCl molten salt. Cold spraying of Ti_{2}AlC and physical vapor deposition (PVD) of Ti_{2}AlC or Zr_{2}AlC were tested to determine the most effective form of coating MAX phases on structural substrates. Corrosion testing at 850°C for 100 hrs showed that 3.9 μm Ti2AlC by PVD was slightly protective while 117 μm Ti_{2}AlC by cold spray and 3.6 μm Zr_{2}AlC by PVD were completely protective. None of the tests showed decomposition of the coating (Ti or Zr) into the salt
Rahus Institute | Open Energy Information
article is a stub. You can help OpenEI by expanding it. Rahus Institute is a policy organization located in Martinez, California. References About Rahus Institute Retrieved...
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.
Strategies for Achieving Institutional Change
Broader source: Energy.gov [DOE]
Many strategies—including those derived from Institutional Change Principles–may be used to effect institutional change in support of energy and sustainability objectives.
Ecologic Institute | Open Energy Information
Institute Name: Ecologic Institute Address: Pfalzburger Strasse 4344 Place: Berlin, Germany Year Founded: 1995 Phone Number: +49 (30) 86880-0 Website: ecologic.eu...
Commitment Institutional Change Principle
Office of Energy Efficiency and Renewable Energy (EERE)
Commitment can be a crucial element that helps federal agencies inject and emphasize sustainability in their organizational culture. Institutions and people change when they have made definite commitments to change, especially when those commitments relate to future conditions. Research shows that explicit commitments improve the rate at which people adopt energy-efficient behaviors.
Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]
2003-04-09
The Policy ensures that the Department of Energy will use institutional controls in the management of resources, facilities and properties under its control, and in implementing its programmatic responsibilities. Certified 1-28-11. Superseded by Chg 1 (Admin Chg), dated 12-7-15.
Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]
2003-04-09
The Policy ensures that the Department of Energy will use institutional controls in the management of resources, facilities and properties under its control, and in implementing its programmatic responsibilities. Certified 1-28-11. Supersedes DOE P 454.1, dated 4-9-03.
Aghamousa, Amir; Shafieloo, Arman; Arjunwadkar, Mihir; Souradeep, Tarun E-mail: shafieloo@kasi.re.kr E-mail: tarun@iucaa.ernet.in
2015-02-01
Estimation of the angular power spectrum is one of the important steps in Cosmic Microwave Background (CMB) data analysis. Here, we present a nonparametric estimate of the temperature angular power spectrum for the Planck 2013 CMB data. The method implemented in this work is model-independent, and allows the data, rather than the model, to dictate the fit. Since one of the main targets of our analysis is to test the consistency of the ΛCDM model with Planck 2013 data, we use the nuisance parameters associated with the best-fit ΛCDM angular power spectrum to remove foreground contributions from the data at multipoles ℓ ≥50. We thus obtain a combined angular power spectrum data set together with the full covariance matrix, appropriately weighted over frequency channels. Our subsequent nonparametric analysis resolves six peaks (and five dips) up to ℓ ∼1850 in the temperature angular power spectrum. We present uncertainties in the peak/dip locations and heights at the 95% confidence level. We further show how these reflect the harmonicity of acoustic peaks, and can be used for acoustic scale estimation. Based on this nonparametric formalism, we found the best-fit ΛCDM model to be at 36% confidence distance from the center of the nonparametric confidence set—this is considerably larger than the confidence distance (9%) derived earlier from a similar analysis of the WMAP 7-year data. Another interesting result of our analysis is that at low multipoles, the Planck data do not suggest any upturn, contrary to the expectation based on the integrated Sachs-Wolfe contribution in the best-fit ΛCDM cosmology.
Poisson-Nernst-Planck-Fermi theory for modeling biological ion channels
Liu, Jinn-Liang; Eisenberg, Bob
2014-12-14
A Poisson-Nernst-Planck-Fermi (PNPF) theory is developed for studying ionic transport through biological ion channels. Our goal is to deal with the finite size of particle using a Fermi like distribution without calculating the forces between the particles, because they are both expensive and tricky to compute. We include the steric effect of ions and water molecules with nonuniform sizes and interstitial voids, the correlation effect of crowded ions with different valences, and the screening effect of water molecules in an inhomogeneous aqueous electrolyte. Including the finite volume of water and the voids between particles is an important new part of the theory presented here. Fermi like distributions of all particle species are derived from the volume exclusion of classical particles. Volume exclusion and the resulting saturation phenomena are especially important to describe the binding and permeation mechanisms of ions in a narrow channel pore. The Gibbs free energy of the Fermi distribution reduces to that of a Boltzmann distribution when these effects are not considered. The classical Gibbs entropy is extended to a new entropy form — called Gibbs-Fermi entropy — that describes mixing configurations of all finite size particles and voids in a thermodynamic system where microstates do not have equal probabilities. The PNPF model describes the dynamic flow of ions, water molecules, as well as voids with electric fields and protein charges. The model also provides a quantitative mean-field description of the charge/space competition mechanism of particles within the highly charged and crowded channel pore. The PNPF results are in good accord with experimental currents recorded in a 10{sup 8}-fold range of Ca{sup 2+} concentrations. The results illustrate the anomalous mole fraction effect, a signature of L-type calcium channels. Moreover, numerical results concerning water density, dielectric permittivity, void volume, and steric energy provide useful
A COMPREHENSIVE VIEW OF A STRONGLY LENSED PLANCK-ASSOCIATED SUBMILLIMETER GALAXY
Fu Hai; Cooray, A.; Jullo, E.; Bussmann, R. S.; Ivison, R. J.; Perez-Fournon, I.; Djorgovski, S. G.; Scoville, N.; Yan, L.; Riechers, D. A.; Bradford, M.; Aguirre, J.; Auld, R.; Baes, M.; Baker, A. J.; Cava, A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; and others
2012-07-10
We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 {mu}m flux density ({approx}300 mJy). It is the only high-redshift Planck detection in the 130 deg{sup 2} H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 {mu}m and CO(1{yields}0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over {approx}1.6 kpc, the dust in a compact ({approx}1 kpc) region {approx}3 kpc north of the stars, and the cold molecular gas in an extended ({approx}7 kpc) disk {approx}5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by {approx}17, {approx}8, and {approx}7 times, respectively, by four lensing galaxies at z {approx} 1. Intrinsically, the lensed galaxy is a warm (T{sub dust} {approx} 40-65 K), hyper-luminous (L{sub IR} {approx} 1.7 Multiplication-Sign 10{sup 13} L{sub Sun }; star formation rate (SFR) {approx}2000 M{sub Sun} yr{sup -1}), gas-rich (M{sub gas}/M{sub baryon} {approx} 70%), young (M{sub stellar}/SFR {approx} 20 Myr), and short-lived (M{sub gas}/SFR {approx} 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.
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(NEI) Summit Presentation University-Industry- Laboratory Partnerships: Gauging Effectiveness Douglas Kothe, CASL Director Oak Ridge National Laboratory February 26, 2014 CASL-U-2014-0355-000 CASL-U-2014-0355-000 University-Industry-Laboratory Partnerships Gauging Effectiveness CASL: The Consortium for Advanced Simulation of Light Water Reactors A DOE Energy Innovation Hub Douglas B. Kothe Oak Ridge National Laboratory Director, CASL 9 th Nuclear Energy R&D Summit Nuclear Energy Institute
Publications - Cyclotron Institute
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Publications "Progress in Research", Cyclotron Institute Annual Reports View individual articles: 2016 / 2015 / 2014 / 2013 / 2012 / 2011 / 2010 / 2009 / 2008 / 2007 / 2006 / 2005 / 2004 / 2003 / 2002 / 2001 / 2000 / 1999 Download complete documents: 2016 / 2015 / 2014 / 2013 / 2012 / 2011 / 2010 / 2009 / 2008 / 2007 / 2006 / 2005 / 2004 / 2003 List of Papers Published by Year 2012 / 2011 / 2010 / 2009 / 2008 / 2007/ 2006 / 2005 / 2004 / 2003 / 2002 / 2001 / 2000 / 1999 / 1998 / 1997 /
Research - Cyclotron Institute
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Overview Viewing gamma ray spectra. The Institute research program focuses on the atomic nucleus, a many-body system of strongly interacting constituents bound together by the strongest forces known in nature. The properties investigated often can be described in terms of the motions of single nucleons (neutrons and protons), the correlated motions of several nucleons, and the collective motions of many nucleons. On a finer scale, they can be understood in terms of the degrees of freedom of
Research | Critical Materials Institute
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Research Four Research Thrusts organizational chart of four research thrusts (A click on the org chart image will lead to a pdf version that includes hotlinks for the e-mail addresses for leaders.) CMI has more than 30 projects focused in four areas. Project titles are available in a table, which can be sorted by project leader, location of project leader, project title or project number. CMI research is conducted at partner institutions, including national laboratories, universities and
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SRF Institute Jefferson Lab is recognized as a world leader in accelerator science. This expertise comes from the planning, building, maintaining and operating of the Continuous Electron Beam Accelerator Facility (CEBAF) - the lab's particle accelerator. CEBAF is based on superconducting radiofrequency (SRF) technology and produces a stream of charged electrons that scientists use to probe the nucleus of the atom. CEBAF was the first large-scale application of SRF technology in the U.S., and it
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Contact Website Manager Bruce Hyman Email: hyman@comp.tamu.edu Mailing Address Cyclotron Institute Texas A&M University 3366 TAMU College Station, TX, 77843-3366 Campus Location Luedecke Building / Building #434 Campus Map Google Map Phone Number 979-845-1411 Fax Number 979-845-1899 Directory Graduate Faculty Full Directory For Information about Graduate Studies Contact: Professor Che Ming Ko Email: ko@comp.tamu.edu For Potential Use of Our Facility Contact: Professor Sherry J. Yennello
INSTITUTE COLLOQUIA AND SEMINARS
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1-March 31, 2002 2001 April 10 Dr. Massimo Di Toro, LNS/INFN and the University of Catania, Italy Isospin Effects on Nuclear Dynamics April 12 Dr. C. Lewis, U.S. Environmental Protection Agency, Research Triangle, North Carolina Air Pollution Research Using Radiocarbon Measurements April 17 Professor Olga Kocharovskaya, Department of Physics, Texas A&M University, College Station, Texas Laser Control of Mossbauer Nuclear Transitions May 1 Dr. Bency John, Cyclotron Institute, Texas A&M
INSTITUTE COLLOQUIA AND SEMINARS
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6-March 31, 2007 2006 April 6 Dr. Jamal Jalilian-Marian, Institute for Nuclear Theory, University of Washington, Seattle, Washington An Introduction to Particle Production in High Energy Nuclear Collisions April 7 Professor Taka Kajino, National Astronomical Observatory, University of Tokyo, Tokyo, Japan A Frontier of Nuclear Astrophysics: Big-Bang Cosmology and Supernova Nucleosynthesis April 19 Dr. Anna Stasto, Brookhaven National Laboratory, Upton, New York High Energy Limit and Parton
INSTITUTE COLLOQUIA AND SEMINARS
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7-March 31, 2008 2007 April 5 Dr. Nigel Orr, Laboratoire de Physique Corpusculaire, Universite de Caen Basse-Normandie, France Probing Nuclear Structure Far from Stability: from Breakup to Knockout April 10 Dr. Lie-wen Chen, Institute of Theoretical Physics, Shanghai Jiao Tong University, Shanghai, China Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions Induced by Neutron- Rich Nuclei April 11 Dr. Nigel Orr, Laboratoire de Physique Corpusculaire, Universite de Caen Basse-Normandie,
INSTITUTE COLLOQUIA AND SEMINARS
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09-March 31, 2010 2009 April 17 Professor Jian-Wei Qiu, Department of Physics and Astronomy, Iowa State University, Ames, Iowa and Brookhaven National Laboratory, Upton, New York QCD and High Energy Nuclear Collisions April 21 Dr. Peter Levai, KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary Can We Find Quark-Gluon Plasma in pp Collision at LHC? April 28 Professor Wolfgang Mittig, NSCL, Michigan State University, East Lansing, Michigan Nuclear Power and Global Energy
Boride-based nano-laminates with MAX-phase-like behaviour
Telle, Rainer . E-mail: telle@ghi.rwth-aachen.de; Momozawa, Ai; Music, Denis; Schneider, Jochen M.
2006-09-15
MAX-phases being usually composed of transition metals, group A elements and carbon/nitrogen are considered interesting materials for many applications because of their tremendous bulk modulus, 'reversible' plasticity, and machinability. This is mainly due to their unique kind of bonding comprising covalent, ionic as well as metallic bonds providing 'easy' planes of rupture and deformability due to the layered crystal structures. In transition metal boride systems, similar types of bonding are available. In particular the W{sub 2}B{sub 5}-structure type and its stacking variations allow the synthesis of strongly layered crystal structures exhibiting unique delamination phenomena. The paper presents ab initio calculations showing the similarities of bonding between the ternary carbides and the corresponding ternary or quaternary borides. Formation of boride-based nano-laminates from auxiliary liquid phases, from the melt as well as during sintering and precipitation from supersaturated solid solutions will be discussed by means of SEM and TEM studies. The role of impurities weakening the interlayer bonding will be addressed in particular. The pronounced cleavage parallel to the basal plane gives rise for crack deflection and pull-out mechanisms if the laminates are dispersed in brittle matrices such as boron carbide, silicon carbide or other transition metal borides. - Graphical abstract: Some transition metal borides crystallise in a layered structure of alternating stacks of metal and boron atoms giving rise for strongly anisotropic properties. Their preferred cleavage parallel and the deformability perpendicular to the basal plan are similar to the peculiar mechanical behaviour recently described for MAX-phases. Ab initio calculations of the crystal structure prove the weak bonds between the layers for a variety of borides which can be used to reinforce ceramic materials on a nano-scale level.
Ethiopian Development Research Institute | Open Energy Information
Ethiopian Development Research Institute Jump to: navigation, search Logo: Ethiopian Development Research Institute Name: Ethiopian Development Research Institute Address: Ethiopia...
Utilization Technology Institute | Open Energy Information
Utilization Technology Institute Jump to: navigation, search Name: Utilization Technology Institute Place: Des Plaines, IL References: Utilization Technology Institute1...
CMI Social Media | Critical Materials Institute
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Social Media Facebook: Critical Materials Institute Twitter: CMI_hub LinkedIn: Critical Materials Institute Flickr: Critical Materials Institute
An implicit energy-conservative 2D Fokker-Planck algorithm -- 2. Jacobian-free Newton-Krylov solver
Chacon, L.; Barnes, D.C.; Knoll, D.A.; Miley, G.H.
2000-01-20
Energy-conservative implicit integration schemes for the Fokker-Planck transport equation in multidimensional geometries require inverting a dense, non-symmetric matrix (Jacobian), which is very expensive to store and solve using standard solvers. However, these limitations can be overcome with Newton-Krylov iterative techniques, since they can be implemented Jacobian-free (the Jacobian matrix from Newton's algorithm is never formed nor stored to proceed with the iteration), and their convergence can be accelerated by preconditioning the original problem. In this document, the efficient numerical implementation of an implicit energy-conservative scheme for multidimensional Fokker-Planck problems using multigrid-preconditioned Krylov methods is discussed. Results show that multigrid preconditioning is very effective in speeding convergence and decreasing CPU requirements, particularly in fine meshes. The solver is demonstrated on grids up to 128 x 128 points in a 2D cylindrical velocity space ({upsilon}{sub r}, {upsilon}{sub p}) with implicit time steps of the order of the collisional time scale of the problem, {tau}. The method preserves particles exactly, and energy conservation is improved over alternative approaches, particularly in coarse meshes. Typical errors in the total energy over a time period of 10{tau} remain below a percent.
Massachusetts Institute of Technology
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05/2010 Teppei Katori, MIT 1 Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology U-Maryland Nuclear/HEP seminar, College Park, October, 5, 2010 MiniBooNE, a neutrino oscillation experiment at Fermilab 10/05/2010 Teppei Katori, MIT 2 Outline 1. Introduction 2. Neutrino beam 3. Events in the detector 4. Cross section model 5. Oscillation analysis and result 6. New Low energy excess result 7. Anti-neutrino oscillation result 8. Neutrino disappearance result 9.
LIG - Facilities - Cyclotron Institute
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Light Ion Guide Light Ion Guide. Texas A&M University is currently configuring a scheme for the production of radioactive-ion beams that incorporates a light-ion guide (LIG) coupled with an ECRIS constructed for charge-boosting (CB-ECRIS). This scheme is part of an upgrade to the Cyclotron Institute and is intended to produce radioactive beams suitable for injection into the K500 superconducting cyclotron. The Light-Ion Guide (LIG) will produce radioactive species mainly from (p,n)
Cyclotron Institute REU Program
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"Texas A&M Science - Labors of Lab." REU student Kassie Marble featured in TAMU College of Science Video The Texas A&M Cyclotron Institute, with support from the National Science Foundation, serves as a Research Experiences for Undergraduates site during the summer of each year. Alysssa Dibidad in the K150 control room. This REU site focuses on research in nuclear and particle science. Students will have the opportunity to work closely with internationally renowned scientists
INSTITUTE COLLOQUIA AND SEMINARS
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4-March 31, 2005 2004 April 8 Dr. Jeffrey W. Martin, Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California Ultracold Neutrons April 20 Professor J. W. Watson, Department of Physics, Kent State University, Kent, Ohio Short-range Correlations in Nuclei from (p,2p+n) and (e,e'p+N) Measurements May 10 Mr. Sean Liddick, NSCL- Michigan State University, East Lansing, Michigan The Evolution of Shell Structure in the A~60 Mass Region May 25 Dr. Juha Ärje, Department of
Ocean Carbon Cycle Models from the Carbon Dioxide Information Analysis Center (CDIAC)
DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]
The following Ocean Carbon Cycle models and modeling results are available from CDIAC: • CSIRO/Matear Data [Model simulation of climate change from 1880 till 2100 (Matear and Hirst 2003, GBC) • Lequere Data, Model Results • McKinley MITgcm offline biogeochemical model - posted May 2004 • McKinley MITgcm offline biogeochemical model - posted December 2004 • NCOM-Pacific-Biogeochemical Modeling Results from Fei Chai • ROMS-Pacific-Biogeochemical Modeling Results from Fei CHai • WHOI/NCAR/Irvine Eco-BGC (Doney, Moore, Lindsay, and Lima) - Posted May 2005 • Max-Planck-Institut f?r Biogeochemie (Lequere, Buitenhuis) Modeling Results • Max-Planck-Institut f?r Biogeochemie (Lequere, Buitenhuis) Modeling Results - Posted March 2005 • Jim Christian model output for (a) Climatologies of T, S, PO4 at 50 m depth intervals; (b) SST, SSS, MLD, pCO2, CO2 flux from 1990-2003, and (c) climatological surface horizontal velocity • Max-Planck-Institut f?r Biogeochemie (Lequere, Buitenhuis) Modeling Results • Deutsch (UW) model output results for Oxygen variability in the North Pacific • Pacific data-model intercomparison from Patrick Wetzel (Max Planck Institute for Meteorology, Germany)
Cyclotron Institute Upgrade Project
Clark, Henry; Yennello, Sherry; Tribble, Robert
2014-08-26
The Cyclotron Institute at Texas A&M University has upgraded its accelerator facilities to extend research capabilities with both stable and radioactive beams. The upgrade is divided into three major tasks: (1) re-commission the K-150 (88”) cyclotron, couple it to existing beam lines to provide intense stable beams into the K-500 experimental areas and use it as a driver to produce radioactive beams; (2) develop light ion and heavy ion guides for stopping radioactive ions created with the K-150 beams; and (3) transport 1+ ions from the ion guides into a charge-breeding electron-cyclotron-resonance ion source (CB-ECR) to produce highly-charged radioactive ions for acceleration in the K-500 cyclotron. When completed, the upgraded facility will provide high-quality re-accelerated secondary beams in a unique energy range in the world.
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Office of Scientific and Technical Information (OSTI)
... Paul ; Glover, S.C.O. ; ZAH, Heidelberg ; Greif, T.H. ; Garching, Max Planck Inst. ... Swift-BAT Cappelluti, N. ; Garching, Max Planck Inst., MPE ; Ajello, M. ; SLAC KIPAC, ...
The 60-month all-sky BAT Survey of AGN and the Anisotropy of...
Office of Scientific and Technical Information (OSTI)
Garching, Max Planck Inst., MPE ; Madejski, G.M. ; KIPAC, Menlo Park ; Gehrels, N. ; NASA, Goddard ; Burlon, D. ; Garching, Max Planck Inst., MPE Publication Date: 2012-04-02...
Integrative Bioengineering Institute
Eddington, David; Magin,L,Richard; Hetling, John; Cho, Michael
2009-01-09
Microfabrication enables many exciting experimental possibilities for medicine and biology that are not attainable through traditional methods. However, in order for microfabricated devices to have an impact they must not only provide a robust solution to a current unmet need, but also be simple enough to seamlessly integrate into standard protocols. Broad dissemination of bioMEMS has been stymied by the common aim of replacing established and well accepted protocols with equally or more complex devices, methods, or materials. The marriage of a complex, difficult to fabricate bioMEMS device with a highly variable biological system is rarely successful. Instead, the design philosophy of my lab aims to leverage a beneficial microscale phenomena (e.g. fast diffusion at the microscale) within a bioMEMS device and adapt to established methods (e.g. multiwell plate cell culture) and demonstrate a new paradigm for the field (adapt instead of replace). In order for the field of bioMEMS to mature beyond novel proof-of-concept demonstrations, researchers must focus on developing systems leveraging these phenomena and integrating into standard labs, which have largely been ignored. Towards this aim, the Integrative Bioengineering Institute has been established.
An In-Depth Look at Ground Source Heat Pumps and Other Electric Loads in Two GreenMax Homes
Puttagunta, Srikanth; Shapiro, Carl
2012-04-01
Building America research team Consortium for Advanced Residential Buildings (CARB) partnered with WPPI Energy to answer key research questions on in-field performance of ground-source heat pumps and lighting, appliance, and miscellaneous loads (LAMELs) through extensive field monitoring at two WPPI GreenMax demonstration homes in Wisconsin. These two test home evaluations provided valuable data on the true in-field performance of various building mechanical systems and LAMELs.
Los Alamos National Laboratory Institutes
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Los Alamos National Laboratory Institutes The National Security Education Center has formed several institutes, each with a partner university or consortia of universities. The formation of these institutes serves the need for LANL to recruit new staff and provide educational opportunities that will enhance retention at the Laboratory. This is accomplished by: Developing long-term collaborative relationships with universities whose research interests are important to the Laboratory.
Izabela Stroe: Worcester Polytechnic Institute
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Izabela Stroe: Worcester Polytechnic Institute Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Izabela Stroe: Worcester Polytechnic Institute Former postdoc, now collaborator November 1, 2014 Izabela Stroe Izabela Stroe Contact Linda Anderman Email Izabela Stroe Izabela Stroe now at Worcester Polytechnic Institute Izabela Stroe's history with the Lab dates back to 2001 and over the years she's been a summer student,
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THE EUFAR-FP6 JRA: Airborne Aerosol Reference Pod The AARP project is conducted by 7 research institutions representing 5 countries: Leader : University of Manchester (UK) : Hugh Coe Météo-France, CNRM (FR) : Thierry Bourrianne, Laurent Gomes Enviscope GmbH (DE) : Rolf Maser Stockholm University (SE) : Radovan Krejci Max-Planck-Institute for Chemistry (DE) : Joachim Curtius National University of Ireland, Galway (IE) : Regis Dupuy Leibniz-Institut for Tropospheric Research (DE): Markus Hermann
Atlanta Community Leaders’ Institute Conference
Broader source: Energy.gov [DOE]
The Atlanta Community Leaders Institute (CLI) held a conference on February 8 and 9 at Morehouse School of Medicine, in Atlanta, Georgia.
Bolton Community Leaders’ Institute Conference
Broader source: Energy.gov [DOE]
The Bolton Community Leaders Institute (CLI) held a conference on February 22 and 23 at the Southeastern Community College in Whiteville, North Carolina.
Institutional Change Basics for Sustainability
Office of Energy Efficiency and Renewable Energy (EERE)
Institutional change integrates technology, policy, and behavior to make new sustainability practices and perspectives become a typical part of how an agency operates.
Continuous Change Institutional Change Principle
Office of Energy Efficiency and Renewable Energy (EERE)
ecause it takes time to establish institutional change, federal agencies need multiyear plans that continuously work to achieve, reinforce, and improve significant and persistent sustainability goals.
Research and Institutional Integrity Office
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about any of these ethics policies and related procedures, please contact Meredith Montgomery, Director of Institutional Assurance and Integrity, at 510-486-4453 or...
My Account | Critical Materials Institute
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My Account Primary tabs Log in(active tab) Request new password Username * Enter your Critical Materials Institute username. Password * Enter the password that accompanies your ...
PNNL: About PNNL - Institutional Partnerships
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we engage at the institutional level, inviting them to provide input into the Laboratory strategy. Joint Appointments To enable long term strategic collaborations with...
Form:Research Institution | Open Energy Information
Research Institution Jump to: navigation, search Add a Research or Development Institution Input your research or development institution name below to add to the registry. If your...
Low Carbon Research Institute | Open Energy Information
Research Institute Jump to: navigation, search Logo: Low Carbon Research Institute Name: Low Carbon Research Institute Address: King Edward VII Avenue CF10 3NB Place: Cardiff,...
Cornell Fuel Cell Institute | Open Energy Information
Cornell Fuel Cell Institute Jump to: navigation, search Name: Cornell Fuel Cell Institute Place: Ithaca, New York Zip: 14850 Product: The Cornell Fuel Cell Institute (CFCI)...
GHG Management Institute | Open Energy Information
GHG Management Institute Jump to: navigation, search Name: GHG Management Institute Address: Greenhouse Gas Management Institute 9215 View Avenue NW Seattle, WA USA 98117 Place:...
Hitachi Research Institute | Open Energy Information
Institute Jump to: navigation, search Name: Hitachi Research Institute Place: Tokyo, Japan Zip: 101-8010 Product: Hitachi Research Institute is the think tank of the Hitachi...
Rocky Mountain Institute | Open Energy Information
Rocky Mountain Institute Jump to: navigation, search Logo: Rocky Mountain Institute Name: Rocky Mountain Institute Address: 1820 Folsom Street Place: Boulder, Colorado Zip: 80302...
Industrial Technology Research Institute | Open Energy Information
Technology Research Institute Jump to: navigation, search Logo: Industrial Technology Research Institute Name: Industrial Technology Research Institute Address: Rm. 112, Bldg. 24,...
Sustainable Europe Research Institute | Open Energy Information
Europe Research Institute Jump to: navigation, search Logo: Sustainable Europe Research Institute Name: Sustainable Europe Research Institute Address: Garnisongasse 721 A -1090...
UC Berkeley- Energy Institute | Open Energy Information
Berkeley- Energy Institute Jump to: navigation, search Logo: UC Berkeley- Energy Institute Name: UC Berkeley- Energy Institute Address: 2547 Channing Way Place: Berkeley,...
Honda Research Institute | Open Energy Information
search Name: Honda Research Institute Place: Mountain View, California Sector: Biofuels, Solar Product: California-based research institute of Honda. The institute conducts...
Chervenak, Ann Louise
2013-12-19
The mission of the Earth System Grid Federation (ESGF) is to provide the worldwide climate-research community with access to the data, information, model codes, analysis tools, and intercomparison capabilities required to make sense of enormous climate data sets. Its specific goals are to (1) provide an easy-to-use and secure web-based data access environment for data sets; (2) add value to individual data sets by presenting them in the context of other data sets and tools for comparative analysis; (3) address the specific requirements of participating organizations with respect to bandwidth, access restrictions, and replication; (4) ensure that the data are readily accessible through the analysis and visualization tools used by the climate research community; and (5) transfer infrastructure advances to other domain areas. For the ESGF, the U.S. Department of Energy’s (DOE’s) Earth System Grid Center for Enabling Technologies (ESG-CET) team has led international development and delivered a production environment for managing and accessing ultra-scale climate data. This production environment includes multiple national and international climate projects (such as the Community Earth System Model and the Coupled Model Intercomparison Project), ocean model data (such as the Parallel Ocean Program), observation data (Atmospheric Radiation Measurement Best Estimate, Carbon Dioxide Information and Analysis Center, Atmospheric Infrared Sounder, etc.), and analysis and visualization tools, all serving a diverse user community. These data holdings and services are distributed across multiple ESG-CET sites (such as ANL, LANL, LBNL/NERSC, LLNL/PCMDI, NCAR, and ORNL) and at unfunded partner sites, such as the Australian National University National Computational Infrastructure, the British Atmospheric Data Centre, the National Oceanic and Atmospheric Administration Geophysical Fluid Dynamics Laboratory, the Max Planck Institute for Meteorology, the German Climate Computing
Determine Institutional Change Sustainability Goals
Office of Energy Efficiency and Renewable Energy (EERE)
The first step in the institutional change process is defining your federal agency's sustainability goals. That is, decide what outcomes are desired (or required) over what period of time. Behavioral, organizational, and institutional changes typically are means to achieve desired energy, resource, or greenhouse gas emission outcomes. They are not ends in and of themselves.