PPT-Assessment of ENDF/B-VIII.0 and TENDL-2015 Evaluated Nuclear Data Libraries Using Stellar

Author : eliza | Published Date : 2023-10-26

Boris Pritychenko 1 1 National Nuclear Data Center Brookhaven National Laboratory Upton NY 119735000 USA Heavy Elements Production in a Neutron Star Merger Can we

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Assessment of ENDF/B-VIII.0 and TENDL-2015 Evaluated Nuclear Data Libraries Using Stellar: Transcript

Boris Pritychenko 1 1 National Nuclear Data Center Brookhaven National Laboratory Upton NY 119735000 USA Heavy Elements Production in a Neutron Star Merger Can we apply nuclear data libraries to address current astrophysical observations such as a multimessenger signal from the NGC 4993 galaxy . . atmospheres. a . very. . short. . introduction. Part I. Ewa Niemczura. Astronomical. . Institute. , . UWr. eniem@astro.uni.wroc.pl. Stellar. spectra. Stellar. spectra. One picture is worth 1000 words, but . Patricia . Sánchez-Blázquez. (UAM). Jairo. Mendez-Abreu (IAC). Sebastian F Sánchez (UNAM). Isabel Perez (UGR). Fabian Rosales-Ortega (UAM). And . the CALIFA collaboration. Resolved stellar . population. H.-W. Rix IMPRS Galaxies Course March 11, 2011. Goal:. Determine . n. *. (M. *. ,. t. age. ,[Fe. /H],. R. ). . for a population of galaxies. How many stars of what mass and metallicity . formed when and where in galaxies?. Giuseppina. . Battaglia. Instituto. de . Astrofisica. de Canarias, Tenerife. Credit. : ESO/. H.H.Heyer. Credit. : ESO/L. . Calçada. Karachentsev. et al. 2014. Individual . Red . Giant Branch . stars. 1. /28. Important for transits (see next slides).. . Transit depth = [ . R. planet. (. λ. ,t. ) / . R. star. (. λ,t. ) ]. 2. Not so important for eclipses because the eclipse is a simple difference, and the stellar variability typically is slower than the eclipse: . A first of its kind collaboration between:. Indiana Office of Community and Rural Affairs (OCRA). Indiana Housing and Community Development Authority (IHCDA). Indiana Department of Transportation (INDOT). JEFFREY HALL. LOWELL OBSERVATORY, FLAGSTAFF, AZ. Project Timeline. 1988 1992 1996 2000 2004 2008 2012 . Construction/early observing. Rebuild 1. Broad survey. Solar analog survey. Rebuild 2. A/D boundary. Ian Gauld. Marco Pigni. Reactor and Nuclear Systems Division. May 2, 2013. Nuclear decay data from an end-user perspective.. Evaluated decay data have major importance to areas of reactor safety and nuclear fuel cycle analysis. Dorothea Wiarda. William J. Marshall. Vladimir . Sobes. Friederike. . Bostelmann. Andrew Holcomb. Bradley T. Rearden. Outline. Covariance library creation. Differences between ENDF/B-VII.1 and ENDF/B-VIII.0. Mohamed Sawan. Tim . Bohm. U. Wisconsin-Madison. Fusion Neutronics Team. M. Sawan. 2. Revision to FENDL-2.0 (1995/96) . 71 . elements/isotopes. Working libraries prepared by IAEA/NDS, INDC(NDS)-467 (2004). These statements have not been evaluated by the Food and Drug Administration These products are not intended to diagnose treat cure or prevent any disease Always consult your doctor before taking any TRU . production and . radiotoxicity. ○. Rei Kimura, . Kenichi . Yoshioka, . Kouji Hiraiwa, . Shungo . Sakurai, . Satoshi Wada, . Tsukasa . Sugita. Toshiba Energy Systems & Solutions Corporation. of. FISPACT-II & General-Purpose Nuclear Data Libraries. M. Fleming, . J-Ch. Sublet, M. . . Gilbert,. J. Kopecky. 1. , A. Koning. 2. , D. Rochman. 3. 1. JUKO Research. 2. IAEA Nuclear Data Section. M. . Fleming, J-Ch. Sublet, D. Rochman. 1. , K-H. Schmidt. 2. UK Atomic Energy . Authority. 1. Paul . Scherrer. . Institut. 2. Centre Etudes . Nucl. é. aires. de Bordeaux . Gradignan. Technical Meeting on Fission Yields.

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