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Universality of the p process

The solar abundances provide a concept of universality that the abundance ratios of the p-nucleus to the s-nucleus with the same atomic number are almost constant with the wide region for materials produced by individual stellar nucleosynthesis episode. We study this universality using g -process ca...

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Detalles Bibliográficos
Autores principales: Hayakawa, T, Iwamoto, N, Kajino, T, Shizuma, T, Umeda, H, Nomoto, K
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:http://cds.cern.ch/record/1099458
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author Hayakawa, T
Iwamoto, N
Kajino, T
Shizuma, T
Umeda, H
Nomoto, K
author_facet Hayakawa, T
Iwamoto, N
Kajino, T
Shizuma, T
Umeda, H
Nomoto, K
author_sort Hayakawa, T
collection CERN
description The solar abundances provide a concept of universality that the abundance ratios of the p-nucleus to the s-nucleus with the same atomic number are almost constant with the wide region for materials produced by individual stellar nucleosynthesis episode. We study this universality using g -process calculations with core-collapse supernova explosions under various conditions. The calculated results show that the g -process under the various conditions can occur but the ratios are almost constant with the wide region independent of the conditions. The shift of g -process layers, weak s-process and the b -decay after the g -process contribute to the manifestation of the universality.
id cern-1099458
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2006
record_format invenio
spelling cern-10994582019-09-30T06:29:59Zhttp://cds.cern.ch/record/1099458engHayakawa, TIwamoto, NKajino, TShizuma, TUmeda, HNomoto, KUniversality of the p processAstrophysics and AstronomyThe solar abundances provide a concept of universality that the abundance ratios of the p-nucleus to the s-nucleus with the same atomic number are almost constant with the wide region for materials produced by individual stellar nucleosynthesis episode. We study this universality using g -process calculations with core-collapse supernova explosions under various conditions. The calculated results show that the g -process under the various conditions can occur but the ratios are almost constant with the wide region independent of the conditions. The shift of g -process layers, weak s-process and the b -decay after the g -process contribute to the manifestation of the universality.oai:cds.cern.ch:10994582006
spellingShingle Astrophysics and Astronomy
Hayakawa, T
Iwamoto, N
Kajino, T
Shizuma, T
Umeda, H
Nomoto, K
Universality of the p process
title Universality of the p process
title_full Universality of the p process
title_fullStr Universality of the p process
title_full_unstemmed Universality of the p process
title_short Universality of the p process
title_sort universality of the p process
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/1099458
work_keys_str_mv AT hayakawat universalityofthepprocess
AT iwamoton universalityofthepprocess
AT kajinot universalityofthepprocess
AT shizumat universalityofthepprocess
AT umedah universalityofthepprocess
AT nomotok universalityofthepprocess