Cargando…
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...
Autores principales: | , , , , , |
---|---|
Lenguaje: | eng |
Publicado: |
2006
|
Materias: | |
Acceso en línea: | http://cds.cern.ch/record/1099458 |
_version_ | 1780913970199134208 |
---|---|
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 |