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Neutron capture measurements on 62Ni, 63Ni and 197Au and their relevance for stellar nucleosynthesis

Neutron capture reactions in stars are responsible for forming about 99% of the elemental abundances heavier than Fe. Two processes contribute about equally to the overall abundance pattern: the slow neutron capture process (s process) where neutron densities are small and therefore radioactive deca...

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Detalles Bibliográficos
Autor principal:	Lederer, Claudia
Lenguaje:	eng
Publicado:	2012
Materias:	Nuclear Physics - Experiment
Acceso en línea:	http://cds.cern.ch/record/1474071

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