Theoretical and experimental data are reviewed as they relate to stellar n-capture nucleosynthesis and therefore to constraints on advanced stellar evolution. Attention is given to the mechanisms of n-captures occuring near the valley of beta-stability or with very strong neutron fluxes under dynamical conditions. High-resolution spectroscopic data and advances in nuclear theory are shown to be useful for constraining the explosive stages of stellar evolution as well as the age of the universe.

Understanding n-capture nucleosynthesis - A test for stellar and galactic evolution

BUSSO, Maurizio Maria;
1992

Abstract

Theoretical and experimental data are reviewed as they relate to stellar n-capture nucleosynthesis and therefore to constraints on advanced stellar evolution. Attention is given to the mechanisms of n-captures occuring near the valley of beta-stability or with very strong neutron fluxes under dynamical conditions. High-resolution spectroscopic data and advances in nuclear theory are shown to be useful for constraining the explosive stages of stellar evolution as well as the age of the universe.
1992
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11391/1064048
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