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A Brief Review of the s-process of Nucleosynthesis

Published online by Cambridge University Press:  19 July 2016

M. Arnould
M. Arnould*
Affiliation:
Institut d'Astronomie et d'Astrophysique - CP 165 Université Libre de Bruxelles Av. F.D. Roosevelt 50, B-1050 Bruxelles Belgium

Abstract

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A brief overview is presented of the s-process of nucleosynthesis. Special emphasis is put on some of its nuclear physics aspects, and in particular on the uncertainties that still affect the rates of the 13C(α,n)16O and 22Ne(α,n)25Mg neutron producing reactions. We also briefly review the so-called “classical” s-process model, and put it in perspective with recent s-process calculations conducted in the framework of detailed models for massive stars or for thermally pulsing AGB stars.

Type
The AGB
Information
Symposium - International Astronomical Union , Volume 145: Evolution of Stars: The Photospheric Abundance Connection , 1991 , pp. 287 - 297
Copyright
Copyright © Kluwer 1991 

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