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The Non-Explosive Modes of Hydrogen Burning: A Brief Review

Published online by Cambridge University Press:  12 April 2016

Marcel Arnould  and
Nami Mowlavi
Marcel Arnould
Affiliation:
Institut d’Astronomie et d’AstrophysiqueUniversité Libre de Bruxelles, C.P. 165; Av. F.D. Roosevelt, 50 1050 Bruxelles, Belgium
Nami Mowlavi
Affiliation:
Institut d’Astronomie et d’AstrophysiqueUniversité Libre de Bruxelles, C.P. 165; Av. F.D. Roosevelt, 50 1050 Bruxelles, Belgium

Abstract

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The present status of our theoretical and experimental knowledge of the rates of hydrogen-burning reactions in hydrostatic stellar conditions is very briefly reviewed. Special emphasis is put on reactions of the proton-proton chain, CNO cycles, NeNa cycle and MgAl chain whose rates are still affected by uncertainties that can have an impact on predictions regarding astrophysical issues of interest. This concerns in particular the solar neutrino problem, or the nucleosynthesis accompanying the CNO, NeNa and MgAl chains of reactions, as it is revealed in particular by the first dredge-up episode. A brief discussion of the possibility of reducing the present rate uncertainties is presented.

Type
IV. Input physics and basic stellar data
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 310 - 323
Copyright
Copyright © Astronomical Society of the Pacific 1993

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