The non-explosive modes of hydrogen burning - A brief review

Details The non-explosive modes of hydrogen burning - A brief review The non-explosive modes of hydrogen burning - A brief review

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...40..310a&link_type=abstract

In: Inside the stars; Proceedings of the 137th IAU Colloquium, Univ. of Vienna, Austria, Apr. 13-18, 1992 (A93-53126 23-90), p.

Astronomy and Astrophysics

Astrophysics

6

Hydrogen, Stellar Evolution, Stellar Physics, Abundance, Aluminum, Carbon, Nitrogen, Nuclear Astrophysics, Oxygen, Solar Neutrinos

Scientific paper

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.

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