Branching of the PP chains

Details Branching of the PP chains Branching of the PP chains

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...325..476m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 325, Feb. 1, 1988, p. 476-479. NSERC-supported research.

Astronomy and Astrophysics

Astrophysics

1

Nuclear Fusion, Solar Neutrinos, Stellar Interiors, Abundance, Helium, Hydrogen, Stellar Evolution, Temperature Effects

Scientific paper

The branching of PP chains is discussed, and it is noted that for a given ratio Y/X of helium and hydrogen abundances by mass that the branching to PP III increases continuously as the temperature increases. It is found that for a given temperature there is a critical Y/X for which the branching to PP III is maximum. For higher values, the branching to PP III is shown to decrease. The critical value of X has been calculated as a function of temperature. The impact of the existence of this maximum on the evolution of the solar neutrino counting rate is considered.

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