The stability of stellar structure in non-equilibrium thermodynamics III - The PPI reaction allowing for mass loss

Details The stability of stellar structure in non-equilibrium thermodynamics III - The PPI reaction allowing for mass loss The stability of stellar structure in non-equilibrium thermodynamics III - The PPI reaction allowing for mass loss

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4..191w&link_type=abstract

(Acta Astrophysica Sinica, vol. 4, no. 1, 3, 1984, p. 191-198) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Sept

Astronomy and Astrophysics

Astrophysics

2

Main Sequence Stars, Nonequilibrium Thermodynamics, Stellar Composition, Stellar Mass, Stellar Structure, Thermonuclear Reactions, Entropy, Inequalities, Mass Transfer, Stellar Evolution, Stellar Temperature, Systems Stability

Scientific paper

The present study examines the stability of solar-type stars whose
structure is determined by the PPI reaction according to the criterion
of excess entropy production of nonlinear nonequilibrium thermodynamics,
with allowance for mass loss in the reaction. The star is found to be
stable if the hydrogen-to-helium ratio satisfies a specified inequality.

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