Hydrostatic Instability in Very High Temperature Stars

Details Hydrostatic Instability in Very High Temperature Stars Hydrostatic Instability in Very High Temperature Stars

May 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969pthph..41.1211i&link_type=abstract

Progress of Theoretical Physics, Vol. 41, No. 5, pp. 1211-1216

Physics

1

Scientific paper

Calculating the adiabatic exponent γ ≡ (d log P / d log ρ)ad or the non-degenerate gas consisting of radiation, neutrinos, electron-pairs, muon-pairs, pions and nucleons, we investigate the condition of the hydrostatic instability in high temperature stars in the post-Newtonian approximation. It is found that the general relativistic effect plays a significant role for the hydrostatic stability condition of very high temperature stars.

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