Composition and equation of state of thermally dissociated matter

Details Composition and equation of state of thermally dissociated matter Composition and equation of state of thermally dissociated matter

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213..239v&link_type=abstract

Astrophysical Journal, Part 1, vol. 213, Apr. 1, 1977, p. 239-249. ERDA-supported research.

Astronomy and Astrophysics

Astrophysics

9

Chemical Composition, Equations Of State, Gravitational Collapse, Nuclear Reactions, Stellar Evolution, Thermal Dissociation, Electrons, Ideal Gas, Neutrinos, Nucleons, Photons, Relativity

Scientific paper

The composition and equation of state of a perfect gas of photons, electrons-photons, neutrinos, and nucleons is calculated under the assumption of either perfect neutrino transparency or some buildup of neutrino concentration in dense matter. The calculations are applicable to collapsing stars after thermal dissociation (temperatures above 10 billion K) and before nuclear forces are important (densities below 10 to the 14th power g/cu cm).

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