Composition and adiabatic index of matter at high temperatures

Details Composition and adiabatic index of matter at high temperatures Composition and adiabatic index of matter at high temperatures

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..60..353b&link_type=abstract

Astrophysics and Space Science, vol. 60, no. 2, Feb. 1979, p. 353-365.

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Gravitational Collapse, Matter (Physics), Supernova Remnants, Adiabatic Conditions, Equations Of State, Nucleons, Particle Interactions, Relativistic Particles

Scientific paper

The equation of state and the adiabatic index of thermally dissociated matter composed of nucleons, electrons, positrons, neutrinos, antineutrinos and photons are calculated in the density and temperature ranges from about 10 to the 9th to 10 to the 13th g/cu cm and from about 2 x 10 to the 10th to 5 x 10 to the 11th K, respectively. The interaction between nucleons is explicitly included. This leads to a softening of the equation of state. The implications of the results for the problem of supernova collapse are discussed.

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