Thermodynamics of a system of leptons, photons and interacting nucleons

Details Thermodynamics of a system of leptons, photons and interacting nucleons Thermodynamics of a system of leptons, photons and interacting nucleons

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..471a&link_type=abstract

Astrophysics and Space Science, vol. 69, no. 2, May 1980, p. 471-483.

Astronomy and Astrophysics

Astrophysics

1

Elementary Particle Interactions, Leptons, Nucleons, Photons, Supernovae, Thermodynamic Properties, Equations Of State, Neutron Stars, Particle Energy, Particle Flux Density, Quantum Mechanics, Temperature Effects

Scientific paper

The thermodynamics of matter composed of interacting nucleons with an admixture of leptons and photons is investigated in the density-temperature region relevant to the problem of supernova explosion. A quantum mechanical calculation is carried out using Skyrme effective interaction between nucleons. The equation of state is shown to soften below the nuclear density and suddenly stiffen in the transnuclear density region, a condition which is suitable for producing a strong bounce shock that is needed for effective supernova explosion and leaving a remnant neutron star behind.

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