Mean-field calculations of the equation of state of supernova matter II

Details Mean-field calculations of the equation of state of supernova matter II Mean-field calculations of the equation of state of supernova matter II

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...112..268b&link_type=abstract

Astronomy and Astrophysics, vol. 112, no. 2, Aug. 1982, p. 268-272.

Astronomy and Astrophysics

Astrophysics

32

Equations Of State, Nucleon-Nucleon Interactions, Stellar Mass, Supernovae, Adiabatic Conditions, Baryons, Beta Factor, Electron Capture, Elementary Particle Interactions, Hartree Approximation, Leptons, Neutrinos, Nuclear Interactions

Scientific paper

Further results of Hartree-Fock calculations for the equation of state of hot dense matter are presented. The contribution of neutrinos is included, and matter in beta equilibrium with a value of the lepton fraction Yl equals 0.35 suggested by the latest estimates of electron capture is considered. The adiabat S equals 1 per baryon in the region just below nuclear matter density is discussed. A detailed investigation of the phase transition from nuclei to bubbles along this adiabat is carried out.

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