Temperature and asymmetry dependence of nuclear incompressibility and supernova explosions

Details Temperature and asymmetry dependence of nuclear incompressibility and supernova explosions Temperature and asymmetry dependence of nuclear incompressibility and supernova explosions

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phr...242..165b&link_type=abstract

Physics Reports, Volume 242, Issue 1-3, p. 165-180.

Physics

43

Scientific paper

The properties of hot asymmetric nuclear matter are investigated in the framework of an extended Brueckner-Bethe-Goldstone theory, using the Paris nucleon-nucleon interaction. In particular, the asymmetry and temperature dependence of the incompressibility of nuclear matter are explored in connection with the models of type-II supernova explosions. The present calculations predict a strong decrease of the nuclear incompressibility coming from both the temperature and the asymmetry dependence. The nuclear equation of state (EOS) is calculated along an isentrope, and compared with the phenomenological nuclear EOS which has been commonly used in some hydrodynamical calculations of type-II supernova explosions.

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