Research in nuclear astrophysics: Stellar collapse and supernovae

Details Research in nuclear astrophysics: Stellar collapse and supernovae Research in nuclear astrophysics: Stellar collapse and supernovae

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981suny.rept.....m&link_type=abstract

Progress Report, 1 Dec. 1981 - 30 Nov. 1984 State Univ. of New York, Albany.

Physics

Nuclear Physics

Gravitational Collapse, Neutrino Beams, Nuclear Astrophysics, Nuclear Interactions, Nuclear Physics, Supernovae, Hydrodynamic Equations, Mathematical Models, Stellar Evolution, Variable Stars

Scientific paper

The implications of nuclear theory for the final collapse of massive stars is examined. The development of an appropriate nuclear equation of state and its implementation in hydrodynamics are studied. The influence of nuclear dissociation and neutrino emission on the formation and propagation of shocks are investigated. The long term evolution of collapsed stellar cores after the initial hydrodynamic bounce, neutrino production and emission in all phases are derived, and potential effects of pion condensation and neutrino instabilities are explored.

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