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Supernovae and the nuclear equation of state at high densities
Authors:E. Baron  
Affiliation:

a Physics Dept., SUNY at Stony Brook, Stony Brook, New York 11794, USA

b Physics Dept., Brookhaven National Laboratory, Upton, New York 11973, USA

c Physics Dept., SUNY at Stony Brook, Stony Brook, New York 11794, USA

d Nordita, Copenhagen, Denmark

Physics Dept., Brookhaven National Laboratory, Upton, New York 11973, USA

Abstract:
An extensive study of the shock-explosive mechanism for generating type II supernovae is made. The nuclear high-density equation of state plays an important role, moderate softening of the equation of state leading to a considerable increase in shock strength. A definition of shock energy which can be used throughout the life of the shock is introduced.
Keywords:
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