Research in nuclear astrophysics: Stellar collapse and supernovae. Continuation progress report, December 1, 1994--November 30, 1995

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Abstract
This progress report describes the nuclear astrophysics research activities in the Earth and Space Sciences Department at Stony Brook during the last year. The research focuses on three aspects of nuclear astrophysics: (1) the equation of state of hot, dense matter, (2) the origin of supernovae and neutron stars, (3) the early cooling epoch of neutron stars. Ongoing projects are first described individually, and are followed by a series of detailed reports, which summarize each project completed within the last year.

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