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

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995stin...9525343l&link_type=abstract

Continuation Progress Report, 1 Dec. 1994 - 30 Nov. 1995 State Univ. of New York, Stony Brook, NY. Dept. of Earth and Space Scie

Physics

Condensed Matter

Superconductivity

Cooling Flows (Astrophysics), Gravitational Collapse, Matter (Physics), Neutron Stars, Nuclear Astrophysics, Stellar Activity, Stellar Evolution, Supernovae, Energy Transfer, Equations Of State, Neutrinos, Phase Transformations, Superconductivity, Superfluidity

Scientific paper

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; and (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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