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

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8910778l&link_type=abstract

Annual Performance Report, 1 Dec. 1987 - 30 Nov. 1988 State Univ. of New York, Stony Brook. Dept. of Earth and Space Sciences.

Astronomy and Astrophysics

Astrophysics

Equations Of State, Neutron Stars, Nuclear Astrophysics, Stellar Evolution, Supernovae, Magnetic Moments, Neutrinos

Scientific paper

This annual performance report summarizes the activity in the nuclear astrophysics research program in the Earth and Space Scienes Department at Stony Brook. The central themes in the projects that comprise this program are supernovae, neutron star formation, and the equation of state of hot, dense metter. There is a close coupling between the physics of nuclear matter and weak interactions on the one hand, and supernovae and neutron stars on the other. The properties of nuclear matter might at present best be delineated by astrophysical considerations. We have been active in researching both the nuclear physics of the equation of state and the astrophysics of stellar collapse, neutrino emission, and neutron star formation.

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