Type-II supernovae in 12-solar-mass and 15-solar-mass stars The equation of state and general relativity

Details Type-II supernovae in 12-solar-mass and 15-solar-mass stars The equation of state and general relativity Type-II supernovae in 12-solar-mass and 15-solar-mass stars The equation of state and general relativity

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55..126b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, July 1, 1985, p. 126-129.

Physics

213

Equations Of State, Relativity, Stellar Models, Supernovae, Explosions, Hydrodynamic Equations, Neutrons, Stellar Cores

Scientific paper

The authors present results of hydrodynamic calculations of iron-core collapse and subsequent shock propagation using the 12 M_sun; and 15 M_sun; initial models of Woosley and Weaver. A softening of the equation of state of neutron-rich nuclear matter at high density and the effects of general relativity play a crucial role in generating successful, prompt explosions. The energy of the explosion varies from (≡1 - 3)×1051ergs depending upon the degree of softness.

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