作者: E. Baron , J. Cooperstein , S. Kahana
DOI: 10.1103/PHYSREVLETT.55.126
关键词: Shock wave 、 Physics 、 Nuclear matter 、 Theory of relativity 、 Equation of state 、 Type II supernova 、 Supernova 、 Gravitational collapse 、 Astrophysics 、 General relativity
摘要: We present results of hydrodynamic calculations iron core collapse and subsequent shock propagation using the 12M/sub c/irdot 15M/sub initial models Woosley Weaver. A softening equation state neutron-rich nuclear matter at high density effects general relativity play a crucial role in generating successful, prompt explosions. The energy explosion varies from (approx. 1 to 3) x 10/sup 51/ ergs depending upon degree softness.