Iron core collapse models of Type II supernovae
Conference
·
OSTI ID:6720556
Results of recent numerical, one-dimensional core collapse calculations for 10M/sub sun/, 15M/sub sun/ and 20M/sub sun/ population I stars are reviewed. The physics model is discussed, including recent improvements in the nuclear equations of state, and nuclear binding energies. None of the models produces prompt explosions as a direct result of core collapse and bounce.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 6720556
- Report Number(s):
- LA-UR-84-1937; CONF-8210111-4; ON: DE84013909
- Resource Relation:
- Conference: Numerical astrophysics meeting (in honor of Jim Wilson's 60th birthday), Urbana, IL, USA, 21 Oct 1982; Other Information: Portions are illegible in microfiche products
- Country of Publication:
- United States
- Language:
- English
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