Effect of equation of state and shock energy loss on SN II explosions

Details Effect of equation of state and shock energy loss on SN II explosions Effect of equation of state and shock energy loss on SN II explosions

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acaps...5..171c&link_type=abstract

(Acta Astrophysica Sinica, vol. 5, no. 3-4, 1985, p. 171-179) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, Dec.

Physics

Nuclear Physics

Equations Of State, Gravitational Collapse, Shock Heating, Stellar Cores, Stellar Evolution, Supernovae, Adiabatic Conditions, Energy Dissipation, Hydrodynamic Equations, Nuclear Physics, Stellar Mass, Stellar Structure

Scientific paper

Consideration is given to the effect on the adiabatic gravitational collapse of stellar cores of large mass due to: (1) the use of different equations of state; and (2) the inclusion of energy loss of shock. It is found that different equations of state give very different central densities at rebounce and amplitudes of rebounce. When shock energy loss is not considered, all the equations discussed here will lead to explosions, but when it is considered, small amplitude rebounces will not do so.

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