Physics of supernovae
Description:
Presupernova models of massive stars are presented and their explosion by ''delayed neutrino transport'' examined. A new form of long duration Type II supernova model is also explored based upon repeated encounter with the electron-positron pair instability in stars heavier than about 60 Msub solar. Carbon deflagration in white dwarfs is discussed as the probable explanation of Type I supernovae and special attention is paid to the physical processes whereby a nuclear flame propagates through d…
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Date:
December 13, 1985
Creator:
Woosley, S. E. & Weaver, T. A.
Item Type:
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Partner:
UNT Libraries Government Documents Department