Numerical Analysis of Standing Accretion Shock Instability with Neutrino Heating in Supernova Cores

We have numerically studied the instability of the spherically symmetric standing accretion shock wave against nonspherical perturbations. We have in mind the application to collapse-driven supernovae in the postbounce phase, where the prompt shock wave generated by core bounce is commonly stalled....

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Veröffentlicht in:The Astrophysical journal 2006-04, Vol.641 (2), p.1018-1028
Hauptverfasser: Ohnishi, Naofumi, Kotake, Kei, Yamada, Shoichi
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Sprache:eng
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