The Spherical Accretion Shock Instability in the Linear Regime [electronic resource]
In this article, we use time-dependent, axisymmetric, hydrodynamic simulations to study the linear stability of the stalled, spherical accretion shock that arises in the postbounce phase of core-collapse supernovae. We show that this accretion shock is stable to radial modes, with decay rates and os...
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| Format: | Electronic eBook |
| Language: | English |
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Oak Ridge, Tenn. : Oak Ridge, Tenn. :
Oak Ridge National Laboratory ; Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2006.
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