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arXiv · 1509.02494

Stochasticity and efficiency of simplified core-collapse supernova explosions

Christian Y. Cardall·Reuben D. Budiardja
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Abstract

We present an initial report on 160 simulations of a highly simplified model of the post-bounce core-collapse supernova environment in three spatial dimensions (3D). We set different values of a parameter characterizing the impact of nuclear dissociation at the stalled shock in order to regulate the post-shock fluid velocity, thereby determining the relative importance of convection and the stationary accretion shock instability (SASI). While our convection-dominated runs comport with the paradigmatic notion of a `critical neutrino luminosity' for explosion at a given mass accretion rate (albeit with a nontrivial spread in explosion times just above threshold), the outcomes of our SASI-dominated runs are much more stochastic: a sharp threshold critical luminosity is `smeared out' into a rising probability of explosion over a $\sim 20\%$ range of luminosity. We also find that the SASI-dominated models are able to explode with 3 to 4 times less efficient neutrino heating, indicating that progenitor properties, and fluid and neutrino microphysics, conducive to the SASI would make the neutrino-driven explosion mechanism more robust.

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Christian Y. Cardall, Reuben D. Budiardja. 2015-10-09. Stochasticity and efficiency of simplified core-collapse supernova explosions. https://doi.org/10.1088/2041-8205%2F813%2F1%2Fl6

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