Exploding SNe with jets: time-scales release_k3pq7d6bdvfjrlzw6uyftwafiq

by Oded Papish, Noam Soker

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2012  

Abstract

We perform hydrodynamical simulations of core collapse supernovae (CCSNe) with a cylindrically-symmetrical numerical code (FLASH) to study the inflation of bubbles and the initiation of the explosion within the frame of the jittering-jets model. We study the typical time- scale of the model and compare it to the typical time-scale of the delayed neutrino mechanism. Our analysis shows that the explosion energy of the delayed neutrino mechanism is an order of magnitude less than the required 10^51 erg.
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Type  article
Stage   submitted
Date   2012-04-11
Version   v1
Language   en ?
arXiv  1204.2560v1
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