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arXiv · 1204.2560

Exploding SNe with jets: time-scales

Oded Papish·Noam Soker
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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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Oded Papish, Noam Soker. 2012-04-11. Exploding SNe with jets: time-scales. https://doi.org/10.1017/s1743921312013439

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