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Exploding SNe with jets: time-scales
2011
Proceedings of the International Astronomical Union
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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.
doi:10.1017/s1743921312013439
fatcat:td2jxihmzfa3xntdxsab66cpiu