Exploding SNe with jets: time-scales
High Energy Astrophysical Phenomena
2015-06-04 v1
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.
Keywords
Cite
@article{arxiv.1204.2560,
title = {Exploding SNe with jets: time-scales},
author = {Oded Papish and Noam Soker},
journal= {arXiv preprint arXiv:1204.2560},
year = {2015}
}
Comments
To appear in Death of Massive Stars: Supernovae and Gamma-Ray Bursts, Proceedings IAU Symposium No. 279, 2012, eds. P. Roming, N. Kawai & E. Pian