Exploding Core-Collapse Supernovae by Jets-Driven Feedback Mechanism

We study the flow structure in the jittering-jets explosion model of core-collapse supernovae (CCSNe) using 2.5D hydrodynamical simulations and find that some basic requirements for explosion are met by the flow. In the jittering-jets model jets are launched by intermittent accretion disk around the...

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Veröffentlicht in:	arXiv.org 2013-11
Hauptverfasser:	Papish, Oded, Soker, Noam
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Computer simulation Ejection Explosions Feedback Jets Kinetic energy Neutron stars Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics Supernovae
Online-Zugang:	Volltext
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