Implications of turbulence for jets in core-collapse supernova explosions

@article{Gilkis2014ImplicationsOT,
  title={Implications of turbulence for jets in core-collapse supernova explosions},
  author={A. Gilkis and N. Soker},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2014}
}
We show that turbulence in core collapse supernovae (CCSNe) which has been shown recently to ease shock revival might also lead to the formation of intermittent thick accretion disks, or accretion belts, around the newly born neutron star (NS). The accretion morphology is such that two low density funnels are formed along the polar directions. The disks then are likely to launch jets with a varying axis direction, i.e., jittering-jets, through the two opposite funnels. The energy contribution… Expand

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Numerical Astrophysics, 422 This preprint was prepared with the AAS L
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