TY - JOUR
T1 - Turbulence in core-collapse supernovae
AU - Radice, David
AU - Abdikamalov, Ernazar
AU - Ott, Christian D.
AU - Mösta, Philipp
AU - Couch, Sean M.
AU - Roberts, Luke F.
N1 - Publisher Copyright:
© 2018 IOP Publishing Ltd.
PY - 2018/4/9
Y1 - 2018/4/9
N2 - Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental component of the core-collapse supernova explosion mechanism. Neutrino-driven convection, the standing accretion shock instability, and relic-perturbations from advanced nuclear burning stages can all impact the outcome of core collapse in a qualitative and quantitative way. Here, we review the current understanding of these phenomena and their role in the explosion of massive stars. We also discuss the role of protoneutron star convection and of magnetic fields in the context of the delayed neutrino mechanism.
AB - Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental component of the core-collapse supernova explosion mechanism. Neutrino-driven convection, the standing accretion shock instability, and relic-perturbations from advanced nuclear burning stages can all impact the outcome of core collapse in a qualitative and quantitative way. Here, we review the current understanding of these phenomena and their role in the explosion of massive stars. We also discuss the role of protoneutron star convection and of magnetic fields in the context of the delayed neutrino mechanism.
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U2 - 10.1088/1361-6471/aab872
DO - 10.1088/1361-6471/aab872
M3 - Review article
AN - SCOPUS:85046656428
SN - 0954-3899
VL - 45
JO - Journal of Physics G: Nuclear and Particle Physics
JF - Journal of Physics G: Nuclear and Particle Physics
IS - 5
M1 - 053003
ER -