Turbulence in core-collapse supernovae

Radice, David; Abdikamalov, Ernazar; Ott, Christian D.; Mösta, Philipp; Couch, Sean M.; Roberts, Luke F.

doi:10.1088/1361-6471/aab872

Turbulence in core-collapse supernovae

Journal Article · Mon Apr 09 00:00:00 EDT 2018 · Journal of Physics. G, Nuclear and Particle Physics

DOI:https://doi.org/10.1088/1361-6471/aab872· OSTI ID:1523397

^[1]; Abdikamalov, Ernazar ^[2]; Ott, Christian D. ^[3]; Mösta, Philipp ^[4]; Couch, Sean M. ^[5]; Roberts, Luke F. ^[6]

Inst. for Advanced Study, Princeton, NJ (United States). School of Natural Sciences; Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
Nazarbayev Univ., Astana (Kazakhstan). Dept. of Physics, School of Science and Technology
California Inst. of Technology (CalTech), Pasadena, CA (United States). Walter Burke Inst. for Theoretical Physics
Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy, Dept. of Computational Mathematics, Science, and Engineering, and National Superconducting Cyclotron Lab.
Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy, and National Superconducting Cyclotron Lab.

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.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-05CH11231; AC02-06CH11357; SC0015904; SC0017955

OSTI ID:: 1523397

Alternate ID(s):: OSTI ID: 22899792

Journal Information:: Journal of Physics. G, Nuclear and Particle Physics, Journal Name: Journal of Physics. G, Nuclear and Particle Physics Journal Issue: 5 Vol. 45; ISSN 0954-3899

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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3D Hydrodynamic Simulations of Carbon Burning in Massive Stars Cristini, Andrea; Meakin, Casey; Hirschi, Raphael arXiv https://doi.org/10.48550/arxiv.1610.05173	text	January 2016
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