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Turbulence in core-collapse supernovae

Radice, David and Abdikamalov, Ernazar and Ott, Christian D. and Mösta, Philipp and Couch, Sean M. and Roberts, Luke F. (2018) Turbulence in core-collapse supernovae. Journal of Physics G: Nuclear and Particle Physics, 45 (5). Art. No. 053003. ISSN 0954-3899. https://resolver.caltech.edu/CaltechAUTHORS:20180409-101015330

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Abstract

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1361-6471/aab872DOIArticle
http://iopscience.iop.org/article/10.1088/1361-6471/aab872/metaPublisherArticle
ORCID:
AuthorORCID
Radice, David0000-0001-6982-1008
Ott, Christian D.0000-0003-4993-2055
Mösta, Philipp0000-0002-9371-1447
Roberts, Luke F.0000-0001-7364-7946
Additional Information:© 2018 IOP Publishing Ltd. Received 1 October 2017; Accepted 21 March 2018; Accepted Manuscript online 21 March 2018; Published 9 April 2018.
Group:TAPIR
Issue or Number:5
Record Number:CaltechAUTHORS:20180409-101015330
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180409-101015330
Official Citation:David Radice et al 2018 J. Phys. G: Nucl. Part. Phys. 45 053003
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:85689
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Apr 2018 20:16
Last Modified:09 Mar 2020 13:19

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