A large-scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae

Philipp Mösta (), Christian D. Ott, David Radice, Luke F. Roberts, Erik Schnetter and Roland Haas
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Philipp Mösta: TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology
Christian D. Ott: TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology
David Radice: TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology
Luke F. Roberts: TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology
Erik Schnetter: Perimeter Institute for Theoretical Physics
Roland Haas: Max Planck Institute for Gravitational Physics

Nature, 2015, vol. 528, issue 7582, 376-379

Abstract: Global, three-dimensional simulations of rapidly rotating massive stars show that turbulence driven by magnetohydrodynamic instability is a promising mechanism for the formation of pulsars and magnetars, the latter potentially powering hyperenergetic and superluminous supernovae.

Date: 2015
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DOI: 10.1038/nature15755

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