On the Cosmic Ray Driven Firehose Instability

Author(s): Scott, R; Reville, B; Spitkovsky, Anatoly

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DC Field	Value	Language
dc.contributor.author	Scott, R	-
dc.contributor.author	Reville, B	-
dc.contributor.author	Spitkovsky, Anatoly	-
dc.date.accessioned	2022-01-25T15:03:21Z	-
dc.date.available	2022-01-25T15:03:21Z	-
dc.date.issued	2017-01-04	en_US
dc.identifier.citation	Scott, R, Reville, B, Spitkovsky, A. (On the Cosmic Ray Driven Firehose Instability	en_US
dc.identifier.uri	http://arks.princeton.edu/ark:/88435/pr1rj48t9v	-
dc.description.abstract	The role of the non-resonant firehose instability in conditions relevant to the precursors of supernova remnant shocks is considered. Using a second order tensor expansion of the Vlasov-Fokker-Planck equation we illustrate the necessary conditions for the firehose to operate. It is found that for very fast shocks, the diffusion approximation predicts that the linear firehose growth rate is marginally faster than its resonant counterpart. Preliminary hybrid MHD-Vlasov-Fokker-Planck simulation results using young supernova relevant parameters are presented.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartof	AIP Conference Proceedings	en_US
dc.rights	Final published version. Article is made available in OAR by the publisher's permission or policy.	en_US
dc.title	On the Cosmic Ray Driven Firehose Instability	en_US
dc.type	Conference Article	en_US
dc.identifier.doi	10.1063/1.4807033	-
dc.date.eissued	2017-01-04	en_US
pu.type.symplectic	http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article	en_US

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