Wave Generation and Heat Flux Suppression in Astrophysical Plasma Systems

Roberg-Clark, G. T.; Drake, J. F.; Swisdak, M.; Reynolds, C. S.

doi:10.3847/1538-4357/aae393

Title: Wave Generation and Heat Flux Suppression in Astrophysical Plasma Systems

Journal Article · 10 November 2018 · The Astrophysical Journal (Online)

DOI: https://doi.org/10.3847/1538-4357/aae393 · OSTI ID:1544071

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Univ. of Maryland, College Park, MD (United States). Dept. of Physics
Univ. of Maryland, College Park, MD (United States). Dept. of Physics, Institute for Research in Electronics and Applied Physics, and Institute for Physical Science and Technology; Joint Space-Science Institute (JSI), College Park, MD (United States)
Univ. of Maryland, College Park, MD (United States). Dept. of Physics, Institute for Research in Electronics; Joint Space-Science Institute (JSI), College Park, MD (United States)
Institute of Astronomy, Cambridge (United Kingdom)

Heat flux suppression in collisionless plasmas for a large range of plasma β is explored using two-dimensional particle-in-cell simulations with a strong, sustained thermal gradient. We find that a transition takes place between whistler-dominated (high-β) and double-layer-dominated (low-β) heat flux suppression. Whistlers saturate at small amplitude in the low beta limit and are unable to effectively suppress the heat flux. Electrostatic double layers (DLs) suppress the heat flux to a mostly constant factor of the free-streaming value once this transition happens. The DL physics is an example of ion–electron coupling and occurs on a scale of roughly the electron Debye length. The scaling of ion heating associated with the various heat flux driven instabilities is explored over the full range of β explored. The range of plasma-βs studied in this work makes it relevant to the dynamics of a large variety of astrophysical plasmas, including the intracluster medium of galaxy clusters, hot accretion flows, stellar and accretion disk coronae, and the solar wind.

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Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Univ. of California, Oakland, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1544071

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 867; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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