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Tearing-mediated Alfvénic Turbulence in a Relativistic Plasma

Journal Article · · The Astrophysical Journal

Abstract In astrophysical relativistic plasmas, Alfvénic turbulence exists across a wide range of scales. Similar to a nonrelativistic case, this turbulence can be influenced by the tearing instability. We argue that in an ultrarelativistic pair plasma the tearing effects become significant at the critical scale given by a t d rel L / d rel n / ( 4 + 5 n ) , where L represents the outer scale of the turbulence and d rel the relativistic electron inertial scale. Here n = 1 corresponds to the Harris magnetic configurations, while n = 2 applies to localized (non-Harris) magnetic profiles of turbulence-generated current sheets. Below the critical scale, the energy spectrum of magnetic fluctuations steepens to W ( k ) dk ∝ k −(7 n +2)/3 n dk . However, this happens only when σ ˜ L / d rel ( 2 + 4 n ) / ( 4 + 5 n ) , where σ ˜ is the magnetization parameter based on the magnetic fluctuations. If the opposite inequality holds, the Alfvénic cascade is instead affected by charge starvation at scales below a ch d rel d rel / L 1 / 3 σ ˜ 2 / 3 , and the energy spectrum becomes steeper than W ( k ) dk ∝ k −3 dk . When d rel is replaced by its nonrelativistic equivalent, our results agree with the nonrelativistic analysis of N. F. Loureiro & S. Boldyrev (2018). In the Harris case n = 1, they agree with the recent relativistic studies by I. Demidov & Y. Lyubarsky.

Sponsoring Organization:
USDOE
OSTI ID:
2507366
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Vol. 979 Journal Issue: 2; ISSN 0004-637X
Publisher:
American Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English

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