Journal article
Thermal disequilibration of ions and electrons by collisionless plasma turbulence
- Abstract:
- Does overall thermal equilibrium exist between ions and electrons in a weakly collisional, magnetized, turbulent plasma? And, if not, how is thermal energy partitioned between ions and electrons? This is a fundamental question in plasma physics, the answer to which is also crucial for predicting the properties of far-distant astronomical objects such as accretion disks around black holes. In the context of disks, this question was posed nearly two decades ago and has since generated a sizeable literature. Here we provide the answer for the case in which energy is injected into the plasma via Alfvénic turbulence: Collisionless turbulent heating typically acts to disequilibrate the ion and electron temperatures. Numerical simulations using a hybrid fluid-gyrokinetic model indicate that the ion–electron heating-rate ratio is an increasing function of the thermal-to-magnetic energy ratio, βi: It ranges from ∼0.05 at βi=0.1 to at least 30 for βi≳10. This energy partition is approximately insensitive to the ion-to-electron temperature ratio Ti/Te. Thus, in the absence of other equilibrating mechanisms, a collisionless plasma system heated via Alfvénic turbulence will tend toward a nonequilibrium state in which one of the species is significantly hotter than the other, i.e., hotter ions at high βi and hotter electrons at low βi. Spectra of electromagnetic fields and the ion distribution function in 5D phase space exhibit an interesting new magnetically dominated regime at high βi and a tendency for the ion heating to be mediated by nonlinear phase mixing (“entropy cascade”) when βi≲1 and by linear phase mixing (Landau damping) when βi≫1.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 943.2KB, Terms of use)
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- Publisher copy:
- 10.1073/pnas.1812491116
Authors
+ Engineering and Physical Sciences Research Council
More from this funder
- Funding agency for:
- Schekochihin, A
- Grant:
- EP/M022331/1
- Publisher:
- National Academy of Sciences
- Journal:
- Proceedings of the National Academy of Sciences More from this journal
- Volume:
- 116
- Issue:
- 3
- Pages:
- 771-776
- Publication date:
- 2018-12-31
- Acceptance date:
- 2018-11-30
- DOI:
- EISSN:
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1091-6490
- ISSN:
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0027-8424
- Keywords:
- Pubs id:
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pubs:891167
- UUID:
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uuid:58ddcc2b-5242-437a-b038-82d28f6fafb9
- Local pid:
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pubs:891167
- Source identifiers:
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891167
- Deposit date:
-
2018-11-17
Terms of use
- Copyright holder:
- Kawazura et al
- Copyright date:
- 2018
- Notes:
-
Copyright © 2019 the Author(s). Published by PNAS.
This open access article is distributed under Creative Commons Attribution License 4.0 (CC BY).
- Licence:
- CC Attribution (CC BY)
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