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First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows

Abstract:
We present the largest 3D particle-in-cell shearing-box simulations of turbulence driven by the magnetorotational instability, for the first time employing the realistic proton-to-electron mass ratio. We investigate the energy partition between relativistically hot electrons and subrelativistic ions in turbulent accreting plasma, a regime relevant to collisionless, radiatively inefficient accretion flows around supermassive black holes such as those targeted by the Event Horizon Telescope. We provide a simple empirical formula to describe the measured heating ratio between ions and electrons, which can be used for more accurate global modeling of accretion flows with standard fluid approaches such as general-relativistic magnetohydrodynamics.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/2041-8213/adbca4

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Author
ORCID:
0000-0001-9073-8591
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Role:
Author
ORCID:
0000-0002-7526-8154
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ORCID:
0000-0003-3816-7896
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ORCID:
0000-0001-9039-9032
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Role:
Author
ORCID:
0000-0003-0936-8488


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal Letters More from this journal
Volume:
982
Issue:
1
Article number:
L28
Publication date:
2025-03-19
Acceptance date:
2025-03-05
DOI:
EISSN:
2041-8213
ISSN:
2041-8205


Language:
English
Keywords:
Source identifiers:
2784838
Deposit date:
2025-03-19
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