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

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...

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Main Authors: Evgeny A. Gorbunov, Fabio Bacchini, Vladimir Zhdankin, Gregory R. Werner, Mitchell C. Begelman, Dmitri A. Uzdensky
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/adbca4
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author Evgeny A. Gorbunov
Fabio Bacchini
Vladimir Zhdankin
Gregory R. Werner
Mitchell C. Begelman
Dmitri A. Uzdensky
author_facet Evgeny A. Gorbunov
Fabio Bacchini
Vladimir Zhdankin
Gregory R. Werner
Mitchell C. Begelman
Dmitri A. Uzdensky
author_sort Evgeny A. Gorbunov
collection DOAJ
description 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.
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institution Kabale University
issn 2041-8205
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publishDate 2025-01-01
publisher IOP Publishing
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series The Astrophysical Journal Letters
spelling doaj-art-c2d2e94ba93f482a9d1720f379fbf7782025-08-20T03:39:44ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019821L2810.3847/2041-8213/adbca4First-principles Measurement of Ion and Electron Energization in Collisionless Accretion FlowsEvgeny A. Gorbunov0https://orcid.org/0000-0001-9073-8591Fabio Bacchini1https://orcid.org/0000-0002-7526-8154Vladimir Zhdankin2https://orcid.org/0000-0003-3816-7896Gregory R. Werner3https://orcid.org/0000-0001-9039-9032Mitchell C. Begelman4https://orcid.org/0000-0003-0936-8488Dmitri A. Uzdensky5https://orcid.org/0000-0001-8792-6698Centre for Mathematical Plasma Astrophysics , Department of Mathematics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium ; evgeny.gorbunov@kuleuven.beCentre for Mathematical Plasma Astrophysics , Department of Mathematics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium ; evgeny.gorbunov@kuleuven.be; Royal Belgian Institute for Space Aeronomy , Solar-Terrestrial Centre of Excellence, Ringlaan 3, 1180 Uccle, BelgiumDepartment of Physics, University of Wisconsin-Madison , Madison, WI 53706, USACenter for Integrated Plasma Studies, Department of Physics, University of Colorado , 390 UCB, Boulder, CO 80309-0390, USAJILA, University of Colorado and National Institute of Standards and Technology , 440 UCB, Boulder, CO 80309-0440, USA; Department of Astrophysical and Planetary Sciences, University of Colorado , 391 UCB, Boulder, CO 80309-0391, USACenter for Integrated Plasma Studies, Department of Physics, University of Colorado , 390 UCB, Boulder, CO 80309-0390, USA; Rudolf Peierls Centre for Theoretical Physics, Clarendon Laboratory, University of Oxford , Parks Rd., Oxford, OX1 3PU, UKWe 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.https://doi.org/10.3847/2041-8213/adbca4AccretionAstronomical simulationsSupermassive black holesPlasma astrophysicsPlasma physics
spellingShingle Evgeny A. Gorbunov
Fabio Bacchini
Vladimir Zhdankin
Gregory R. Werner
Mitchell C. Begelman
Dmitri A. Uzdensky
First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
The Astrophysical Journal Letters
Accretion
Astronomical simulations
Supermassive black holes
Plasma astrophysics
Plasma physics
title First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
title_full First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
title_fullStr First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
title_full_unstemmed First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
title_short First-principles Measurement of Ion and Electron Energization in Collisionless Accretion Flows
title_sort first principles measurement of ion and electron energization in collisionless accretion flows
topic Accretion
Astronomical simulations
Supermassive black holes
Plasma astrophysics
Plasma physics
url https://doi.org/10.3847/2041-8213/adbca4
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