Radiative Particle-in-Cell Simulations of Turbulent Comptonization in Magnetized Black-Hole Coronae

Daniel Grošelj, Hayk Hakobyan, Andrei M. Beloborodov, Lorenzo Sironi, and Alexander Philippov
Phys. Rev. Lett. 132, 085202 – Published 23 February 2024

Abstract

We report results from the first radiative particle-in-cell simulations of strong Alfvénic turbulence in plasmas of moderate optical depth. The simulations are performed in a local 3D periodic box and self-consistently follow the evolution of radiation as it interacts with a turbulent electron-positron plasma via Compton scattering. We focus on the conditions expected in magnetized coronae of accreting black holes and obtain an emission spectrum consistent with the observed hard state of Cyg X-1. Most of the turbulence power is transferred directly to the photons via bulk Comptonization, shaping the peak of the emission around 100 keV. The rest is released into nonthermal particles, which generate the MeV spectral tail. The method presented here shows promising potential for ab initio modeling of various astrophysical sources and opens a window into a new regime of kinetic plasma turbulence.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 26 January 2023
  • Revised 30 September 2023
  • Accepted 24 January 2024

DOI:https://doi.org/10.1103/PhysRevLett.132.085202

© 2024 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

Daniel Grošelj1,2, Hayk Hakobyan3,4, Andrei M. Beloborodov4,5, Lorenzo Sironi2, and Alexander Philippov6

  • 1Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, B-3001 Leuven, Belgium
  • 2Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA
  • 3Computational Sciences Department, Princeton Plasma Physics Laboratory, Princeton, New Jersey 08540, USA
  • 4Department of Physics and Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA
  • 5Max Planck Institute for Astrophysics, D-85741 Garching, Germany
  • 6Department of Physics, University of Maryland, College Park, Maryland 20742, USA

Article Text (Subscription Required)

Click to Expand

Supplemental Material (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 132, Iss. 8 — 23 February 2024

Reuse & Permissions
Access Options
CHORUS

Article part of CHORUS

Accepted manuscript will be available starting 22 February 2025.
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×