Origin of Intense Electron Heating in Relativistic Blast Waves

Autor: Arno Vanthieghem, Martin Lemoine, Laurent Gremillet
Přispěvatelé: Institut Lagrange de Paris, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), National Institutes of Natural Sciences [Tokyo] (NINS), Department of Astrophysical Sciences [Princeton], Princeton University, SLAC National Accelerator Laboratory (SLAC), Stanford University, DAM Île-de-France (DAM/DIF), Direction des Applications Militaires (DAM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire Matière sous Conditions Extrêmes (LMCE), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction des Applications Militaires (DAM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, the NSF grants PHY-1804048 and AST-1814708, A0030407666 made by GENCI and on CORI at the National Energy Research Scientific Computing Center (NERSC) through ALCC award, ANR-10-LABX-0063,ILP,Institute Lagrange of Paris(2010), ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), ANR-14-CE33-0019,MACH,Micro-Astro-CHocs(2014), ANR-20-CE30-0030,UnRIP,Vers la compréhension des instabilités plasma relativistes(2020)
Rok vydání: 2022
Předmět:
Zdroj: Astrophys.J.Lett.
Astrophys.J.Lett., 2022, 930 (1), pp.L8. ⟨10.3847/2041-8213/ac634f⟩
ISSN: 2041-8213
2041-8205
Popis: The modeling of gamma-ray burst afterglow emission bears witness to strong electron heating in the precursor of Weibel-mediated, relativistic collisionless shock waves propagating in unmagnetized electron-ion plasmas. In this Letter, we propose a theoretical model, which describes electron heating via a Joule-like process caused by pitch-angle scattering in the decelerating, self-induced microturbulence and the coherent charge-separation field induced by the difference in inertia between electrons and ions. The emergence of this electric field across the precursor of electron-ion shocks is confirmed by large-scale particle-in-cell (PIC) simulations. Integrating the model using a Monte Carlo-Poisson method, we compare the main observables to the PIC simulations to conclude that the above mechanism can indeed account for the bulk of electron heating.
Comment: 9 pages, 8 figures; to be published in Astrophysical Journal Letters
Databáze: OpenAIRE