QR-Code

Microphysical Plasma Relations from Special-relativistic Turbulence

The microphysical, kinetic properties of astrophysical plasmas near accreting compact objects are still poorly understood. For instance, in modern general-relativistic magnetohydrodynamic simulations, the relation between the temperature of electrons T _e and protons T _p is prescribed in terms of s...

Ausführliche Beschreibung

Gespeichert in:
Bibliografische Detailangaben
Hauptverfasser: Claudio Meringolo, Alejandro Cruz-Osorio, Luciano Rezzolla, Sergio Servidio
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2023-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/acaefe
Tags: Tag hinzufügen
Keine Tags, Fügen Sie das erste Tag hinzu!