Effective Resistivity in Relativistic Reconnection: A Prescription Based on Fully Kinetic Simulations
A variety of high-energy astrophysical phenomena are powered by the release—via magnetic reconnection—of the energy stored in oppositely directed fields. Single-fluid resistive magnetohydrodynamic (MHD) simulations with uniform resistivity yield dissipation rates that are much lower (by nearly 1 ord...
Saved in:
Main Authors: | Abigail Moran, Lorenzo Sironi, Aviad Levis, Bart Ripperda, Elias R. Most, Sebastiaan Selvi |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ada158 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Collisionless Tearing Instability in Relativistic Nonthermal Pair Plasma and Its Application to MHD Turbulence
by: Ivan Demidov, et al.
Published: (2025-01-01) -
Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona
by: Navin Sridhar, et al.
Published: (2025-01-01) -
Low-energy Injection and Nonthermal Particle Acceleration in Relativistic Magnetic Turbulence
by: Divjyot Singh, et al.
Published: (2025-01-01) -
Tearing-mediated Alfvénic Turbulence in a Relativistic Plasma
by: Stanislav Boldyrev, et al.
Published: (2025-01-01) -
Ultra-High-Energy Cosmic Rays Accelerated by Magnetically Dominated Turbulence
by: Luca Comisso, et al.
Published: (2024-01-01)