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...

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Autors principals:	Abigail Moran, Lorenzo Sironi, Aviad Levis, Bart Ripperda, Elias R. Most, Sebastiaan Selvi
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal Letters
Matèries:	High energy astrophysics Plasma astrophysics Magnetic fields Magnetohydrodynamics
Accés en línia:	https://doi.org/10.3847/2041-8213/ada158
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