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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Үндсэн зохиолчид:	Abigail Moran, Lorenzo Sironi, Aviad Levis, Bart Ripperda, Elias R. Most, Sebastiaan Selvi
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2025-01-01
Цуврал:	The Astrophysical Journal Letters
Нөхцлүүд:	High energy astrophysics Plasma astrophysics Magnetic fields Magnetohydrodynamics
Онлайн хандалт:	https://doi.org/10.3847/2041-8213/ada158
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!