Effective Resistivity in Relativistic Collisionless Reconnection

Magnetic reconnection can power spectacular high-energy astrophysical phenomena by producing nonthermal energy distributions in highly magnetized regions around compact objects. By means of two-dimensional fully kinetic particle-in-cell (PIC) simulations, we investigate relativistic collisionless pl...

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Hlavní autoři:	S. Selvi, O. Porth, B. Ripperda, F. Bacchini, L. Sironi, R. Keppens
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2023-01-01
Edice:	The Astrophysical Journal
Témata:	High energy astrophysics Plasma astrophysics Compact objects Magnetic fields Relativity Magnetohydrodynamics
On-line přístup:	https://doi.org/10.3847/1538-4357/acd0b0
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