The key role of magnetic fields in binary neutron star mergers

DOI10.1007/S10714-020-02714-XzbMath1445.85001arXiv2003.07572OpenAlexW3102278469MaRDI QIDQ776790

Riccardo Ciolfi

Publication date: 13 July 2020

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2003.07572

zbMATH Keywords

gamma-ray burstsbinary neutron starsgravitational wave sourcesmagnetohydrodynamical simulations

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Electromagnetic fields in general relativity and gravitational theory (83C50) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Gravitational waves (83C35)

Related Items (3)

Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars ⋮ Spritz: general relativistic magnetohydrodynamics with neutrinos ⋮ Relativistic fluid dynamics: physics for many different scales

Cites Work

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• General relativistic simulations of compact binary mergers as engines for short gamma-ray bursts
• Binary and millisecond pulsars

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