A new general relativistic magnetohydrodynamics code for dynamical spacetimes

DOI10.1051/0004-6361:200810086zbMath1156.85320arXiv0804.4572OpenAlexW3106230370WikidataQ68858156 ScholiaQ68858156MaRDI QIDQ3614091

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Publication date: 16 March 2009

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0804.4572

zbMATH Keywords

relativitygravitationhydrodynamicsmagnetohydrodynamics (MHD)methods: numericalstars: supernovae: general

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Software, source code, etc. for problems pertaining to astronomy and astrophysics (85-04)

Related Items (4)

GRaM-X: a new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit ⋮ On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars ⋮ Spritz: a new fully general-relativistic magnetohydrodynamic code ⋮ Gravitational waves from gravitational collapse

Uses Software

• WhiskyMHD
• HARM

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