General Relativistic Simulations of Accretion Disks Around Tilted Kerr Black Holes

DOI10.1007/978-3-319-10488-1_10zbMath1329.85006OpenAlexW2601478092WikidataQ63410479 ScholiaQ63410479MaRDI QIDQ3463600

Nikolaos Stergioulas, V. Mewes, José A. Font, Filippo Galeazzi, Pedro Montero

Publication date: 19 January 2016

Published in: Gravitational Wave Astrophysics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/978-3-319-10488-1_10

zbMATH Keywords

general relativistic simulations of accretiontilted Kerr black holes

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items

Aliasing instabilities in the numerical evolution of the Einstein field equations

Uses Software

• GRHydro
• Einstein Toolkit

Cites Work

• Republication of: The dynamics of general relativity
• The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
• Evolution of three-dimensional gravitational waves: Harmonic slicing case
• Numerical integration of Einstein’s field equations
• Accurate evolutions of unequal-mass neutron-star binaries: properties of the torus and short GRB engines
• Evolutions in 3D numerical relativity using fixed mesh refinement
• GRHydro: a new open-source general-relativistic magnetohydrodynamics code for the Einstein toolkit