AN IMPROVED METHOD FOR CONSTRUCTING MODELS OF SELF-GRAVITATING TORI AROUND BLACK HOLES

DOI10.1142/S021827181101944XzbMath1253.83027arXiv1104.3685OpenAlexW3104268830WikidataQ63410502 ScholiaQ63410502MaRDI QIDQ4649660

Nikolaos Stergioulas

Publication date: 13 November 2012

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1104.3685

zbMATH Keywords

black holesaccretionnumerical relativity

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

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Cites Work

• Numerical relativity confronts compact neutron star binaries: a review and status report
• Accurate evolutions of unequal-mass neutron-star binaries: properties of the torus and short GRB engines
• The dynamical stability of differentially rotating discs with constant specific angular momentum
• The dynamical stability of differentially rotating discs - II