NUMERICAL TREATMENT OF THIN ACCRETION DISK DYNAMICS AROUND ROTATING BLACK HOLES

DOI10.1142/S0218271810018256zbMath1208.83078MaRDI QIDQ3070388

Orhan Dönmez, Deniz Yildiran

Publication date: 3 February 2011

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

zbMATH Keywords

numerical simulationKerr black holerelativistic hydrodynamicsaccretion diskshock cone

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) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Cites Work

• A flux-split algorithm applied to relativistic flows
• Addendum: Hawking radiation of photons in a variable-mass Kerr black hole
• Code development of three-dimensional general relativistic hydrodynamics with AMR (Adaptive-Mesh Refinement) and results from special and general relativistic hydrodynamics

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