DYNAMICAL EVOLUTION OF ROTATING ACCRETION USING DIFFERENT BOUNDARY CONDITIONS: STATE AFTER STABLE ACCRETION DISK CREATED

DOI10.1142/S0218271807010912zbMath1200.85021MaRDI QIDQ3500297

Orhan Dönmez

Publication date: 3 June 2008

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

zbMATH Keywords

boundary conditionsblack holehydrodynamicsaccretion disknumerical relativityspiral shockaccretion tori

Mathematics Subject Classification ID

Black holes (83C57) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Code development of three-dimensional general relativistic hydrodynamics with AMR (Adaptive-Mesh Refinement) and results from special and general relativistic hydrodynamics
• Dynamics of thick discs around Schwarzschild-de Sitter black holes

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