Pseudo-Schwarzschild spherical accretion as a classical black hole analogue

DOI10.1007/s10714-005-0194-9zbMath1082.83020arXivastro-ph/0501410OpenAlexW1973713370MaRDI QIDQ2583268

Surajit Dasgupta, Tapas K. Das, Neven Bilić

Publication date: 13 January 2006

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0501410

zbMATH Keywords

Hawking radiationHydrodynamicsBlack hole physicsAccretionAnalogue gravity

Mathematics Subject Classification ID

Black holes (83C57) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (4)

Relativistic sonic geometry for isothermal accretion in the Kerr metric ⋮ On the stability of steady general-relativistic accretion and analogue black holes ⋮ Analogue gravity ⋮ Acoustic geometry through perturbation of mass accretion rate: radial flow in static spacetimes

Cites Work

• Stability and oscillations of an autotroph-herbivore model with time delay
• Analogue Hawking radiation from astrophysical black-hole accretion
• Acoustic black holes: horizons, ergospheres and Hawking radiation
• Relativistic acoustic geometry

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