NON-LINEARITIES IN ACCRETION AND WINDS AROUND ROTATING BLACK HOLES USING PSEUDO-KERR GEOMETRY

DOI10.1142/S0218271807009279zbMath1200.83081OpenAlexW1966115458MaRDI QIDQ3500283

Soumen Mondal, Sandip K. Chakrabarti

Publication date: 3 June 2008

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

Full work available at URL: https://doi.org/10.1142/s0218271807009279

Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar structure (85A15)

Related Items (1)

ACCRETION PROBLEM IN A KERR BLACK HOLE GEOMETRY VIEWED AS FLOWS IN CONVERGING–DIVERGING DUCTS

Cites Work

• SIGNATURES OF ACCRETION SHOCKS IN BROADBAND SPECTRUM OF ADVECTIVE FLOWS AROUND BLACK HOLES

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