Behaviour of low angular momentum relativistic accretion close to the event horizon

Tapas K. Das, Sankhasubhra Nag, Swathi Hegde, Sourav Bhattacharya, Ishita Maity · arXiv (Cornell University) · 2012

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Type: article
Published: 2012-11-29
Cited by: 1
References: 18
Access: Open access
OpenAlex: https://openalex.org/W43992243
Semantic Scholar: https://api.semanticscholar.org/CorpusID:115204291

Keywords

Physics, Angular momentum, Event horizon, Kerr metric, Rotating black hole

References

Observational Evidence for Black Holes in the UniverseSandip K. Chakrabarti — 2008
Shadows as a tool to evaluate black hole parameters and a dimension of spacetimeA. F. Zakharov, F. De Paolis, G. Ingrosso — 2012
Accretion power in astrophysicsJuhan Frank, A. R. King, D. J. Raine — 1985
Probing relativistic astrophysics around SMBHs: The Suzaku AGN spin surveyC. S. Reynolds, Laura Brenneman, A. Lohfink — 2011
Statistical MechanicsDresden, Max — 2021
Fluid mechanicsPhilip G. Drazin — 1994
Nonlinear Ordinary Differential EquationsArieh Iserles — 1988
Ordinary Differential EquationsVirginia W. Noonburg — 2014

Cited by

Retrograde versus Prograde Models of Accreting Black HolesDavid Garofalo — 2013

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