Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes
In the case of cold accretion disk, coupling between charge neutral gas and magnetic field is too weak such that the magneto-rotational instability will be less effective or even stop working. In such a situation it is of prime interest to investigate the pure hydrodynamic turbulence and transport p...
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| Language: | en_US |
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2013
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| Online Access: | http://etd.iisc.ernet.in/handle/2005/2076 http://etd.ncsi.iisc.ernet.in/abstracts/2677/G24857-Abs.pdf |