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Title: Upper limit of the viscosity parameter in accretion flows around a black hole with shock waves

Journal Article · · Astrophysical Journal

Black hole accretion is necessarily transonic; thus, flows must become supersonic and, therefore, sub-Keplerian before they enter into the black hole. The viscous timescale is much longer than the infall timescale close to a black hole. Hence, the angular momentum remains almost constant and the centrifugal force ∼l{sup 2}/r{sup 3} becomes increasingly dominant over the gravitational force ∼1/r{sup 2}. The slowed down matter piles creating an accretion shock. The flow between shock and inner sonic point is puffed up and behaves like a boundary layer. This so-called Comptonizing cloud/corona produces hard X-rays and jets/outflows and, therefore, is an important component of black hole astrophysics. In this paper, we study steady state viscous, axisymmetric, transonic accretion flows around a Schwarzschild black hole. We adopt a viscosity parameter α and compute the highest possible value of α (namely, α{sub cr}) for each pair of two inner boundary parameters (namely, specific angular momentum carried to horizon, l{sub in} and specific energy at inner sonic point, E(x{sub in})) which is still capable of producing a standing or oscillating shock. We find that while such possibilities exist for α as high as α{sub cr}=0.3 in very small regions of the flow parameter space, typical α{sub cr} appears to be about ∼0.05–0.1. Coincidentally, this also happens to be the typical viscosity parameter achieved by simulations of magnetorotational instabilities in accretion flows. We therefore believe that all realistic accretion flows are likely to have centrifugal pressure supported shocks unless the viscosity parameter everywhere is higher than α{sub cr}.

OSTI ID:
22882333
Journal Information:
Astrophysical Journal, Vol. 816, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X
Country of Publication:
United Kingdom
Language:
English