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On the possibilities of mass loss from an advective accretion disc around stationary black holes

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arxiv 1405.6895 v1 pith:JOYL5545 submitted 2014-05-27 astro-ph.HE

Santabrata Das , Indranil Chattopadhyay , Anuj Nandi , Biplob Sarkar This is my paper · ORCID
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keywords discparameterviscosityaccretionadvectivearoundblackcooling
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We study the coupled disc-jet system around the black hole where the outflow solutions are obtained in terms of the inflow parameters. We observe that an advective accretion disc can eject outflows/jets for wide range of viscosity parameter. However, such possibility is reduced if the cooling is active as the energy dissipative process inside the disc. For mass outflow, we obtain the parameter space spanned by the inflow angular momentum and the viscosity in terms of cooling and quantify the limits of viscosity parameter.

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  1. Thermal Conduction and Thermal-Driven Winds in Magnetized Viscous Accretion Disk Dynamics

    astro-ph.HE 2025-01 conditional novelty 7.0 of 10

    In a magnetized viscous accretion disk model, adding saturated thermal conduction and thermal-driven winds moves the standing shock outward from the black hole and shrinks the parameter space for shock solutions, offe...

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