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, offering a qualitative explanation for the declining QPO frequencies in black hole…
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Thermal Conduction and Thermal-Driven Winds in Magnetized Viscous Accretion Disk Dynamics
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, offering a qualitative explanation for the declining QPO frequencies in black hole…