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Natural Quenching of Inner Viscous Torques in Accretion Disks Around Mini-Boson Stars
The standard Novikov-Thorne model for geometrically thin accretion disks assumes a zero-torque inner boundary condition at the innermost stable circular orbit (ISCO). Relaxing this assumption to allow a finite viscous torque---driven by magnetic stresses bridging the plunging region---can significan
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