Viscous transonic accretion flow simulations around spinning black holes show that QPO frequency ranges and power-law photon indices correlate with black hole spin.
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2 Pith papers cite this work, alongside 15 external citations. Polarity classification is still indexing.
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Winds in shocked magnetized viscous accretion flows around rotating black holes reduce luminosity, modify shock radius, compression, and strength, and impose a critical wind parameter p^crit above which steady shocks cease to exist.
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QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole
Viscous transonic accretion flow simulations around spinning black holes show that QPO frequency ranges and power-law photon indices correlate with black hole spin.
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Influence of winds on shocked magnetized viscous accretion flows around rotating black holes
Winds in shocked magnetized viscous accretion flows around rotating black holes reduce luminosity, modify shock radius, compression, and strength, and impose a critical wind parameter p^crit above which steady shocks cease to exist.