A critical scalar field charge in a magnetized black hole produces universal QNM power-law scaling with exponent ~1/2, marking a confined-to-deconfined transition.
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Acoustic horizons in spinning black-hole accretion with spatially varying adiabatic index have surface gravities that depend on the black-hole spin parameter.
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Universality in quasinormal modes of a magnetized black hole
A critical scalar field charge in a magnetized black hole produces universal QNM power-law scaling with exponent ~1/2, marking a confined-to-deconfined transition.
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On the spin dependence of the emergent gravity phenomena as observed in axially symmetric black hole accretion with spatially varying adiabatic index
Acoustic horizons in spinning black-hole accretion with spatially varying adiabatic index have surface gravities that depend on the black-hole spin parameter.