A new Ricci-flat rotating metric is obtained by demagnetizing the KBR solution, yielding a deformed Kerr geometry with non-flat asymptotics for which black hole thermodynamics is established.
Kerr black holes in a magnetic universe
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External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.
Numerical simulations show Shannon entropy and MIPP indicators distinguish chaotic from regular orbits of charged particles near weakly magnetized black holes in Einstein-ModMax theory, with parameters restricted by EHT shadow observations.
citing papers explorer
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Demagnetizing KBR and New Ricci-flat Rotating Metric
A new Ricci-flat rotating metric is obtained by demagnetizing the KBR solution, yielding a deformed Kerr geometry with non-flat asymptotics for which black hole thermodynamics is established.
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Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes
External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.
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Chaotic dynamics of charged particles near weakly magnetized black holes in Einstein-ModMax Theory
Numerical simulations show Shannon entropy and MIPP indicators distinguish chaotic from regular orbits of charged particles near weakly magnetized black holes in Einstein-ModMax theory, with parameters restricted by EHT shadow observations.