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.
Black holes in a magnetic universe
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
fields
gr-qc 4years
2026 4verdicts
UNVERDICTED 4representative citing papers
New exact Kerr black hole solution in an electromagnetic background spacetime that includes a cosmological horizon without a cosmological constant.
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.
Epicyclic frequencies, periapsis shift, and gravitational Larmor precession are derived for charged particles in the weak-magnetic limit of a magnetized Kiselev black hole.
citing papers explorer
-
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.
-
New Rotating Black Hole in Electromagnetic Fields: Cosmological Horizon without Cosmological Constant
New exact Kerr black hole solution in an electromagnetic background spacetime that includes a cosmological horizon without a cosmological constant.
-
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.
-
Epicyclic motion of charged particles around a weakly magnetized Kiselev black hole
Epicyclic frequencies, periapsis shift, and gravitational Larmor precession are derived for charged particles in the weak-magnetic limit of a magnetized Kiselev black hole.