Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2verdicts
UNVERDICTED 2representative citing papers
Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.
citing papers explorer
-
Orbital dynamics and precession in magnetized Kerr spacetime
Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.
-
Hidden Symmetries and Gyromagnetic Ratio of Kerr-Newman Black Holes in $f(R)$ Gravity
Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.