On the Gravitational Angular Momentum of Axial Perturbations of a Regular Black Hole
arXiv:2605.23711 · doi:10.1209/0295-5075/ae63f1
Abstract
This Letter deals with the gravitational angular momentum carried by axial (odd-parity) perturbations of the Bardeen regular black hole within the teleparallel equivalent of general relativity (TEGR). Using the Hamiltonian definition of conserved quantities in TEGR, we derive a closed expression for the perturbative angular momentum in terms of the axial perturbation function . The result exhibits a sharp multipolar selection rule: vanishes for odd values of the multipole index , while even- modes yield a nonzero contribution. The radial and temporal behavior of is illustrated using the known axial quasinormal modes of the Bardeen spacetime.
5 pages, 4 figures
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