Parity violation in photon quasinormal modes of black holes
arXiv:2506.04149 · doi:10.1103/mnw1-nlpr
Abstract
Given that black holes are ubiquitous in the universe and axion-like scalar fields are potential candidates for dark energy and/or dark matter, it is natural to consider cosmological black holes endowed with axion hair. We investigate the photon quasinormal modes of a Schwarzschild black hole with axion hair where the electromagnetic field is coupled to the axion field via a Chern-Simons interaction. We derive the master equations for the electromagnetic field as a set of coupled equations for parity-even and parity-odd modes and numerically compute quasinormal modes by using Leaver's continued fraction method. We find parity violation in the polarization of photons within the quasinormal mode spectrum. This parity violation in electromagnetic signals could serve as a new probe to explore the nature of the dark sector.
22 pages, 1 figure
References in corpus (6)
- Ultralight scalars as cosmological dark matter
- Chiral Primordial Gravitational Waves from a Lifshitz Point
- Circular Polarization of Primordial Gravitational Waves in String-inspired Inflationary Cosmology
- Probing Parity-Violation with the Four-Point Correlation Function of BOSS Galaxies
- Black Hole Hair from Scalar Dark Matter
- Circularly polarized gravitational waves in Chern-Simons gravity originated from an axion domain wall