Can we distinguish black holes with electric and magnetic charges from quasinormal modes?
arXiv:2312.03191 · doi:10.1103/PhysRevD.109.084022
Abstract
We compute the quasinormal modes of static and spherically symmetric black holes (BHs) with electric and magnetic charges. For the electrically charged case, the dynamics of perturbations separates into the odd- and even-parity sectors with two coupled differential equations in each sector. In the presence of both electric and magnetic charges, the differential equations of four dynamical degrees of freedom are coupled with each other between odd- and even-parity perturbations. Despite this notable modification, we show that, for a given total charge and mass, a BH with mixed electric and magnetic charges gives rise to the same quasinormal frequencies for fundamental modes. This includes the case in which two BHs have equal electric and magnetic charges for each of them. Thus, the gravitational-wave observations of quasinormal modes during the ringdown phase alone do not distinguish between electrically and magnetically charged BHs.
16 pages, 4 figures
References in corpus (19)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- Constraints on black-hole charges with the 2017 EHT observations of M87*
- Quasinormal modes of charged black holes with corrections from nonlinear electrodynamics
- Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
- Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
- Astrophysical hints for magnetic black holes
- Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone
- Spectral method for metric perturbations of black holes: Kerr background case in general relativity
- Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Hyperbolic orbits on a cone
- Black hole perturbations in Maxwell-Horndeski theories
- Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
- Asymptotics of linear differential systems and application to quasi-normal modes of nonrotating black holes
- Merger rate of charged black holes from the two-body dynamical capture
- Hairy Magnetic and Dyonic Black Holes in the Standard Model
- Monopole-Antimonopole Pair Production in Primordial Magnetic Fields
- Constraining Horndeski theory with gravitational waves from coalescing binaries
- Gravitoelectromagnetic coupled perturbations and quasinormal modes of a charged black hole with scalar hair
- Stability and Observability of Magnetic Primordial Black Hole-Neutron Star Collisions
- Gravitational capture of magnetic monopoles by primordial black holes in the early universe
Cited by in corpus (9)
- Instability of nonsingular black holes in nonlinear electrodynamics
- Superradiant Instability of Magnetic Black Holes
- Probing the signature of axions through the quasinormal modes of black holes
- Quasinormal Modes and Greybody Factors of Charged Symmergent Black Hole
- Linear stability of vector Horndeski black holes
- Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes
- Greybody factors of charged black holes with axion hair
- Greybody Factor for massive scalar field in charged black hole
- Vector Horndeski black holes in nonlinear electrodynamics