Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
Sep 3, 20219 pages
Published in:
- Phys.Lett.B 823 (2021) 136734
- Published: Dec 10, 2021
e-Print:
- 2109.01640 [gr-qc]
DOI:
- 10.1016/j.physletb.2021.136734 (publication)
View in:
Citations per year
Abstract: (Elsevier B.V.)
Recently, Cardoso et al. [1] found an exact solution describing the black hole immersed in a galactic-like distribution of matter. There, the properties of gravitational radiation were studied. Here we continue analysis of properties of this geometry via consideration of the electromagnetic radiation. We calculate quasinormal modes, asymptotic tails and grey-body factors for electromagnetic radiation. In addition, we discuss the Unruh temperature for this spacetime. Estimations made in the regime which is best fitting the galaxies behavior show that influence of the environment on classical and quantum radiation around such black holes must be relatively small.Note:
- 7 pages, revtex, the version accepted for publication in Physics Letters B
- radiation: electromagnetic
- radiation: quantum
- black hole
- temperature
- galaxy
- space-time
- geometry
- gravitational radiation
- quasinormal mode
- Unruh effect
References(28)
Figures(4)
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