Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature

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 radiatio...

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Autor principal: R.A. Konoplya
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Lenguaje:EN
Publicado: Elsevier 2021
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spelling oai:doaj.org-article:08b11ff561e846cfa4c65cb1de2c3af22021-12-04T04:32:31ZBlack holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature0370-269310.1016/j.physletb.2021.136734https://doaj.org/article/08b11ff561e846cfa4c65cb1de2c3af22021-12-01T00:00:00Zhttp://www.sciencedirect.com/science/article/pii/S0370269321006742https://doaj.org/toc/0370-2693Recently, 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.R.A. KonoplyaElsevierarticlePhysicsQC1-999ENPhysics Letters B, Vol 823, Iss , Pp 136734- (2021)
institution DOAJ
collection DOAJ
language EN
topic Physics
QC1-999
spellingShingle Physics
QC1-999
R.A. Konoplya
Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
description 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.
format article
author R.A. Konoplya
author_facet R.A. Konoplya
author_sort R.A. Konoplya
title Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
title_short Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
title_full Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
title_fullStr Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
title_full_unstemmed Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature
title_sort black holes in galactic centers: quasinormal ringing, grey-body factors and unruh temperature
publisher Elsevier
publishDate 2021
url https://doaj.org/article/08b11ff561e846cfa4c65cb1de2c3af2
work_keys_str_mv AT rakonoplya blackholesingalacticcentersquasinormalringinggreybodyfactorsandunruhtemperature
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