Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair

Abstract A static spherically symmetric black hole usually turns out to be either a Schwarzschild black hole or a Reissner-Nordström black hole. This result was summarised by Ruffini and Wheeler as the so-called no hair conjecture which states that for a spherically symmetric black hole only the inf...

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Main Author: Avijit Chowdhury
Format: Article
Language:English
Published: SpringerOpen 2019-11-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-019-7452-6
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author Avijit Chowdhury
author_facet Avijit Chowdhury
author_sort Avijit Chowdhury
collection DOAJ
description Abstract A static spherically symmetric black hole usually turns out to be either a Schwarzschild black hole or a Reissner-Nordström black hole. This result was summarised by Ruffini and Wheeler as the so-called no hair conjecture which states that for a spherically symmetric black hole only the information about mass (M) and electric charge (e) of the black hole is available for an external observer. In this work, we calculate the emission rate of charged particles from an asymptotically flat charged spherically symmetric black hole endowed with a scalar hair using a semi-classical tunneling formalism. We observe that the total entropy of the black hole contains an energy-dependent part due to the scalar charge. The upper bound on the charge-mass ratio of the emitted particles is also observed to decrease with the scalar charge as well.
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spelling doaj.art-110b9409e56a44238a6c05fb4ec4e32d2022-12-22T01:20:16ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-11-0179111710.1140/epjc/s10052-019-7452-6Hawking emission of charged particles from an electrically charged spherical black hole with scalar hairAvijit Chowdhury0IISER KolkataAbstract A static spherically symmetric black hole usually turns out to be either a Schwarzschild black hole or a Reissner-Nordström black hole. This result was summarised by Ruffini and Wheeler as the so-called no hair conjecture which states that for a spherically symmetric black hole only the information about mass (M) and electric charge (e) of the black hole is available for an external observer. In this work, we calculate the emission rate of charged particles from an asymptotically flat charged spherically symmetric black hole endowed with a scalar hair using a semi-classical tunneling formalism. We observe that the total entropy of the black hole contains an energy-dependent part due to the scalar charge. The upper bound on the charge-mass ratio of the emitted particles is also observed to decrease with the scalar charge as well.http://link.springer.com/article/10.1140/epjc/s10052-019-7452-6
spellingShingle Avijit Chowdhury
Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
European Physical Journal C: Particles and Fields
title Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
title_full Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
title_fullStr Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
title_full_unstemmed Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
title_short Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
title_sort hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
url http://link.springer.com/article/10.1140/epjc/s10052-019-7452-6
work_keys_str_mv AT avijitchowdhury hawkingemissionofchargedparticlesfromanelectricallychargedsphericalblackholewithscalarhair