Quantum corrected black holes from string T-duality

In this letter we present some stringy corrections to black hole spacetimes emerging from string T-duality. As a first step, we derive the static Newtonian potential by exploiting the relation between the T-duality and the path integral duality. We show that the intrinsic non-perturbative nature of...

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Main Authors: Piero Nicolini, Euro Spallucci, Michael F. Wondrak
Format: Article
Language:English
Published: Elsevier 2019-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269319306021
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spelling doaj-b24a02caa316405d8c370446209f31102020-11-25T01:08:44ZengElsevierPhysics Letters B0370-26932019-10-01797Quantum corrected black holes from string T-dualityPiero Nicolini0Euro Spallucci1Michael F. Wondrak2Frankfurt Institute for Advanced Studies (FIAS), Ruth-Moufang-Straße 1, 60438 Frankfurt am Main, Germany; Institut für Theoretische Physik, Johann Wolfgang Goethe-Universität Frankfurt am Main, Max-von-Laue-Straße 1, 60438 Frankfurt am Main, Germany; Corresponding author.Dipartimento di Fisica, Università degli Studi di Trieste, Strada Costiera 11, 34151 Trieste, Italy; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Strada Costiera 11, 34151 Trieste, ItalyFrankfurt Institute for Advanced Studies (FIAS), Ruth-Moufang-Straße 1, 60438 Frankfurt am Main, Germany; Institut für Theoretische Physik, Johann Wolfgang Goethe-Universität Frankfurt am Main, Max-von-Laue-Straße 1, 60438 Frankfurt am Main, GermanyIn this letter we present some stringy corrections to black hole spacetimes emerging from string T-duality. As a first step, we derive the static Newtonian potential by exploiting the relation between the T-duality and the path integral duality. We show that the intrinsic non-perturbative nature of stringy corrections introduces an ultraviolet cutoff known as zero-point length in the path integral duality literature. As a result, the static potential is found to be regular. We use this result to derive a consistent black hole metric for the spherically symmetric, electrically neutral case. It turns out that the new spacetime is regular and is formally equivalent to the Bardeen metric, apart from a different ultraviolet regulator. On the thermodynamics side, the Hawking temperature admits a maximum before a cooling down phase towards a thermodynamically stable end of the black hole evaporation process. The findings support the idea of universality of quantum black holes. Keywords: Quantum corrected black hole, String T-duality, Zero-point length, Path integral dualityhttp://www.sciencedirect.com/science/article/pii/S0370269319306021
collection DOAJ
language English
format Article
sources DOAJ
author Piero Nicolini
Euro Spallucci
Michael F. Wondrak
spellingShingle Piero Nicolini
Euro Spallucci
Michael F. Wondrak
Quantum corrected black holes from string T-duality
Physics Letters B
author_facet Piero Nicolini
Euro Spallucci
Michael F. Wondrak
author_sort Piero Nicolini
title Quantum corrected black holes from string T-duality
title_short Quantum corrected black holes from string T-duality
title_full Quantum corrected black holes from string T-duality
title_fullStr Quantum corrected black holes from string T-duality
title_full_unstemmed Quantum corrected black holes from string T-duality
title_sort quantum corrected black holes from string t-duality
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2019-10-01
description In this letter we present some stringy corrections to black hole spacetimes emerging from string T-duality. As a first step, we derive the static Newtonian potential by exploiting the relation between the T-duality and the path integral duality. We show that the intrinsic non-perturbative nature of stringy corrections introduces an ultraviolet cutoff known as zero-point length in the path integral duality literature. As a result, the static potential is found to be regular. We use this result to derive a consistent black hole metric for the spherically symmetric, electrically neutral case. It turns out that the new spacetime is regular and is formally equivalent to the Bardeen metric, apart from a different ultraviolet regulator. On the thermodynamics side, the Hawking temperature admits a maximum before a cooling down phase towards a thermodynamically stable end of the black hole evaporation process. The findings support the idea of universality of quantum black holes. Keywords: Quantum corrected black hole, String T-duality, Zero-point length, Path integral duality
url http://www.sciencedirect.com/science/article/pii/S0370269319306021
work_keys_str_mv AT pieronicolini quantumcorrectedblackholesfromstringtduality
AT eurospallucci quantumcorrectedblackholesfromstringtduality
AT michaelfwondrak quantumcorrectedblackholesfromstringtduality
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