Quantum corrections and extremal black holes
We consider static solutions of two dimensional dilaton gravity models as toy laboratories to address the question of the final fate of black holes. A nonperturbative correction to the CGHS potential tern is shown to lead classically to an extremal black hole geometry, thus providing a plausible sol...
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1995
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v355_n1-2_p92_Alejandro http://hdl.handle.net/20.500.12110/paper_03702693_v355_n1-2_p92_Alejandro |
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paper:paper_03702693_v355_n1-2_p92_Alejandro2023-06-08T15:36:34Z Quantum corrections and extremal black holes Alejandro, Gabriela Mazzitelli, Francisco Diego Nuñez, Carmen Alicia We consider static solutions of two dimensional dilaton gravity models as toy laboratories to address the question of the final fate of black holes. A nonperturbative correction to the CGHS potential tern is shown to lead classically to an extremal black hole geometry, thus providing a plausible solution to the Hawking evaporation paradox. However, the full quantum theory does not admit an extremal solution. © 1995. Fil:Alejandro, G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mazzitelli, F.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Núñez, C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 1995 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v355_n1-2_p92_Alejandro http://hdl.handle.net/20.500.12110/paper_03702693_v355_n1-2_p92_Alejandro |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
We consider static solutions of two dimensional dilaton gravity models as toy laboratories to address the question of the final fate of black holes. A nonperturbative correction to the CGHS potential tern is shown to lead classically to an extremal black hole geometry, thus providing a plausible solution to the Hawking evaporation paradox. However, the full quantum theory does not admit an extremal solution. © 1995. |
author |
Alejandro, Gabriela Mazzitelli, Francisco Diego Nuñez, Carmen Alicia |
spellingShingle |
Alejandro, Gabriela Mazzitelli, Francisco Diego Nuñez, Carmen Alicia Quantum corrections and extremal black holes |
author_facet |
Alejandro, Gabriela Mazzitelli, Francisco Diego Nuñez, Carmen Alicia |
author_sort |
Alejandro, Gabriela |
title |
Quantum corrections and extremal black holes |
title_short |
Quantum corrections and extremal black holes |
title_full |
Quantum corrections and extremal black holes |
title_fullStr |
Quantum corrections and extremal black holes |
title_full_unstemmed |
Quantum corrections and extremal black holes |
title_sort |
quantum corrections and extremal black holes |
publishDate |
1995 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v355_n1-2_p92_Alejandro http://hdl.handle.net/20.500.12110/paper_03702693_v355_n1-2_p92_Alejandro |
work_keys_str_mv |
AT alejandrogabriela quantumcorrectionsandextremalblackholes AT mazzitellifranciscodiego quantumcorrectionsandextremalblackholes AT nunezcarmenalicia quantumcorrectionsandextremalblackholes |
_version_ |
1768546211852189696 |