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On the Evaporation of Black Holes in String Theory

We show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known t...

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Detalles Bibliográficos
Autores principales: Ellis, John R., Mavromatos, N.E., Nanopoulos, Dimitri V.
Lenguaje:eng
Publicado: 1992
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0370-2693(92)90541-B
http://cds.cern.ch/record/227327
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author Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
author_facet Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
author_sort Ellis, John R.
collection CERN
description We show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known to express the instabilities of massive string states in general, and are not thermal in character. The absence of such imaginary parts in the matrix model limit confirms that the latter constitutes the final stage of the evaporation process, at least in perturbation theory. Our arguments appear to be quite generic, related only to the summation over world-sheet surfaces, and hence should also apply to higher-dimensional target spaces.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1992
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spelling cern-2273272023-03-14T17:13:26Zdoi:10.1016/0370-2693(92)90541-Bhttp://cds.cern.ch/record/227327engEllis, John R.Mavromatos, N.E.Nanopoulos, Dimitri V.On the Evaporation of Black Holes in String TheoryParticle Physics - TheoryWe show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known to express the instabilities of massive string states in general, and are not thermal in character. The absence of such imaginary parts in the matrix model limit confirms that the latter constitutes the final stage of the evaporation process, at least in perturbation theory. Our arguments appear to be quite generic, related only to the summation over world-sheet surfaces, and hence should also apply to higher-dimensional target spaces.We show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known to express the instabilities of massive string states in general, and are not thermal in character. The absence of such imaginary parts in the matrix model limit confirms that the latter constitutes the final stage of the evaporation process, at least in perturbation theory. Our arguments appear to be quite generic, related only to the summation over world-sheet surfaces, and hence should also apply to higher-dimensional target spaces.We show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known to express the instabilities of massive string states in general, and are not thermal in character. The absence of such imaginary parts in the matrix model limit confirms that the latter constitutes the final stage of the evaporation process, at least in perturbation theory. Our arguments appear to be quite generic, related only to the summation over world-sheet surfaces, and hence should also apply to higher-dimensional target spaces.We show that, in string theory, the quantum evaporation and decay of black holes in two-dimensional target space is related to imaginary parts in higher-genus string amplitudes. These arise from the regularisation of modular infinities due to the sum over world-sheet configurations, that are known to express the instabilities of massive string states in general, and are not thermal in character. The absence of such imaginary parts in the matrix-model limit confirms that the latter constitutes the final stage of the evaporation process, at least in perturbation theory. Our arguments appear to be quite generic, related only to the summation over world-sheet surfaces, and hence should also apply to higher-dimensional target spaces.hep-th/9111031CTP-TAMU-90-91CERN-TH-6309-91ACT-53ACT-53CERN-TH-6309-91CTP-TAMU-90-91oai:cds.cern.ch:2273271992
spellingShingle Particle Physics - Theory
Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
On the Evaporation of Black Holes in String Theory
title On the Evaporation of Black Holes in String Theory
title_full On the Evaporation of Black Holes in String Theory
title_fullStr On the Evaporation of Black Holes in String Theory
title_full_unstemmed On the Evaporation of Black Holes in String Theory
title_short On the Evaporation of Black Holes in String Theory
title_sort on the evaporation of black holes in string theory
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/0370-2693(92)90541-B
http://cds.cern.ch/record/227327
work_keys_str_mv AT ellisjohnr ontheevaporationofblackholesinstringtheory
AT mavromatosne ontheevaporationofblackholesinstringtheory
AT nanopoulosdimitriv ontheevaporationofblackholesinstringtheory