stu Black Holes Unveiled

The general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing central charge Z and for Z=0, are obtained for the so-called stu model, the minimal rank-3 N=2 symmetric supergravity in d=4 space-time dimensions. Comparisons with previous res...

Descripción completa

Detalles Bibliográficos
Autores principales: Bellucci, Stefano, Ferrara, Sergio, Marrani, Alessio, Yeranyan, Armen
Lenguaje:eng
Publicado: 2008
Materias:
Particle Physics - Theory
Acceso en línea:https://dx.doi.org/10.3390/e10040507
http://cds.cern.ch/record/1116774
_version_ 1780914429197549568
author Bellucci, Stefano
Ferrara, Sergio
Marrani, Alessio
Yeranyan, Armen
author_facet Bellucci, Stefano
Ferrara, Sergio
Marrani, Alessio
Yeranyan, Armen
author_sort Bellucci, Stefano
collection CERN
description The general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing central charge Z and for Z=0, are obtained for the so-called stu model, the minimal rank-3 N=2 symmetric supergravity in d=4 space-time dimensions. Comparisons with previous results, as well as the fake supergravity (first order) formalism and an analysis of the BPS bound all along the non-BPS attractor flows and of the marginal stability of corresponding D-brane configurations, are given.
id cern-1116774
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2008
record_format invenio
spelling cern-11167742023-03-14T16:47:23Zdoi:10.3390/e10040507http://cds.cern.ch/record/1116774engBellucci, StefanoFerrara, SergioMarrani, AlessioYeranyan, Armenstu Black Holes UnveiledParticle Physics - TheoryThe general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing central charge Z and for Z=0, are obtained for the so-called stu model, the minimal rank-3 N=2 symmetric supergravity in d=4 space-time dimensions. Comparisons with previous results, as well as the fake supergravity (first order) formalism and an analysis of the BPS bound all along the non-BPS attractor flows and of the marginal stability of corresponding D-brane configurations, are given.The general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing central charge Z and for Z=0, are obtained for the so-called stu model, the minimal rank-3 N=2 symmetric supergravity in d=4 space-time dimensions. Comparisons with previous results, as well as the fake supergravity (first order) formalism and an analysis of the BPS bound all along the non-BPS attractor flows and of the marginal stability of corresponding D-brane configurations, are given.arXiv:0807.3503CERN-PH-TH-2008-158UCB-PTH-08-73SU-ITP-08-28CERN-PH-TH-2008-158oai:cds.cern.ch:11167742008-07-23
spellingShingle Particle Physics - Theory
Bellucci, Stefano
Ferrara, Sergio
Marrani, Alessio
Yeranyan, Armen
stu Black Holes Unveiled
title stu Black Holes Unveiled
title_full stu Black Holes Unveiled
title_fullStr stu Black Holes Unveiled
title_full_unstemmed stu Black Holes Unveiled
title_short stu Black Holes Unveiled
title_sort stu black holes unveiled
topic Particle Physics - Theory
url https://dx.doi.org/10.3390/e10040507
http://cds.cern.ch/record/1116774
work_keys_str_mv AT belluccistefano stublackholesunveiled
AT ferrarasergio stublackholesunveiled
AT marranialessio stublackholesunveiled
AT yeranyanarmen stublackholesunveiled

Ejemplares similares