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d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms

We generalize the description of the d=4 Attractor Mechanism based on an effective black hole (BH) potential to the presence of a gauging which does not modify the derivatives of the scalars and does not involve hypermultiplets. The obtained results do not rely necessarily on supersymmetry, and they...

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Detalles Bibliográficos
Autores principales: Bellucci, S, Ferrara, Sergio, Marrani, A, Yeranyan, A
Lenguaje:eng
Publicado: 2008
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.77.085027
http://cds.cern.ch/record/1083979
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author Bellucci, S
Ferrara, Sergio
Marrani, A
Yeranyan, A
author_facet Bellucci, S
Ferrara, Sergio
Marrani, A
Yeranyan, A
author_sort Bellucci, S
collection CERN
description We generalize the description of the d=4 Attractor Mechanism based on an effective black hole (BH) potential to the presence of a gauging which does not modify the derivatives of the scalars and does not involve hypermultiplets. The obtained results do not rely necessarily on supersymmetry, and they can be extended to d>4, as well. Thence, we work out the example of the stu model of N=2 supergravity in the presence of Fayet-Iliopoulos terms, for the supergravity analogues of the magnetic and D0-D6 BH charge configurations, and in three different symplectic frames: the SO(1,1)^{2}, SO(2,2) covariant and SO(8)-truncated ones. The attractive nature of the critical points, related to the semi-positive definiteness of the Hessian matrix, is also studied.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2008
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spelling cern-10839792019-09-30T06:29:59Zdoi:10.1103/PhysRevD.77.085027http://cds.cern.ch/record/1083979engBellucci, SFerrara, SergioMarrani, AYeranyan, Ad=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos TermsParticle Physics - TheoryWe generalize the description of the d=4 Attractor Mechanism based on an effective black hole (BH) potential to the presence of a gauging which does not modify the derivatives of the scalars and does not involve hypermultiplets. The obtained results do not rely necessarily on supersymmetry, and they can be extended to d>4, as well. Thence, we work out the example of the stu model of N=2 supergravity in the presence of Fayet-Iliopoulos terms, for the supergravity analogues of the magnetic and D0-D6 BH charge configurations, and in three different symplectic frames: the SO(1,1)^{2}, SO(2,2) covariant and SO(8)-truncated ones. The attractive nature of the critical points, related to the semi-positive definiteness of the Hessian matrix, is also studied.arXiv:0802.0141CERN-PH-TH-2008-020oai:cds.cern.ch:10839792008-02-04
spellingShingle Particle Physics - Theory
Bellucci, S
Ferrara, Sergio
Marrani, A
Yeranyan, A
d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title_full d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title_fullStr d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title_full_unstemmed d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title_short d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
title_sort d=4 black hole attractors in n=2 supergravity with fayet-iliopoulos terms
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.77.085027
http://cds.cern.ch/record/1083979
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AT ferrarasergio d4blackholeattractorsinn2supergravitywithfayetiliopoulosterms
AT marrania d4blackholeattractorsinn2supergravitywithfayetiliopoulosterms
AT yeranyana d4blackholeattractorsinn2supergravitywithfayetiliopoulosterms