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A cigar-like Universe

We study the localization of gravity on a string-like topological defect within a 6-dimensional space-time. Assuming zero cosmological constant we find complete numerical solutions to a set of first-order, Bogomol'nyi-Prasad-Sommeferld (BPS)-like, equations for the metric and the scalar field,...

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Detalles Bibliográficos
Autores principales: de Carlos, B., Moreno, J.M.
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2003/11/040
http://cds.cern.ch/record/645419
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author de Carlos, B.
Moreno, J.M.
author_facet de Carlos, B.
Moreno, J.M.
author_sort de Carlos, B.
collection CERN
description We study the localization of gravity on a string-like topological defect within a 6-dimensional space-time. Assuming zero cosmological constant we find complete numerical solutions to a set of first-order, Bogomol'nyi-Prasad-Sommeferld (BPS)-like, equations for the metric and the scalar field, where the dynamics of the latter are dictated by a supergravity-type potential. Our axially symmetric solutions have no deficit angle and factorize as $AdS_5 \times S_1 $ far from the core. They are regular everywhere, providing complete smooth cigar-like geometries. The total energy of these configurations depends only on the boundary conditions for the warp factor and it is shown to vanish.
id cern-645419
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
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spelling cern-6454192023-03-14T18:16:27Zdoi:10.1088/1126-6708/2003/11/040http://cds.cern.ch/record/645419engde Carlos, B.Moreno, J.M.A cigar-like UniverseParticle Physics - TheoryWe study the localization of gravity on a string-like topological defect within a 6-dimensional space-time. Assuming zero cosmological constant we find complete numerical solutions to a set of first-order, Bogomol'nyi-Prasad-Sommeferld (BPS)-like, equations for the metric and the scalar field, where the dynamics of the latter are dictated by a supergravity-type potential. Our axially symmetric solutions have no deficit angle and factorize as $AdS_5 \times S_1 $ far from the core. They are regular everywhere, providing complete smooth cigar-like geometries. The total energy of these configurations depends only on the boundary conditions for the warp factor and it is shown to vanish.We study the localization of gravity on a string-like topological defect within a 6-dimensional space-time. Assuming zero cosmological constant we find complete numerical solutions to a set of first-order, Bogomol'nyi-Prasad-Sommeferld (BPS)-like, equations for the metric and the scalar field, where the dynamics of the latter are dictated by a supergravity-type potential. Our axially symmetric solutions have no deficit angle and factorize as $AdS_5 \times S_1 $ far from the core. They are regular everywhere, providing complete smooth cigar-like geometries. The total energy of these configurations depends only on the boundary conditions for the warp factor and it is shown to vanish.hep-th/0309259SUSX-TH-03-011CERN-TH-2003-218IEM-FT-232-03IFT-UAM-CSIC-03-36CERN-TH-2003-218IEM-FT-232-2003IFT-UAM-CSIC-2003-36SUSX-TH-2003-011oai:cds.cern.ch:6454192003-09-29
spellingShingle Particle Physics - Theory
de Carlos, B.
Moreno, J.M.
A cigar-like Universe
title A cigar-like Universe
title_full A cigar-like Universe
title_fullStr A cigar-like Universe
title_full_unstemmed A cigar-like Universe
title_short A cigar-like Universe
title_sort cigar-like universe
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1126-6708/2003/11/040
http://cds.cern.ch/record/645419
work_keys_str_mv AT decarlosb acigarlikeuniverse
AT morenojm acigarlikeuniverse
AT decarlosb cigarlikeuniverse
AT morenojm cigarlikeuniverse