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Brane singularities and their avoidance
The singularity structure and the corresponding asymptotic behavior of a 3-brane coupled to a scalar field or to a perfect fluid in a five-dimensional bulk is analyzed in full generality using the method of asymptotic splittings. In the case of the scalar field, it is shown that the collapse singula...
Autores principales: | , , |
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Formato: | info:eu-repo/semantics/article |
Lenguaje: | eng |
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Class. Quantum Gravity
2010
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/27/23/235018 http://cds.cern.ch/record/1303738 |
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author | Antoniadis, Ignatios Cotsakis, Spiros Klaoudatou, Ifigeneia |
author_facet | Antoniadis, Ignatios Cotsakis, Spiros Klaoudatou, Ifigeneia |
author_sort | Antoniadis, Ignatios |
collection | CERN |
description | The singularity structure and the corresponding asymptotic behavior of a 3-brane coupled to a scalar field or to a perfect fluid in a five-dimensional bulk is analyzed in full generality using the method of asymptotic splittings. In the case of the scalar field, it is shown that the collapse singularity at a finite distance from the brane can be avoided only at the expense of making the brane world-volume positively or negatively curved. In the case where the bulk field content is parametrized by an analogue of perfect fluid with an arbitrary equation of state P=\gamma\rho between the `pressure' P and the `density' \rho, our results depend crucially on the constant fluid parameter \gamma: (i) For \gamma>-1/2, the flat brane solution suffers from a collapse singularity at finite distance, that disappears in the curved case. (ii) For \gamma<-1, the singularity cannot be avoided and it becomes of the big rip type for a flat brane. (iii) For -1<\gamma< or = -1/2, the surprising result is found that while the curved brane solution is singular, the flat brane is not, opening the possibility for a revival of the self-tuning proposal. |
format | info:eu-repo/semantics/article |
id | cern-1303738 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2010 |
publisher | Class. Quantum Gravity |
record_format | invenio |
spelling | cern-13037382023-03-15T19:12:06Z doi:10.1088/0264-9381/27/23/235018 http://cds.cern.ch/record/1303738 eng Antoniadis, Ignatios Cotsakis, Spiros Klaoudatou, Ifigeneia Brane singularities and their avoidance General Relativity and Cosmology The singularity structure and the corresponding asymptotic behavior of a 3-brane coupled to a scalar field or to a perfect fluid in a five-dimensional bulk is analyzed in full generality using the method of asymptotic splittings. In the case of the scalar field, it is shown that the collapse singularity at a finite distance from the brane can be avoided only at the expense of making the brane world-volume positively or negatively curved. In the case where the bulk field content is parametrized by an analogue of perfect fluid with an arbitrary equation of state P=\gamma\rho between the `pressure' P and the `density' \rho, our results depend crucially on the constant fluid parameter \gamma: (i) For \gamma>-1/2, the flat brane solution suffers from a collapse singularity at finite distance, that disappears in the curved case. (ii) For \gamma<-1, the singularity cannot be avoided and it becomes of the big rip type for a flat brane. (iii) For -1<\gamma< or = -1/2, the surprising result is found that while the curved brane solution is singular, the flat brane is not, opening the possibility for a revival of the self-tuning proposal. The singularity structure and the corresponding asymptotic behavior of a 3-brane coupled to a scalar field or to a perfect fluid in a five-dimensional bulk is analyzed in full generality using the method of asymptotic splittings. In the case of the scalar field, it is shown that the collapse singularity at a finite distance from the brane can be avoided only at the expense of making the brane world-volume positively or negatively curved. In the case where the bulk field content is parametrized by an analogue of perfect fluid with an arbitrary equation of state P=\gamma\rho between the `pressure' P and the `density' \rho, our results depend crucially on the constant fluid parameter \gamma: (i) For \gamma>-1/2, the flat brane solution suffers from a collapse singularity at finite distance, that disappears in the curved case. (ii) For \gamma<-1, the singularity cannot be avoided and it becomes of the big rip type for a flat brane. (iii) For -1<\gamma< or = -1/2, the surprising result is found that while the curved brane solution is singular, the flat brane is not, opening the possibility for a revival of the self-tuning proposal. info:eu-repo/grantAgreement/EC/FP7/226371 info:eu-repo/semantics/openAccess Education Level info:eu-repo/semantics/article http://cds.cern.ch/record/1303738 Class. Quantum Gravity Class. Quantum Gravity, (2010) pp. 235018 2010-11-01 |
spellingShingle | General Relativity and Cosmology Antoniadis, Ignatios Cotsakis, Spiros Klaoudatou, Ifigeneia Brane singularities and their avoidance |
title | Brane singularities and their avoidance |
title_full | Brane singularities and their avoidance |
title_fullStr | Brane singularities and their avoidance |
title_full_unstemmed | Brane singularities and their avoidance |
title_short | Brane singularities and their avoidance |
title_sort | brane singularities and their avoidance |
topic | General Relativity and Cosmology |
url | https://dx.doi.org/10.1088/0264-9381/27/23/235018 http://cds.cern.ch/record/1303738 http://cds.cern.ch/record/1303738 |
work_keys_str_mv | AT antoniadisignatios branesingularitiesandtheiravoidance AT cotsakisspiros branesingularitiesandtheiravoidance AT klaoudatouifigeneia branesingularitiesandtheiravoidance |