Cosmological constant, near brane behavior and singularities
Cosmological constant, near brane behavior and singularities
We show that the classical cosmological constant in type II flux compactifications can be written as a sum of terms from the action of localized sources plus a specific contribution from non-trivial background fluxes. Exploiting two global scaling symmetries of the classical supergravity action, we find that the flux contribution can in many interesting cases be set to zero such that the cosmological constant is fully determined by the boundary conditions of the fields in the near-source region. This generalizes and makes more explicit previous arguments in the literature. We then discuss the problem of putting -branes at the tip of the Klebanov-Strassler throat glued to a compact space in type IIB string theory so as to engineer a de Sitter solution. Our result for the cosmological constant and a simple global argument indicate that inserting a fully localized and backreacting -brane into such a background yields a singular energy density for the NSNS and RR 3-form field strengths at the -brane. This argument does not rely on partial smearing of the -brane or a linearization of field equations, but on a few general assumptions that we also discuss carefully.
Gautason, Fridrik Freyr
0c48d448-e092-48bf-a310-45862bd6fc5f
Junghans, Daniel
72aa7aa8-dbba-48ee-a35d-8deead944975
Zagermann, Marco
547e40b6-e2d0-4c56-bd2d-1de1341b53b9
2013
Gautason, Fridrik Freyr
0c48d448-e092-48bf-a310-45862bd6fc5f
Junghans, Daniel
72aa7aa8-dbba-48ee-a35d-8deead944975
Zagermann, Marco
547e40b6-e2d0-4c56-bd2d-1de1341b53b9
Gautason, Fridrik Freyr, Junghans, Daniel and Zagermann, Marco
(2013)
Cosmological constant, near brane behavior and singularities.
JHEP, 2013, [123].
(doi:10.1007/JHEP09(2013)123).
Abstract
We show that the classical cosmological constant in type II flux compactifications can be written as a sum of terms from the action of localized sources plus a specific contribution from non-trivial background fluxes. Exploiting two global scaling symmetries of the classical supergravity action, we find that the flux contribution can in many interesting cases be set to zero such that the cosmological constant is fully determined by the boundary conditions of the fields in the near-source region. This generalizes and makes more explicit previous arguments in the literature. We then discuss the problem of putting -branes at the tip of the Klebanov-Strassler throat glued to a compact space in type IIB string theory so as to engineer a de Sitter solution. Our result for the cosmological constant and a simple global argument indicate that inserting a fully localized and backreacting -brane into such a background yields a singular energy density for the NSNS and RR 3-form field strengths at the -brane. This argument does not rely on partial smearing of the -brane or a linearization of field equations, but on a few general assumptions that we also discuss carefully.
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Accepted/In Press date: 23 January 2013
Published date: 2013
Identifiers
Local EPrints ID: 497174
URI: http://eprints.soton.ac.uk/id/eprint/497174
ISSN: 1126-6708
PURE UUID: 95bf53b3-34e7-475f-993c-c7932a54d102
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Date deposited: 15 Jan 2025 17:53
Last modified: 08 Feb 2025 03:17
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Author:
Fridrik Freyr Gautason
Author:
Daniel Junghans
Author:
Marco Zagermann
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