Supergravity backgrounds for deformations of AdSn×Sn supercoset string models
We consider type IIB supergravity backgrounds corresponding to the deformed AdSn×Sn×T10−2n supercoset string models of the type constructed in arXiv:1309.5850 [2] which depend on one deformation parameter κ. In AdS2×S2 case we find that the deformed metric can be extended to a full supergravity solu...
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doaj-e8e3043db2164cb4996cb250cafd12472020-11-24T23:09:59ZengElsevierNuclear Physics B0550-32132015-02-01891106127Supergravity backgrounds for deformations of AdSn×Sn supercoset string modelsO. Lunin0R. Roiban1A.A. Tseytlin2Department of Physics, University at Albany (SUNY), Albany, NY 12222, USA; Corresponding author.Department of Physics, The Pennsylvania State University, University Park, PA 16802, USA; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106, USAThe Blackett Laboratory, Imperial College, London SW7 2AZ, UKWe consider type IIB supergravity backgrounds corresponding to the deformed AdSn×Sn×T10−2n supercoset string models of the type constructed in arXiv:1309.5850 [2] which depend on one deformation parameter κ. In AdS2×S2 case we find that the deformed metric can be extended to a full supergravity solution with non-trivial dilaton, RR scalar and RR 5-form strength. The solution depends on a free parameter a that should be chosen as a particular function of κ to correspond to the deformed supercoset model. In AdS3×S3 case the full solution supported by the dilaton, RR scalar and RR 3-form strength exists only in the two special cases, a=0 and a=1. We conjecture that there may be a more general one-parameter solution supported by several RR fields that for particular a=a(κ) corresponds to the supercoset model. In the most complicated deformed AdS5×S5 case we were able to find only the expressions for the dilaton and the RR scalar. The full solution is likely to be supported by a combination of the 5-form and 3-form field strengths. We comment on the singularity structure of the resulting metric and exact dilaton field.http://www.sciencedirect.com/science/article/pii/S0550321314003757 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
O. Lunin R. Roiban A.A. Tseytlin |
spellingShingle |
O. Lunin R. Roiban A.A. Tseytlin Supergravity backgrounds for deformations of AdSn×Sn supercoset string models Nuclear Physics B |
author_facet |
O. Lunin R. Roiban A.A. Tseytlin |
author_sort |
O. Lunin |
title |
Supergravity backgrounds for deformations of AdSn×Sn supercoset string models |
title_short |
Supergravity backgrounds for deformations of AdSn×Sn supercoset string models |
title_full |
Supergravity backgrounds for deformations of AdSn×Sn supercoset string models |
title_fullStr |
Supergravity backgrounds for deformations of AdSn×Sn supercoset string models |
title_full_unstemmed |
Supergravity backgrounds for deformations of AdSn×Sn supercoset string models |
title_sort |
supergravity backgrounds for deformations of adsn×sn supercoset string models |
publisher |
Elsevier |
series |
Nuclear Physics B |
issn |
0550-3213 |
publishDate |
2015-02-01 |
description |
We consider type IIB supergravity backgrounds corresponding to the deformed AdSn×Sn×T10−2n supercoset string models of the type constructed in arXiv:1309.5850 [2] which depend on one deformation parameter κ. In AdS2×S2 case we find that the deformed metric can be extended to a full supergravity solution with non-trivial dilaton, RR scalar and RR 5-form strength. The solution depends on a free parameter a that should be chosen as a particular function of κ to correspond to the deformed supercoset model. In AdS3×S3 case the full solution supported by the dilaton, RR scalar and RR 3-form strength exists only in the two special cases, a=0 and a=1. We conjecture that there may be a more general one-parameter solution supported by several RR fields that for particular a=a(κ) corresponds to the supercoset model. In the most complicated deformed AdS5×S5 case we were able to find only the expressions for the dilaton and the RR scalar. The full solution is likely to be supported by a combination of the 5-form and 3-form field strengths. We comment on the singularity structure of the resulting metric and exact dilaton field. |
url |
http://www.sciencedirect.com/science/article/pii/S0550321314003757 |
work_keys_str_mv |
AT olunin supergravitybackgroundsfordeformationsofadsnsnsupercosetstringmodels AT rroiban supergravitybackgroundsfordeformationsofadsnsnsupercosetstringmodels AT aatseytlin supergravitybackgroundsfordeformationsofadsnsnsupercosetstringmodels |
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