Self-tuning Solution of Cosmological Constant in RS-II Model and Goldstone Boson
I give a review on the self-tuning solution of the cosmological constant in a 5D RS-II model using a three index antisymmetric tensor field $A_{MNP}$. The three index antisymmetric tensor field can be the fundamental one appearing in 11D supergravity. Also, the dual of its field strength $H_{MNPQ}$,...
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| Format: | Report |
| Language: | unknown |
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arXiv
2001
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| Online Access: | https://dx.doi.org/10.48550/arxiv.hep-ph/0112344 https://arxiv.org/abs/hep-ph/0112344 |
| Summary: | I give a review on the self-tuning solution of the cosmological constant in a 5D RS-II model using a three index antisymmetric tensor field $A_{MNP}$. The three index antisymmetric tensor field can be the fundamental one appearing in 11D supergravity. Also, the dual of its field strength $H_{MNPQ}$, being a massless scalar, may be interpreted as a Goldstone boson of some spontaneously broken global symmetry. : 11 pages including 7 eps figures, talk presented at COSMO-01, Rovaniemi, Finland, Aug. 29 - Sep. 4, 2001. Typos corrected |
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