Self-tuning Solution of Cosmological Constant in RS-II Model and Goldstone Boson

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dc.creatorKim, Jihn E.
dc.date2001-12-28
dc.date2002-01-09
dc.date.accessioned2026-07-07T03:46:14Z
dc.date.available2026-07-07T03:46:14Z
dc.descriptionI 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.
dc.description11 pages including 7 eps figures, talk presented at COSMO-01, Rovaniemi, Finland, Aug. 29 - Sep. 4, 2001. Typos corrected
dc.identifierhttps://arxiv.org/abs/hep-ph/0112344
dc.identifierhttp://arxiv.org/abs/hep-ph/0112344
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41208
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSelf-tuning Solution of Cosmological Constant in RS-II Model and Goldstone Boson
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