Self-tuning of the cosmological constant and Einstein Gravity on the brane

Simple item page
dc.creatorKim, Jihn E.
dc.creatorKyae, Bumseok
dc.creatorShafi, Qaisar
dc.date2004-02-10
dc.date.accessioned2026-07-07T03:52:01Z
dc.date.available2026-07-07T03:52:01Z
dc.descriptionWe show that a self-tuning mechanism of the cosmological constant could work in 5D non-compact space-time. The standard model matter fields live only on the 4D brane. The change of vacuum energy on the brane just gives rise to dynamical shifts of the profiles of the background metric and a bulk scalar field in the extra dimension, keeping 4D space-time flat. To obtain the Newtonian potential on the brane, we introduce an additional brane-localized 4D Einstein-Hilbert term.
dc.descriptionTalk presented by B. Kyae at SUSY 2003: Supersymmetry in the Desert, held at the University of Arizona, Tucson, AZ, June 5-10, 2003. To appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/hep-ph/0402111
dc.identifierhttp://arxiv.org/abs/hep-ph/0402111
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43314
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSelf-tuning of the cosmological constant and Einstein Gravity on the brane
dc.typetext

Files

Collections

arXiv