A note on dark energy induced by D-brane motion

Simple item page
dc.creatorChingangbam, R.
dc.creatorDeshamukhya, A.
dc.date2008-07-15
dc.date.accessioned2026-07-07T12:54:04Z
dc.date.available2026-07-07T12:54:04Z
dc.descriptionIn this note we study the possibility of obtaining dark energy solution in a D-brane scenario in a warped background that includes brane-position dependent corrections for the non-perturbative superpotential. The volume modulus is stabilized at instantaneous minima of the potential. Though the model can account for the existence of dark energy within present observational bound - fine-tuning of the model parameters becomes unavoidable. Moreover, the model does not posses a tracker solution.
dc.description5 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/0807.2317
dc.identifierhttp://arxiv.org/abs/0807.2317
dc.identifierInt.J.Mod.Phys.D17:2577-2583,2009
dc.identifierdoi:10.1142/S0218271808014199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223803
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA note on dark energy induced by D-brane motion
dc.typetext

Files

Collections

arXiv