A Microscopic Limit on Gravitational Waves from D-brane Inflation

dc.creatorBaumann, Daniel
dc.creatorMcAllister, Liam
dc.date2006-10-26
dc.date.accessioned2026-07-07T10:26:08Z
dc.date.available2026-07-07T10:26:08Z
dc.descriptionWe derive a microscopic bound on the maximal field variation of the inflaton during warped D-brane inflation. By a result of Lyth, this implies an upper limit on the amount of gravitational waves produced during inflation. We show that a detection at the level $r > 0.01$ would falsify slow roll D-brane inflation. In DBI inflation, detectable tensors may be possible in special compactifications, provided that $r$ decreases rapidly during inflation. We also show that for the special case of DBI inflation with a quadratic potential, current observational constraints imply strong upper bounds on the five-form flux.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0610285
dc.identifierhttp://arxiv.org/abs/hep-th/0610285
dc.identifierPhys.Rev.D75:123508,2007
dc.identifierdoi:10.1103/PhysRevD.75.123508
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176775
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleA Microscopic Limit on Gravitational Waves from D-brane Inflation
dc.typetext

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