Inflationary Hubble Parameter from the Gravitational Wave Spectrum in the General Slow-roll Approximation

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dc.creatorJoy, Minu
dc.date2007-09-20
dc.date.accessioned2026-07-07T13:13:14Z
dc.date.available2026-07-07T13:13:14Z
dc.descriptionImproved general slow-roll formulae giving the primordial gravitational wave spectrum are derived in the present work. Also the first and second order general slow-roll inverse formulae giving the Hubble parameter $H$ in terms of the gravitational wave spectrum are derived. Moreover, the general slow-roll consistency condition relating the scalar and tensor spectra is obtained.
dc.identifierhttps://arxiv.org/abs/0709.3211
dc.identifierhttp://arxiv.org/abs/0709.3211
dc.identifierJCAP 0709:019,2007
dc.identifierdoi:10.1088/1475-7516/2007/09/019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229824
dc.subjectAstrophysics
dc.titleInflationary Hubble Parameter from the Gravitational Wave Spectrum in the General Slow-roll Approximation
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