Holonomy corrections to the cosmological primordial tensor power spectrum

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dc.creatorBarrau, A.
dc.creatorGrain, J.
dc.date2008-05-03
dc.date.accessioned2026-07-07T09:36:53Z
dc.date.available2026-07-07T09:36:53Z
dc.descriptionLoop quantum gravity is one of the leading candidate theory to non-perturbatively quantize gravity. In this framework, holonomy corrections to the equation of propagation of gravitons in a FLRW background have been derived. We investigate the consequences of those corrections on the tensor power spectrum in de-Sitter and slow-roll inflations, for n=-1/2. Depending on the value of the Barbero-Immirzi parameter, several observational features could be expected.
dc.description5 pages, Proc. of the 43rd Rencontres de Moriond "Cosmology 2008"
dc.identifierhttps://arxiv.org/abs/0805.0356
dc.identifierhttp://arxiv.org/abs/0805.0356
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160278
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleHolonomy corrections to the cosmological primordial tensor power spectrum
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