Gravitational waves about curved backgrounds: a consistency analysis in de Sitter spacetime

dc.creatorBini, Donato
dc.creatorCapozziello, Salvatore
dc.creatorEsposito, Giampiero
dc.date2008-05-05
dc.date2008-12-21
dc.date.accessioned2026-07-07T12:20:39Z
dc.date.available2026-07-07T12:20:39Z
dc.descriptionGravitational waves are considered as metric perturbations about a curved background metric, rather than the flat Minkowski metric since several situations of physical interest can be discussed by this generalization. In this case, when the de Donder gauge is imposed, its preservation under infinitesimal spacetime diffeomorphisms is guaranteed if and only if the associated covector is ruled by a second-order hyperbolic operator which is the classical counterpart of the ghost operator in quantum gravity. In such a wave equation, the Ricci term has opposite sign with respect to the wave equation for Maxwell theory in the Lorenz gauge. We are, nevertheless, able to relate the solutions of the two problems, and the algorithm is applied to the case when the curved background geometry is the de Sitter spacetime. Such vector wave equations are studied in two different ways: i) an integral representation, ii) through a solution by factorization of the hyperbolic equation. The latter method is extended to the wave equation of metric perturbations in the de Sitter spacetime. This approach is a step towards a general discussion of gravitational waves in the de Sitter spacetime and might assume relevance in cosmology in order to study the stochastic background emerging from inflation.
dc.description17 pages. Misprints amended in Eqs. 50, 54, 55, 75, 76
dc.identifierhttps://arxiv.org/abs/0805.0486
dc.identifierhttp://arxiv.org/abs/0805.0486
dc.identifierInt.J.Geom.Meth.Mod.Phys.5:1069-1083,2008
dc.identifierdoi:10.1142/S0219887808003211
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213124
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waves about curved backgrounds: a consistency analysis in de Sitter spacetime
dc.typetext

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