Purely radiative irrotational dust spacetimes

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dc.creatorBergh, N Van den
dc.creatorBastiaensen, B
dc.creatorKarimian, H R
dc.creatorWylleman, L
dc.date2006-11-14
dc.date2007-02-27
dc.date.accessioned2026-07-07T11:43:06Z
dc.date.available2026-07-07T11:43:06Z
dc.descriptionWe consider irrotational dust spacetimes in the full non-linear regime which are "purely radiative" in the sense that the gravitational field satisfies the covariant transverse conditions div(H) = div(E) = 0. Within this family we show that the Bianchi class A spatially homogeneous dust models are uniquely characterised by the condition that $H$ is diagonal in the shear-eigenframe.
dc.description6 pages, ERE 2006 conference, minor corrections
dc.identifierhttps://arxiv.org/abs/gr-qc/0611079
dc.identifierhttp://arxiv.org/abs/gr-qc/0611079
dc.identifierJ.Phys.Conf.Ser.66:012023,2007
dc.identifierdoi:10.1088/1742-6596/66/1/012023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201117
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePurely radiative irrotational dust spacetimes
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