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Open AccessArticle

Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies

1
Department of Physics, Umeå University, 901 87 Umeå, Sweden
2
Department of Theoretical Physics, University of Szeged, Tisza Lajos krt 84-86, Szeged 6720, Hungary
3
Department of Experimental Physics, University of Szeged, Dóm Tér 9, Szeged 6720, Hungary
*
Author to whom correspondence should be addressed.
Universe 2017, 3(4), 69; https://doi.org/10.3390/universe3040069
Received: 28 August 2017 / Revised: 15 September 2017 / Accepted: 26 September 2017 / Published: 2 October 2017
(This article belongs to the Special Issue Gravitational Waves: Prospects after the First Direct Detections)
In this work we consider perturbations of homogeneous and hypersurface orthogonal cosmological backgrounds with local rotational symmetry (LRS), using a method based on the 1 + 1 + 2 covariant split of spacetime. The backgrounds, of LRS class II, are characterised by that the vorticity, the twist of the 2-sheets, and the magnetic part of the Weyl tensor all vanish. They include the flat Friedmann universe as a special case. The matter contents of the perturbed spacetimes are given by vorticity-free perfect fluids, but otherwise the perturbations are arbitrary and describe gravitational, shear, and density waves. All the perturbation variables can be given in terms of the time evolution of a set of six harmonic coefficients. This set decouples into one set of four coefficients with the density perturbations acting as source terms, and another set of two coefficients describing damped source-free gravitational waves with odd parity. We also consider the flat Friedmann universe, which has been considered by several others using the 1 + 3 covariant split, as a check of the isotropic limit. In agreement with earlier results we find a second-order wavelike equation for the magnetic part of the Weyl tensor which decouples from the density gradient for the flat Friedmann universes. Assuming vanishing vector perturbations, including the density gradient, we find a similar equation for the electric part of the Weyl tensor, which was previously unnoticed. View Full-Text
Keywords: cosmology; covariant split; perturbation theory; gravitational waves cosmology; covariant split; perturbation theory; gravitational waves
MDPI and ACS Style

Bradley, M.; Forsberg, M.; Keresztes, Z. Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies. Universe 2017, 3, 69. https://doi.org/10.3390/universe3040069

AMA Style

Bradley M, Forsberg M, Keresztes Z. Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies. Universe. 2017; 3(4):69. https://doi.org/10.3390/universe3040069

Chicago/Turabian Style

Bradley, Michael; Forsberg, Mats; Keresztes, Zoltán. 2017. "Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies" Universe 3, no. 4: 69. https://doi.org/10.3390/universe3040069

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