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On the integrability of spherical gravitational waves in vacuum

The general class of Robinson-Trautman metrics that describe gravitational radiation in the exterior of bounded sources in four space-time dimensions is shown to admit zero curvature formulation in terms of appropriately chosen two-dimensional gauge connections. The result, which is valid for either...

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Autor principal: Bakas, Ioannis
Lenguaje:eng
Publicado: 2005
Materias:
Acceso en línea:http://cds.cern.ch/record/834084
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author Bakas, Ioannis
author_facet Bakas, Ioannis
author_sort Bakas, Ioannis
collection CERN
description The general class of Robinson-Trautman metrics that describe gravitational radiation in the exterior of bounded sources in four space-time dimensions is shown to admit zero curvature formulation in terms of appropriately chosen two-dimensional gauge connections. The result, which is valid for either type II or III metrics, implies that the gravitational analogue of the Lienard-Wiechert fields of Maxwell equations form a new integrable sector of Einstein equations for any value of the cosmological constant. The method of investigation is similar to that used for integrating the Ricci flow in two dimensions. The zero modes of the gauge symmetry (factored by the center) generate Kac's K_2 simple Lie algebra with infinite growth.
id cern-834084
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2005
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spelling cern-8340842023-03-14T19:11:46Zhttp://cds.cern.ch/record/834084engBakas, IoannisOn the integrability of spherical gravitational waves in vacuumGeneral Relativity and CosmologyThe general class of Robinson-Trautman metrics that describe gravitational radiation in the exterior of bounded sources in four space-time dimensions is shown to admit zero curvature formulation in terms of appropriately chosen two-dimensional gauge connections. The result, which is valid for either type II or III metrics, implies that the gravitational analogue of the Lienard-Wiechert fields of Maxwell equations form a new integrable sector of Einstein equations for any value of the cosmological constant. The method of investigation is similar to that used for integrating the Ricci flow in two dimensions. The zero modes of the gauge symmetry (factored by the center) generate Kac's K_2 simple Lie algebra with infinite growth.The general class of Robinson-Trautman metrics that describe gravitational radiation in the exterior of bounded sources in four space-time dimensions is shown to admit zero curvature formulation in terms of appropriately chosen two-dimensional gauge connections. The result, which is valid for either type II or III metrics, implies that the gravitational analogue of the Lienard-Wiechert fields of Maxwell equations form a new integrable sector of Einstein equations for any value of the cosmological constant. The method of investigation is similar to that used for integrating the Ricci flow in two dimensions. The zero modes of the gauge symmetry (factored by the center) generate Kac's K_2 simple Lie algebra with infinite growth.gr-qc/0504130CERN-PH-TH-2005-069CERN-PH-TH-2005-069oai:cds.cern.ch:8340842005-04-26
spellingShingle General Relativity and Cosmology
Bakas, Ioannis
On the integrability of spherical gravitational waves in vacuum
title On the integrability of spherical gravitational waves in vacuum
title_full On the integrability of spherical gravitational waves in vacuum
title_fullStr On the integrability of spherical gravitational waves in vacuum
title_full_unstemmed On the integrability of spherical gravitational waves in vacuum
title_short On the integrability of spherical gravitational waves in vacuum
title_sort on the integrability of spherical gravitational waves in vacuum
topic General Relativity and Cosmology
url http://cds.cern.ch/record/834084
work_keys_str_mv AT bakasioannis ontheintegrabilityofsphericalgravitationalwavesinvacuum