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Stability of the intrinsic energy vanishing in the Schwarzschild metric under slow rotation

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Stability of the intrinsic energy vanishing in the Schwarzschild metric under slow rotation

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dc.contributor.author Aguirregabiria, Juan M.
dc.contributor.author Lapiedra Civera, Ramón
dc.contributor.author Morales Lladosa, Juan Antonio
dc.date.accessioned 2019-01-16T14:31:42Z
dc.date.available 2019-01-16T14:31:42Z
dc.date.issued 2014
dc.identifier.citation Aguirregabiria, Juan M. Lapiedra Civera, Ramón Morales Lladosa, Juan Antonio 2014 Stability of the intrinsic energy vanishing in the Schwarzschild metric under slow rotation General Relativity and Gravitation 46 6 1744-1 1744-10
dc.identifier.uri http://hdl.handle.net/10550/68501
dc.description.abstract The linearized Kerr metric is considered and put in some Gauss coordinates which are further intrinsic ones. The linear and angular 4-momenta of this metric are calculated in these coordinates and the resulting value is just zero. Thus, the global vanishing previously found for the Schwarzschild metric remains linearly stable under slow rotational perturbations of this metric.
dc.language.iso eng
dc.relation.ispartof General Relativity and Gravitation, 2014, vol. 46, num. 6, p. 1744-1-1744-10
dc.subject Relativitat general (Física)
dc.subject Gravitació
dc.title Stability of the intrinsic energy vanishing in the Schwarzschild metric under slow rotation
dc.type journal article es_ES
dc.date.updated 2019-01-16T14:31:42Z
dc.identifier.doi 10.1007/s10714-014-1744-9
dc.identifier.idgrec 103890
dc.rights.accessRights open access es_ES

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