Cosmological sector for localized mass and spin in 2+1 dimensional topologically massive gravity

dc.creatorParanjape, A. Edery M. B.
dc.date1997-08-25
dc.date.accessioned2026-07-07T12:22:40Z
dc.date.available2026-07-07T12:22:40Z
dc.descriptionThe cosmological sector to the full non-linear topologically massive gravity (TMG) is obtained for localized sources of mass $m$ and spin $σ$ besides the asymptotically spinning conical flat sector previously obtained. In a small region near but outside the sources, the metric resembles the spinning conical flat metric, but we find that the mass $m$ creates a negative deficit angle of $3m$ as opposed to $m$. Furthermore, it is not possible to recover the results of pure Einstein gravity in the limit $μ\to \infty$ unlike the flat sector.
dc.description8 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9708061
dc.identifierhttp://arxiv.org/abs/gr-qc/9708061
dc.identifierPhys.Lett.B415:344-348,1997
dc.identifierdoi:10.1016/S0370-2693(97)01221-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213728
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmological sector for localized mass and spin in 2+1 dimensional topologically massive gravity
dc.typetext

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