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Einstein gravity with torsion induced by the scalar field

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dc.contributor.authorOzcelik, H. T.
dc.contributor.authorKaya, R.
dc.contributor.authorHortacsu, M.
dc.date.accessioned2026-06-27T14:14:12Z
dc.date.issued2018
dc.description.abstractWe couple a conformal scalar field in (2+1) dimensions to Einstein gravity with torsion. The field equations are obtained by a variational principle. We could not solve the Einstein and Cartan equations analytically. These equations are solved numerically with 4th order Runge-Kutta method. From the numerical solution, we make an ansatz for the rotation parameter in the proposed metric, which gives an analytical solution for the scalar field for asymptotic regions. (C) 2018 Elsevier Inc. All rights reserved.en
dc.description.urihttps://doi.org/10.1016/j.aop.2018.04.012
dc.identifier.doi10.1016/j.aop.2018.04.012
dc.identifier.eissn1096-035X
dc.identifier.endpage144
dc.identifier.issn0003-4916
dc.identifier.startpage132
dc.identifier.urihttps://hdl.handle.net/20.500.14981/58281
dc.identifier.volume393
dc.identifier.wos000435430900007
dc.language.isoeng
dc.publisherACADEMIC PRESS INC ELSEVIER SCIENCE
dc.relation.ispartofANNALS OF PHYSICS
dc.rightsopenAccess
dc.subjectTorsion
dc.subjectCoupled to scalar
dc.subjectSolutions with torsion
dc.subjectGENERAL-RELATIVITY
dc.subjectCOSMOLOGICAL CONSTANT
dc.subject2+1 DIMENSIONS
dc.subjectBLACK-HOLE
dc.subjectSPACE-TIME
dc.subjectCARTAN
dc.subjectSUPERNOVAE
dc.subjectSPIN
dc.subjectPhysics
dc.titleEinstein gravity with torsion induced by the scalar field
dc.typeArticle
dspace.entity.typePublication
local.import.sourceWOS

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