Self-gravitating spherically symmetric fluid models in Brans–Dicke gravity.

dc.contributor.authorManzoor, Rubab
dc.date.accessioned2018-10-19T11:37:10Z
dc.date.available2018-10-19T11:37:10Z
dc.date.issued2015-08-06
dc.description.abstractThis paper is devoted to study self-gravitating spherically symmetric fluid models in Brans–Dicke gravity. We formulate a set of equations which govern the dynamics of evolving gravitating fluids through Weyl tensor, shear tensor, expansion scalar, anisotropy, energy inhomogeneity, dissipation as well as scalar field. We also discuss some particular cases according to different dynamical conditions. It is concluded that fluid models for regular distribution of scalar field are consistent with general relativity and models due to irregular distribution of scalar field deviate from theory of general relativity.en_US
dc.identifier.citationSharif, M., & Manzoor, R. (2015). Self-gravitating spherically symmetric fluid models in Brans–Dicke gravity. General Relativity and Gravitation, 47(9), 1-17.(Rubab Manzoor) (IF 1.77 JCR Listed)en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/3374
dc.language.isoenen_US
dc.publisherGeneral Relativity and Gravitation.en_US
dc.subjectMathematicsen_US
dc.subjectBrans–Dicke theory · Relativistic dissipative fluiden_US
dc.titleSelf-gravitating spherically symmetric fluid models in Brans–Dicke gravity.en_US
dc.typeArticleen_US
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