LRS Bianchi I model with constant expansion rate in f (R, T) gravity

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dc.contributor.authorBeesham, Aroonkumar
dc.contributor.authorSingh, Vijay
dc.date.accessioned2026-02-24T08:06:39Z
dc.date.available2026-02-24T08:06:39Z
dc.date.issued2020
dc.departmentNameMathematical Sciences
dc.description.abstractLocally-rotationally-symmetric Bianchi-I space time model is studied with constant Hubble parameter in f (R,T ) = R + 2λT gravity. Although a single (primary) matter source is considered, an additional matter source appears due to the coupling between matter and f (R,T ) gravity. The constraints are obtained for a realistic cosmological scenario. The solutions are also extended to the case of a scalar field (normal or phantom) model, and it is found that the model is consistent with a phantom scalar field only. The coupled matter also acts as phantom matter. The study shows that if one expects an accelerating universe from an anisotropic model, then the solutions become physically relevant only at late times when the universe enters into an accelerated phase. Placing some observational bounds on the present equation of state of dark energy, ω0, the behavior of ω(z) is depicted, which shows that the phantom field starts dominating very recently, somewhere between 0.2 < z < 0.5. The geometrical behavior of the model remains identical to the one in general relativity
dc.facultyFaculty of Science, Agriculture and Engineering
dc.identifier.citationSingh, V. and Beesham, A., 2020. LRS Bianchi I model with constant expansion rate in f (R, T) gravity. Astrophysics and Space Science, 365(7), pp.1-8.
dc.identifier.issn1572-946X (online)
dc.identifier.issn0004-640X (print)
dc.identifier.otherhttps://doi.org/10.1007/s10509-020-03839-w
dc.identifier.urihttp://hdl.handle.net/10530/58818
dc.issuenumber365 / 7
dc.language.isoen
dc.pages1 - 8
dc.peerreviewedYes
dc.publisherSpringer Nature
dc.subjectLRS Bianchi I model
dc.subjectExact solutions
dc.subjectScalar field
dc.subjectConstant Hubble parameter
dc.subjectf (R,T ) modified gravity
dc.subjectAanisotropic model
dc.titleLRS Bianchi I model with constant expansion rate in f (R, T) gravity
dc.title.journalAstrophysics and Space Science
dc.typeJournal Article
dspace.entity.typePublication
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relation.isOrgUnitOfPublication71c06a0e-e111-424c-8caf-20609eacb82c
relation.isOrgUnitOfPublication.latestForDiscovery71c06a0e-e111-424c-8caf-20609eacb82c
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