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Electromagnetic field and complexity of relativistic fluids in f (G) gravity

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dc.contributor.authorBhatti, M. Z.
dc.contributor.authorYousaf, Z.
dc.contributor.authorKhan, S.
dc.contributor.authorKhlopov, M. Y.
dc.contributor.authorХлопов, Максим Юрьевич
dc.date.accessioned2024-11-29T23:46:10Z
dc.date.available2024-11-29T23:46:10Z
dc.date.issued2021
dc.description.abstract© 2021 The Author(s).The principal idea behind this manuscript is to inspect the complexity of dissipating as well as non-dissipating self-gravitating sources which are coupled with locally anisotropic charged matter. The gravitational equations in the regime of f (G) (G is the Gauss-Bonnet invariant) theory have elaborated for the imperfectly charged stellar configuration to scrutinize the charged object in the presence of f (G) corrections. The impact of charge distribution on the connection between density inhomogeneity, Weyl tensor, and pressure anisotropy is investigated. By incorporating the constraints of QH (i.e. the quasi-homologous) evolution and CF = 0, (where CF denotes the complexity factor) multiple analytical solutions to the f (G) equations of gravity are developed defining the imperfectly charged compact spherical matter. Some of these stellar models (exact solutions) portray a spherical collapsing configuration of a charged fluid in which there arise a cavity about the fluid centre, while other models exhibit a fluid configuration wherein the sphere is totally filled by the fluid. These interior solutions to f (G) gravitational equations may exhibit some appealing astrophysical phenomenons.
dc.format.extentС. 4543-4560
dc.identifier.citationElectromagnetic field and complexity of relativistic fluids in f (G) gravity / Bhatti, M.Z. [et al.] // Monthly Notices of the Royal Astronomical Society. - 2021. - 506. - № 3. - P. 4543-4560. - 10.1093/mnras/stab2062
dc.identifier.doi10.1093/mnras/stab2062
dc.identifier.urihttps://www.doi.org/10.1093/mnras/stab2062
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dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000767866800008
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/25023
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleElectromagnetic field and complexity of relativistic fluids in f (G) gravity
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue3
oaire.citation.volume506
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