Strange quark matter solutions for Marder's universe in f (R, T) gravity with Λ
dc.authorid | Aygün, Sezgin / 0000-0002-2969-4195 | |
dc.authorid | Aktaş, Can / 0000-0002-0603-7862 | |
dc.authorid | Yılmaz, İhsan / 0000-0001-7684-9690 | |
dc.contributor.author | Aygün, Sezgin | |
dc.contributor.author | Aktaş, Can | |
dc.contributor.author | Yılmaz, İhsan | |
dc.date.accessioned | 2025-01-27T21:01:34Z | |
dc.date.available | 2025-01-27T21:01:34Z | |
dc.date.issued | 2016 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description.abstract | In this paper, we investigate homogeneous cylindrically symmetric Marder's universe in the presence of strange quark matter (SQM) source in f (R, T) gravity with cosmological constant Lambda. For this aim we have used the anisotropy feature (sigma(x)(x)/theta) of Marder type universe and equation of state (EoS) strange quark matter to obtain solutions in two classes f (R, T) gravity (Harko et al. in Phys. Rev. D 84:024020, 2011). Finally, some physical and kinematical properties are discussed. | |
dc.identifier.doi | 10.1007/s10509-016-2956-0 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.issn | 1572-946X | |
dc.identifier.issue | 12 | |
dc.identifier.scopus | 2-s2.0-84994824027 | |
dc.identifier.scopusquality | Q2 | |
dc.identifier.uri | https://doi.org/10.1007/s10509-016-2956-0 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/27099 | |
dc.identifier.volume | 361 | |
dc.identifier.wos | WOS:000389150500011 | |
dc.identifier.wosquality | Q3 | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.publisher | Springer | |
dc.relation.ispartof | Astrophysics and Space Science | |
dc.relation.publicationcategory | info:eu-repo/semantics/openAccess | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | Marder universe | |
dc.subject | f(R, T) gravity | |
dc.subject | Strange quark matter | |
dc.title | Strange quark matter solutions for Marder's universe in f (R, T) gravity with Λ | |
dc.type | Article |
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