Magnetized Strange Quark Models in Lyra Theory

dc.authoridAktaş, Can / 0000-0002-0603-7862
dc.authoridÖzcan, Kadir / 0009-0006-4473-1229
dc.contributor.authorÖzcan, Kadir
dc.contributor.authorAktaş, Can
dc.date.accessioned2025-01-27T19:37:15Z
dc.date.available2025-01-27T19:37:15Z
dc.date.issued2023
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this study, the behavior of magnetized strange quark matter (MSQM) distribution in Lyra theory was investigated for homogeneous anisotropic Bianchi III, locally rotationally symmetric (LRS) Bianchi I, and Kantowski-Sachs universe models. We have used the equations of state, anisotropy, and linearly varying deceleration parameters to obtain the exact solutions of field equations in Lyra theory. When switching from the anisotropic universe model to the isotropic universe model, the magnetic field was not observed in the LRS Bianchi I universe. Besides, the graphs of the dynamic quantities obtained for each universe model were analyzed in detail. Finally, we inquire whether further research should be conducted.
dc.identifier.doi10.53570/jnt.1310436
dc.identifier.endpage101
dc.identifier.issn2149-1402
dc.identifier.issue43
dc.identifier.startpage92
dc.identifier.trdizinid1187132
dc.identifier.urihttps://doi.org/10.53570/jnt.1310436
dc.identifier.urihttps://search.trdizin.gov.tr/tr/yayin/detay/1187132
dc.identifier.urihttps://hdl.handle.net/20.500.12428/17168
dc.indekslendigikaynakTR-Dizin
dc.language.isoen
dc.relation.ispartofJournal of New Theory
dc.relation.publicationcategoryMakale - Ulusal Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_TRD_20250125
dc.subjectFizik
dc.subjectKatı Hal
dc.subjectFizik
dc.subjectNükleer
dc.subjectFizik
dc.subjectPartiküller ve Alanlar
dc.titleMagnetized Strange Quark Models in Lyra Theory
dc.typeArticle

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