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dc.contributor.authorKorpınar, Talat
dc.contributor.authorÜnlütürk, Yasin
dc.date.accessioned2021-12-12T17:01:05Z
dc.date.available2021-12-12T17:01:05Z
dc.date.issued2015
dc.identifier.issn0001-7701
dc.identifier.issn1572-9532
dc.identifier.urihttps://doi.org/10.1007/s10714-015-1980-7
dc.identifier.urihttps://hdl.handle.net/20.500.11857/3061
dc.description.abstractAnisotropic Bianchi type-I magnetized string cosmological models are obtained in decaying vacuum energy density proposed by Pradhan (Commun Theor Phys 55: 931-941, 2011). In this study, we obtain some physical and geometrical properties of biharmonic particles of a new spacetime using Bianchi type-I (B-I) cosmological model. We use solution of the Einstein's field equations for biharmonic particles. Some important features of the model have been discussed. Established the existence of string cosmological models for biharmonic particles, unlike the earlier authors, in this theory and studied some physical and geometrical properties.en_US
dc.language.isoengen_US
dc.publisherSpringer/Plenum Publishersen_US
dc.relation.ispartofGeneral Relativity and Gravitationen_US
dc.identifier.doi10.1007/s10714-015-1980-7
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectEnergyen_US
dc.subjectBienergyen_US
dc.subjectBiharmonic particleen_US
dc.subjectBianchi type-I (B-I) cosmological modelen_US
dc.subjectVariable cosmological constanten_US
dc.titleNew Bianchi type-I cosmological models for biharmonic particles using string cosmology with exponential lawen_US
dc.typearticle
dc.authoridKorpinar, Talat/0000-0003-4000-0892
dc.departmentFakülteler, Fen-Edebiyat Fakültesi, Matematik Bölümü
dc.identifier.volume47en_US
dc.identifier.issue11en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.authorscopusid36442531900
dc.authorscopusid26530489900
dc.identifier.wosWOS:000363971300010en_US
dc.identifier.scopus2-s2.0-84945258591en_US


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