Barrow holographic dark energy models in Lyra and general relativity theories

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dc.contributor.authorAktaş, Arzu
dc.contributor.authorAygün, Sezgin
dc.date.accessioned2025-01-27T19:37:20Z
dc.date.available2025-01-27T19:37:20Z
dc.date.issued2024
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThis study investigates the Barrow holographic dark energy (BHDE) matter distribution in the Bianchi I universe model in Lyra and General Relativity Theories. To this end, it obtains exact solutions by Hubble parameter, conservation equation, and BHDE energy density equation and supports them with graphics. The results show that the solutions are in harmony with the functioning of the universe and the nature of dark energy. It finally discusses the need for further research.
dc.identifier.doi10.54187/jnrs.1517322
dc.identifier.endpage127
dc.identifier.issn1304-7981
dc.identifier.issue2
dc.identifier.startpage119
dc.identifier.trdizinid1260191
dc.identifier.urihttps://doi.org/10.54187/jnrs.1517322
dc.identifier.urihttps://search.trdizin.gov.tr/tr/yayin/detay/1260191
dc.identifier.urihttps://hdl.handle.net/20.500.12428/17195
dc.identifier.volume13
dc.indekslendigikaynakTR-Dizin
dc.language.isoen
dc.relation.ispartofJournal of New Results in Science
dc.relation.publicationcategoryMakale - Ulusal Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_TRD_20250125
dc.subjectHubble parameter
dc.subjectLyra theory
dc.subjectBarrow holographic dark energy
dc.subjectGeneral relativity
dc.titleBarrow holographic dark energy models in Lyra and general relativity theories
dc.typeArticle

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