Barrow holographic dark energy models in Lyra and general relativity theories

dc.contributor.authorAktaş, Arzu
dc.contributor.authorAygün, Sezgin
dc.date.accessioned2025-03-17T07:29:56Z
dc.date.available2025-03-17T07:29:56Z
dc.date.issued2024
dc.departmentFakülteler, Mühendislik Fakültesi, Bilgisayar Mühendisliği Bölümü
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.citationAktaş, A., & Aygün, S. (2024). Barrow holographic dark energy models in Lyra and general relativity theories. Journal of New Results in Science, 13(2), 119-127. https://doi.org/10.54187/jnrs.1517322
dc.identifier.doi10.54187/jnrs.1517322
dc.identifier.endpage127
dc.identifier.issue2
dc.identifier.startpage119
dc.identifier.urihttps://hdl.handle.net/20.500.12941/293
dc.identifier.volume13
dc.indekslendigikaynakTR-Dizin
dc.institutionauthorAktaş, Arzu
dc.language.isoen
dc.publisherJournal of New Results in Science
dc.relation.ispartofJournal of New Results in Science
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectBarrow holographic dark energy
dc.subjectLyra theory
dc.subjectHubble parameter
dc.subjectGeneral relativity
dc.titleBarrow holographic dark energy models in Lyra and general relativity theories
dc.typeArticle

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