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Sharma–Mittal holographic dark energy and scalar field in Bianchi type-I cosmology

MakaleYalnız künyeScopus SJRQ1

Özet

In this work, we studied Sharma–Mittal holographic dark energy model by considering Bianchi type-I cosmology. For this purpose we analyzed equation of state parameter using IR cutoff scale. Also it is reconstructed correspondence between Sharma–Mittal holographic dark energy and tachyon and quintessence scalar fields. Finally, we created plots for the time-evolution of the equation of state, kinetic energy, and scalar potential.

Anahtar Kelimeler

Bianchi type-I universescalar fieldsSharma–Mittal holographic dark energy
RDL Kalıcı Bağlantı (PID)
https://rdlopen.rawdatalibrary.net/r/munzur/2093Resmi atıflarda kullanılan kalıcı adres
DOI
https://doi.org/10.1007/s10714-023-03188-3Yayıncı resmi DOI adresi
İndeks kayıtları
ScopusScopusWeb of ScienceWeb of Science
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Atıflar
Scopus
3
WoS
4
OpenAlex
4
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Tam Kayıt
AlanDeğerDil
dc.contributor.authorKorunur, Sibel
dc.date.accessioned2026-10-28T14:54:55.722907816Z
dc.date.available2026-10-28T14:54:55.722907816Z
dc.date.issued2024
dc.description.abstractIn this work, we studied Sharma–Mittal holographic dark energy model by considering Bianchi type-I cosmology. For this purpose we analyzed equation of state parameter using IR cutoff scale. Also it is reconstructed correspondence between Sharma–Mittal holographic dark energy and tachyon and quintessence scalar fields. Finally, we created plots for the time-evolution of the equation of state, kinetic energy, and scalar potential.
dc.identifier.articlenumber2
dc.identifier.doi10.1007/s10714-023-03188-3
dc.identifier.eissn1572-9532
dc.identifier.issn0001-7701
dc.identifier.issue1
dc.identifier.scopus2-s2.0-85180205711
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/munzur/2093
dc.identifier.volume56
dc.identifier.wosWOS:001126440300001
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofGeneral Relativity and Gravitation
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectBianchi type-I universe
dc.subjectscalar fields
dc.subjectSharma–Mittal holographic dark energy
dc.subject.classificationAstronomy & Astrophysics
dc.subject.classificationPhysics, Multidisciplinary
dc.subject.classificationPhysics, Particles & Fields
dc.subject.classificationPhysics
dc.subject.otherBLACK-HOLES
dc.subject.otherCONSTANT
dc.subject.otherUNIVERSE
dc.subject.otherMODELS
dc.subject.otherRENYI
dc.subject.otherDYNAMICS
dc.subject.otherTSALLIS
dc.subject.otherGRAVITY
dc.titleSharma–Mittal holographic dark energy and scalar field in Bianchi type-I cosmology
dc.typeArticle
rdl.citation.openalex4
rdl.citation.scopus3
rdl.citation.wos4
rdl.oa.statusclosed
rdl.scopus.quartileQ1
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)