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Cosmology via thermodynamics of polytropic gas

MakaleYalnız künyeScopus SJRQ2

Özet

We study cosmological scenarios of the polytropic gas (PG) dark matter-energy proposal in a Friedmann-Robertson-Walker (FRW) Universe. As a first step, we obtain an exact expression for the energy density of PG model by making use of the thermodynamics. Later, we investigate some cosmological quantities and perform neo-classical analyzes. Finally, we implement a connection between the PG and a homogenous minimally coupled scalar field by introducing its self-interacting potential.

Anahtar Kelimeler

Cosmologydark energypolytropic gas
RDL Kalıcı Bağlantı (PID)
https://rdlopen.rawdatalibrary.net/r/munzur/3895Resmi atıflarda kullanılan kalıcı adres
DOI
https://doi.org/10.1142/s0217732317501772Yayıncı resmi DOI adresi
İndeks kayıtları
ScopusScopusWeb of ScienceWeb of Science
Kaydın indeks veri tabanlarındaki sayfası (aktarımda alınan kayıt numarasıyla). Erişim, indeksin kendi koşullarına bağlıdır.
Atıflar
Scopus
10
WoS
10
OpenAlex
13
Her kaynağın kendi saydığı toplam atıf; aktarım ve zenginleştirme sırasında alındı.
Tam Kayıt
AlanDeğerDil
dc.contributor.authorAskin, Muzaffer
dc.contributor.authorSalti, Mustafa
dc.contributor.authorAydogdu, Oktay
dc.date.accessioned2026-10-28T14:57:16.425681230Z
dc.date.available2026-10-28T14:57:16.425681230Z
dc.date.issued2017
dc.description.abstractWe study cosmological scenarios of the polytropic gas (PG) dark matter-energy proposal in a Friedmann-Robertson-Walker (FRW) Universe. As a first step, we obtain an exact expression for the energy density of PG model by making use of the thermodynamics. Later, we investigate some cosmological quantities and perform neo-classical analyzes. Finally, we implement a connection between the PG and a homogenous minimally coupled scalar field by introducing its self-interacting potential.
dc.description.sponsorshipMersin University in Turkey, (2017-2-AP4-2022)
dc.description.sponsorshipResearch Fund of Mersin University
dc.identifier.articlenumber1750177
dc.identifier.doi10.1142/s0217732317501772
dc.identifier.eissn1793-6632
dc.identifier.issn0217-7323
dc.identifier.issue32
dc.identifier.scopus2-s2.0-85030830107
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/munzur/3895
dc.identifier.volume32
dc.identifier.wosWOS:000412829600006
dc.language.isoen
dc.publisherWorld Scientific Publishing Co. Pte Ltd
dc.relation.ispartofModern Physics Letters A
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectCosmology
dc.subjectdark energy
dc.subjectpolytropic gas
dc.subject.classificationAstronomy & Astrophysics
dc.subject.classificationPhysics, Nuclear
dc.subject.classificationPhysics, Particles & Fields
dc.subject.classificationPhysics, Mathematical
dc.subject.classificationPhysics
dc.subject.otherPROBE WMAP OBSERVATIONS
dc.subject.otherCONSTANT
dc.subject.otherSTATE
dc.titleCosmology via thermodynamics of polytropic gas
dc.typeArticle
rdl.citation.openalex13
rdl.citation.scopus10
rdl.citation.wos10
rdl.oa.statusclosed
rdl.scopus.quartileQ2
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)