THERMODYNAMICS IN f (T, ?) GRAVITY

Basit Öğe Kaydı
dc.contributor.authorAskin, Muzaffer
dc.contributor.authorAbedi, Habib
dc.contributor.authorSalti, Mustafa
dc.date.accessioned2024-04-24T17:47:48Z
dc.date.available2024-04-24T17:47:48Z
dc.date.issued2015
dc.departmentDicle Üniversitesien_US
dc.description.abstractIn the present study, we discuss a non-equilibrium picture of thermodynamics at the apparent horizon of flat Friedmann-Roberton-Walker universe in f(T,theta) theory of gravity, where T is the torsion scalar and theta is the trace of the energy-momentum tensor. Mainly, we investigate the validity of the first and second laws of thermodynamics in this scenario. We consider two descriptions of the energy-momentum tensor of dark energy density and pressure and discuss that an equilibrium picture of gravitational thermodynamics can not be given in both cases. Furthermore, we also conclude that the second law of gravitational thermodynamics can be achieved both in phantom and quintessence phases of the universe.en_US
dc.identifier.endpage55en_US
dc.identifier.issn1221-146X
dc.identifier.issue1-2en_US
dc.identifier.startpage44en_US
dc.identifier.urihttps://hdl.handle.net/11468/22751
dc.identifier.volume60en_US
dc.identifier.wosWOS:000351190000005
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.language.isoenen_US
dc.publisherEditura Acad Romaneen_US
dc.relation.ispartofRomanian Journal of Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectThermodynamicsen_US
dc.subjectDark Matteren_US
dc.titleTHERMODYNAMICS IN f (T, ?) GRAVITYen_US
dc.titleTHERMODYNAMICS IN f (T, ?) GRAVITY
dc.typeArticleen_US

Dosyalar

Koleksiyon

WoS İndeksli Yayınlar Koleksiyonu