Gravitational energy–momentum pseudo-tensor in Palatini and metric f ( R ) gravity

dc.contributor.authorAbedi, Habib
dc.contributor.authorCapozziello, Salvatore
dc.contributor.authorCapriolo, Maurizio
dc.contributor.authorAbbassi, Amir M.
dc.date.accessioned2022-07-14T06:07:28Z
dc.date.available2022-07-14T06:07:28Z
dc.date.issued2022
dc.description.abstractWe derive the gravitational energy-momentum pseudo-tensor tau(mu)(upsilon) in both Palatini and metric approaches to f (R) gravity. We then obtain the related cosmological gravitational energy density. Considering a flat Friedmann-Lemaitre-Robertson-Walker spacetime, the energy density complex of matter and gravitation vanishes in the metric approach, but results non-vanishing in the Palatini formalism. This feature could be relevant in order to physically discriminate between the two approaches.cs
dc.description.firstpageart. no. 168796cs
dc.description.sourceWeb of Sciencecs
dc.description.volume439cs
dc.identifier.citationAnnals of Physics. 2022, vol. 439, art. no. 168796.cs
dc.identifier.doi10.1016/j.aop.2022.168796
dc.identifier.issn0003-4916
dc.identifier.issn1096-035X
dc.identifier.urihttp://hdl.handle.net/10084/146382
dc.identifier.wos000790347000012
dc.language.isoencs
dc.publisherElseviercs
dc.relation.ispartofseriesAnnals of Physicscs
dc.relation.urihttps://doi.org/10.1016/j.aop.2022.168796cs
dc.rights© 2022 Elsevier Inc. All rights reserved.cs
dc.subjectenergy–momentum complexcs
dc.subjectalternative gravitycs
dc.subjectcosmologycs
dc.titleGravitational energy–momentum pseudo-tensor in Palatini and metric f ( R ) gravitycs
dc.typearticlecs
dc.type.statusPeer-reviewedcs

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