Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/372
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dc.contributor.authorDimitrijevic, Ivanen_US
dc.contributor.authorDragovich, Brankoen_US
dc.contributor.authorKoshelev, Alexey S.en_US
dc.contributor.authorRakić, Zoranen_US
dc.contributor.authorStankovic, Jelenaen_US
dc.date.accessioned2022-08-10T19:26:21Z-
dc.date.available2022-08-10T19:26:21Z-
dc.date.issued2020-06-01-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/372-
dc.description.abstractIn this paper, we investigate a nonlocal modification of general relativity (GR) with action is an analytic function of the d'Alembertian □. We found a few exact cosmological solutions of the corresponding equations of motion. There are two solutions which are valid only if Λ ≠ 0, k = 0, and they have no analogs in Einstein's gravity with cosmological constant Λ. One of these two solutions is, that mimics properties similar to an interference between the radiation and the dark energy. Another solution is a nonsingular bounce one. For these two solutions, some cosmological aspects are discussed. We also found explicit form of the nonlocal operator F(□), which satisfies obtained necessary conditions.en_US
dc.relation.ispartofSymmetryen_US
dc.subjectCosmological solutionsen_US
dc.subjectDark energyen_US
dc.subjectNonlocal gravityen_US
dc.subjectRadiationen_US
dc.titleSome cosmological solutions of a new nonlocal gravity modelen_US
dc.typeArticleen_US
dc.identifier.doi10.3390/SYM12060917-
dc.identifier.scopus2-s2.0-85087464028-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85087464028-
dc.contributor.affiliationGeometryen_US
dc.relation.issn20738994en_US
dc.relation.volume12en_US
dc.relation.issue6en_US
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptGeometry-
crisitem.author.orcid0000-0002-6226-0479-
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