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dc.contributor.authorAcunzo, Adriano
dc.contributor.authorBajardi, Francesco
dc.contributor.authorCapozziello, Salvatore
dc.date.accessioned2022-08-31T10:55:01Z
dc.date.available2022-08-31T10:55:01Z
dc.date.issued2022
dc.identifier.citationPhysics Letters B. 2022, vol. 826, art. no. 136907.cs
dc.identifier.issn0370-2693
dc.identifier.issn1873-2445
dc.identifier.urihttp://hdl.handle.net/10084/146442
dc.description.abstractWe consider extensions of General Relativity based on the non-local function f (R, rectangle(-1) R), where R is the Ricci curvature scalar and the non-locality is due to the term rectangle(-1) R. We focus on cosmological minisuperspaces and select viable models by the Noether Symmetry Approach. Then we find viable exact solutions pointing out the role of non-locality in cosmology.cs
dc.language.isoencs
dc.publisherElseviercs
dc.relation.ispartofseriesPhysics Letters Bcs
dc.relation.urihttps://doi.org/10.1016/j.physletb.2022.136907cs
dc.rights© 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.cs
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/cs
dc.subjectnon-local gravitycs
dc.subjectNoether symmetriescs
dc.subjectcosmologycs
dc.subjectexact solutionscs
dc.titleNon-local curvature gravity cosmology via Noether symmetriescs
dc.typearticlecs
dc.identifier.doi10.1016/j.physletb.2022.136907
dc.rights.accessopenAccesscs
dc.type.versionpublishedVersioncs
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume826cs
dc.description.firstpageart. no. 136907cs
dc.identifier.wos000792884500011


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© 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.
Except where otherwise noted, this item's license is described as © 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.