dc.contributor.author | Acunzo, Adriano | |
dc.contributor.author | Bajardi, Francesco | |
dc.contributor.author | Capozziello, Salvatore | |
dc.date.accessioned | 2022-08-31T10:55:01Z | |
dc.date.available | 2022-08-31T10:55:01Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Physics Letters B. 2022, vol. 826, art. no. 136907. | cs |
dc.identifier.issn | 0370-2693 | |
dc.identifier.issn | 1873-2445 | |
dc.identifier.uri | http://hdl.handle.net/10084/146442 | |
dc.description.abstract | We 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.iso | en | cs |
dc.publisher | Elsevier | cs |
dc.relation.ispartofseries | Physics Letters B | cs |
dc.relation.uri | https://doi.org/10.1016/j.physletb.2022.136907 | cs |
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.uri | http://creativecommons.org/licenses/by/4.0/ | cs |
dc.subject | non-local gravity | cs |
dc.subject | Noether symmetries | cs |
dc.subject | cosmology | cs |
dc.subject | exact solutions | cs |
dc.title | Non-local curvature gravity cosmology via Noether symmetries | cs |
dc.type | article | cs |
dc.identifier.doi | 10.1016/j.physletb.2022.136907 | |
dc.rights.access | openAccess | cs |
dc.type.version | publishedVersion | cs |
dc.type.status | Peer-reviewed | cs |
dc.description.source | Web of Science | cs |
dc.description.volume | 826 | cs |
dc.description.firstpage | art. no. 136907 | cs |
dc.identifier.wos | 000792884500011 | |