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dc.creatorAnagnostopoulos F.K., Bonanno A., Mitra A., Zarikas V.en
dc.date.accessioned2023-01-31T07:31:18Z
dc.date.available2023-01-31T07:31:18Z
dc.date.issued2022
dc.identifier10.1103/PhysRevD.105.083532
dc.identifier.issn24700010
dc.identifier.urihttp://hdl.handle.net/11615/70516
dc.description.abstractA convincing explanation for the nature of the dark energy and dark matter is still missing. In recent works a RG-improved swiss-cheese cosmology with an evolving cosmological constant dependent on the Schücking radius has been proven to be a promising model to explain the observed cosmic acceleration. In this work we extend this model to consider the combined scaling of the Newton constant G and the cosmological constant Λ according to the IR-fixed point hypothesis. We shall show that our model easily generates the observed recent passage from deceleration to acceleration without need of extra energy scales, exotic fields or fine-tuning. In order to check the generality of the concept, two different scaling relations have been analyzed and we proved that both are in very good agreement with ΛCDM cosmology while one of them has no fine-tuning problem. We also show that our model satisfies the observational local constraints on Ġ/G. © 2022 American Physical Society.en
dc.language.isoenen
dc.sourcePhysical Review Den
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85129228452&doi=10.1103%2fPhysRevD.105.083532&partnerID=40&md5=184c10d9378bfea852bb9168e6c362d1
dc.subjectAmerican Physical Societyen
dc.titleSwiss-cheese cosmologies with variable G and Λ from the renormalization groupen
dc.typejournalArticleen


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