Εμφάνιση απλής εγγραφής

dc.creatorAnagnostopoulos F.K., Kofinas G., Zarikas V.en
dc.date.accessioned2023-01-31T07:31:18Z
dc.date.available2023-01-31T07:31:18Z
dc.date.issued2019
dc.identifier10.1142/S0218271819440139
dc.identifier.issn02182718
dc.identifier.urihttp://hdl.handle.net/11615/70517
dc.description.abstractThe novel idea is that the undergoing accelerated expansion of the universe happens due to infrared quantum gravity modifications at intermediate astrophysical scales of galaxies or galaxy clusters, within the framework of Asymptotically Safe gravity. The reason is that structures of matter are associated with a scale-dependent positive cosmological constant of quantum origin. In this context, no extra unproven energy scales or fine-tuning are used. Furthermore, this model was confronted with the most recent observational data from a variety of probes, and with the aid of Bayesian analysis, the most probable values of the free parameters were extracted. Finally, the model proved to be statistically equivalent with I CDM, and thus being able to resolve naturally the concept of dark energy and its associated cosmic coincidence problem. © 2019 World Scientific Publishing Company.en
dc.language.isoenen
dc.sourceInternational Journal of Modern Physics Den
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85072560925&doi=10.1142%2fS0218271819440139&partnerID=40&md5=aeb51297721bec1873680dda14872b0b
dc.subjectWorld Scientific Publishing Co. Pte Ltden
dc.titleIR quantum gravity solves naturally cosmic acceleration and its coincidence problemen
dc.typeotheren


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Εμφάνιση απλής εγγραφής