IR quantum gravity solves naturally cosmic acceleration and its coincidence problem

dc.contributor.authorFotios K. Anagnostopoulos
dc.contributor.authorGeorgios Kofinas
dc.contributor.authorVasilios Zarikas
dc.date.accessioned2025-08-13T06:31:20Z
dc.date.available2025-08-13T06:31:20Z
dc.date.issued2019
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 ΛCDM, and thus being able to resolve naturally the concept of dark energy and its associated cosmic coincidence problem.
dc.identifier.citationAnagnostopoulos, F. K.; Kofinas, G.; Zarikas, V. (2019). IR quantum gravity solves naturally cosmic acceleration and its coincidence problem. International Journal of Modern Physics D, 28(14):1944013. DOI: 10.1142/S0218271819440139 (arXiv:2102.07578)
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9198
dc.language.isoen
dc.publisherInternational Journal of Modern Physics D (World Scientific)
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United Statesen
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/
dc.subjectinfrared quantum gravity
dc.subjectasymptotic safety
dc.subjectcosmic acceleration
dc.subjectcoincidence problem
dc.subjectscale-dependent cosmological constant
dc.subjecttype of access: open access
dc.titleIR quantum gravity solves naturally cosmic acceleration and its coincidence problem
dc.typeArticle

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