Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28387
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | BONANNO, Alfio Maurizio | en_US |
dc.contributor.author | Saueressig, Frank | en_US |
dc.date.accessioned | 2020-11-17T15:53:41Z | - |
dc.date.available | 2020-11-17T15:53:41Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1631-0705 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28387 | - |
dc.description.abstract | Asymptotic safety, based on a non-Gaussian fixed point of the gravitational renormalization group flow, provides an elegant mechanism for completing the gravitational force at sub-Planckian scales. At high energies, the fixed point controls the scaling of couplings such that unphysical divergences are absent, while the emergence of classical low-energy physics is linked to a crossover between two renormalization group fixed points. These features make asymptotic safety an attractive framework for the building of a cosmological model. The resulting scenarios may naturally give rise to a quantum-gravity-driven inflationary phase in the very early universe and an almost scale-free fluctuation spectrum. Moreover, effective descriptions arising from an improvement of the renormalization group permit a direct comparison to cosmological observations as, e.g., Planck data. | en_US |
dc.language.iso | eng | en_US |
dc.title | Asymptotically safe cosmology - A status report | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.crhy.2017.02.002 | en_US |
dc.identifier.scopus | 2-s2.0-85019870331 | en_US |
dc.identifier.isi | 000404687900007 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S1631070517300270 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 18 | en_US |
dc.relation.issue | 3-4 | en_US |
dc.relation.firstpage | 254 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 2 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | COMPTES RENDUS PHYSIQUE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017CRPhy..18..254B | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 1631-0705 | - |
crisitem.journal.ance | E041092 | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.orcid | 0000-0003-3175-9776 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
CRP preprint1702.04137.pdf | preprint | 775.11 kB | Adobe PDF | Visualizza/apri |
OA1.pdf | [Administrators only] | 457.55 kB | Adobe PDF |
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