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Author (up) Montani, G.; De Angelis, M.; Bombacigno, F.; Carlevaro, N. url  doi
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  Title Metric f(R) gravity with dynamical dark energy as a scenario for the Hubble tension Type Journal Article
  Year 2024 Publication Monthly Notices of the Royal Astronomical Society Abbreviated Journal Mon. Not. Roy. Astron. Soc.  
  Volume 527 Issue 1 Pages L156-L161  
  Keywords supernovae: general; galaxies: distances and redshifts; cosmological parameters; dark energy; cosmology:theory  
  Abstract We introduce a theoretical framework to interpret the Hubble tension, based on the combination of a metric f(R) gravity with a dynamical dark energy contribution. The modified gravity provides the non-minimally coupled scalar field responsible for the proper scaling of the Hubble constant, in order to accommodate for the local SNIa pantheon+ data and Planck measurements. The dynamical dark energy source, which exhibits a phantom divide line separating the low redshift quintessence regime (-1 < w < -1/3) from the phantom contribution ( w < -1) in the early Universe, guarantees the absence of tachyonic instabilities at low redshift. The resulting H-0(z) profile rapidly approaches the Planck value, with a plateau behaviour for z greater than or similar to 5. In this scenario, the Hubble tension emerges as a low redshift effect, which can be in principle tested by comparing SNIa predictions with far sources, like QUASARS and gamma ray bursts.  
  Address [Montani, Giovanni; Carlevaro, Nakia] ENEA, Fusion & Nucl Safety Dept, C R Frascati, Via E. Fermi 45, I-00044 Rome, Italy, Email: giovanni.montani@enea.it;  
  Corporate Author Thesis  
  Publisher Oxford Univ Press Place of Publication Editor  
  Language English Summary Language Original Title  
  Series Editor Series Title Abbreviated Series Title  
  Series Volume Series Issue Edition  
  ISSN 0035-8711 ISBN Medium  
  Area Expedition Conference  
  Notes WOS:001594527500028 Approved no  
  Is ISI yes International Collaboration yes  
  Call Number IFIC @ pastor @ Serial 6902  
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