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Author  |
Montani, G.; De Angelis, M.; Bombacigno, F.; Carlevaro, N. |

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Title |
Metric f(R) gravity with dynamical dark energy as a scenario for the Hubble tension |
Type |
Journal Article |
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Year |
2024 |
Publication |
Monthly Notices of the Royal Astronomical Society |
Abbreviated Journal |
Mon. Not. Roy. Astron. Soc. |
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Volume |
527 |
Issue |
1 |
Pages |
L156-L161 |
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Keywords |
supernovae: general; galaxies: distances and redshifts; cosmological parameters; dark energy; cosmology:theory |
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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. |
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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; |
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Publisher |
Oxford Univ Press |
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Language |
English |
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Original Title |
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Series Volume |
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ISSN |
0035-8711 |
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Notes |
WOS:001594527500028 |
Approved |
no |
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Is ISI |
yes |
International Collaboration |
yes |
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Call Number |
IFIC @ pastor @ |
Serial |
6902 |
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