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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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	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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