Built on

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2024

Modified gravity bridges the cosmological tensions

Ye, Gen

Understand

The standard model of cosmology, $\Lambda$CDM, is plagued by various tensions with recent observations.

The most pressing one is the Hubble tension, where the observed expansion rate of our Universe is $5\sigma$ larger than that predicted by $\Lambda$CDM.
Recently, the result from DESI also reveals a new inconsistency between the baryon acoustic oscillation and cosmic microwave background (CMB) observations in $\Lambda$CDM.
It is found that these major cosmological tensions can be traced back to a common physical origin - the non-minimal coupling between gravity and matter, different from the expectation of general relativity (GR).

Built on

P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Phys. Dark Univ. 42
Original
1904
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Phys. Rev. D 100
Original
1905
Earlier work this paper cites.
W. Handley, J. Open Source Softw. 4
Original
1905
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky, and C. Umiltà, Phys. Rev. D 100
Original
1906
Earlier work this paper cites.
N. Aghanim et al. (Planck), Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, Phys. Rev. D 103
Original
1910
Earlier work this paper cites.
J. Alvey, N. Sabti, M. Escudero, and M. Fairbairn, Eur. Phys. J. C 80
Original
1910
Earlier work this paper cites.
A. Lewis, (2019) , arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
H. Jeffreys, The Theory of Probability , Oxford Classic Texts in the Physical Sciences (1939)
1939
Earlier work this paper cites.
A. I. Vainshtein, Phys. Lett. B 39
1972
Earlier work this paper cites.
G. W. Horndeski, Int. J. Theor. Phys. 10
1974
Earlier work this paper cites.
E. Garcia-Berro, E. Gaztanaga, J. Isern, O. Benvenuto, and L. Althaus, (1999), arXiv:astro-ph/9907440
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538
2000
Earlier work this paper cites.
B. Boisseau, G. Esposito-Farese, D. Polarski, and A. A. Starobinsky, Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
A. G. Riess, Nature Rev. Phys. 2
Original
2001
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
M. Escudero Abenza, JCAP 05
Original
2001
Earlier work this paper cites.
A. Riazuelo and J.-P. Uzan, Phys. Rev. D 66
2002
Earlier work this paper cites.
E. V. Linder, Phys. Rev. Lett. 90
2003
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Phys. Rev. D 102
Original
2003
Earlier work this paper cites.
M. Braglia, M. Ballardini, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, K. Koyama, and D. Paoletti, Phys. Rev. D 102
Original
2004
Earlier work this paper cites.
G. Ballesteros, A. Notari, and F. Rompineve, JCAP 11
Original
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, Phys. Rev. Lett. 93
2004
Earlier work this paper cites.
J. Torrado and A. Lewis, JCAP 05
Original
2005
Earlier work this paper cites.
S. Nesseris and L. Perivolaropoulos, Phys. Rev. D 73
2006
Earlier work this paper cites.
R. Trotta, Mon. Not. Roy. Astron. Soc. 378
2007
Earlier work this paper cites.
R. Trotta, Contemp. Phys. 49
Original
2008
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Phys. Rev. D 102
Original
2008
Earlier work this paper cites.