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2024

Alleviating cosmological tensions with a hybrid dark sector

Teixeira, Elsa M., Poulot, Gaspard, van de Bruck, Carsten et al.

Understand

We investigate a cosmological model inspired by hybrid inflation, where two scalar fields representing dark energy (DE) and dark matter (DM) interact through a coupling that is proportional to the DE scalar field $1/\phi$.

The strength of the coupling is governed solely by the initial condition of the scalar field, $\phi_i$, which parametrises deviations from the standard $\Lambda$CDM model.
In this model, the scalar field tracks the behaviour of DM during matter-domination until it transitions to DE while the DM component decays quicker than standard CDM during matter-domination, and is therefore different from some interacting DM-DE models which behaves like phantom dark energy.
Using \textit{Planck} 2018 CMB data, DESI BAO measurements and Pantheon+ supernova observations, we find that the model allows for an increase in $H_0$ that can help reduce the Hubble tension.

Built on

L. Verde, T. Treu, and A. G. Riess, Nature Astron. 3
Original
1907
Earlier work this paper cites.
N. Aghanim et al. (Planck), Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
W. Handley, Phys. Rev. D 103
Original
1908
Earlier work this paper cites.
A. Lewis, “GetDist: a Python package for analysing Monte Carlo samples,” (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, and J. Silk, Nature Astron. 4
Original
1911
Earlier work this paper cites.
H. Jeffreys, Theory of Probability (Clarendon Press, Oxford, England, 1939)
1939
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Statistical Science 7
1992
Earlier work this paper cites.
A. D. Linde, Phys. Rev. D 49
1994
Earlier work this paper cites.
M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
G. Efstathiou and S. Gratton, Mon. Not. Roy. Astron. Soc. 496
Original
2002
Earlier work this paper cites.
E. V. Linder, Phys. Rev. Lett. 90
2003
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, and J. Silk, Astrophys. J. Lett. 908
Original
2003
Earlier work this paper cites.
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2005
Earlier work this paper cites.
S. Das, P. S. Corasaniti, and J. Khoury, Physical Review D 73
2006
Earlier work this paper cites.
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2006
Earlier work this paper cites.
C. Heymans et al. , Astron. Astrophys. 646
Original
2007
Earlier work this paper cites.
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Original
2007
Earlier work this paper cites.
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Original
2007
Earlier work this paper cites.
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Original
2007
Earlier work this paper cites.
A. Tamone et al. (eBOSS), Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
A. de Mattia et al. (eBOSS), Mon. Not. Roy. Astron. Soc. 501
Original
2007
Earlier work this paper cites.
J. Hou et al. (eBOSS), Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
R. Neveux et al. (eBOSS), Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
H. du Mas des Bourboux et al. (eBOSS), Astrophys. J. 901
Original
2007
Earlier work this paper cites.
E. Di Valentino et al. , Astropart. Phys. 131
Original
2008
Earlier work this paper cites.

Similar

E. Di Valentino et al. , Astropart. Phys. 131
Original
2008
Cited alongside, same era.
E. Calabrese, A. Slosar, A. Melchiorri, G. F. Smoot, and O. Zahn, Phys. Rev. D 77
Original
2008
Cited alongside, same era.
K. Jedamzik, L. Pogosian, and G.-B. Zhao, Commun. in Phys. 4
Original
2010
Cited alongside, same era.
D. Blas, J. Lesgourgues, and T. Tram, Journal of Cosmology and Astroparticle Physics 2011
2011
Cited alongside, same era.
F. Beutler et al. , Monthly Notices of the Royal Astronomical Society 416
Original
2011
Cited alongside, same era.

Then

E. Abdalla et al. , JHEAp 34
Original
2022
Later among the works it cites.
L. Perivolaropoulos and F. Skara, New Astron. Rev. 95
Original
2022
Later among the works it cites.
E. Rosenberg, S. Gratton, and G. Efstathiou, Mon. Not. Roy. Astron. Soc. 517
Original
2022
Later among the works it cites.
D. Scolnic et al. , Astrophys. J. 938
Original
2022
Later among the works it cites.
Y. S. Murakami, A. G. Riess, B. E. Stahl, W. D. Kenworthy, D.-M. A. Pluck, A. Macoretta, D. Brout, D. O. Jones, D. M. Scolnic, and A. V. Filippenko, JCAP 11
Original
2023

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J. Martin, Comptes Rendus Physique 13

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