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1901
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2008
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K. Bamba, S. Nojiri, and S. D. Odintsov, Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills-F(R) gravity and non-minimal vector-F(R) gravity
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J. Zuntz, T. G. Zlosnik, F. Bourliot, P. G. Ferreira, and G. D. Starkman, Vector field models of modified gravity and the dark sector
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2010
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D. Blas, J. Lesgourgues, and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
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Original
2012
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Then

B. Sagredo, S. Nesseris, and D. Sapone, Internal Robustness of Growth Rate data
Original
2018
Later among the works it cites.
DES Collaboration
2019
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Original
2019
Later among the works it cites.
R. Arjona, W. Cardona, and S. Nesseris, Unraveling the effective fluid approach for f ⁡ ( R ) f(R) models in the subhorizon approximation
Original
2019
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S. Nakamura, A. De Felice, R. Kase, and S. Tsujikawa, Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
Original
2019

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2023

Scrutinizing coupled vector dark energy in light of data

Cardona, Wilmar, Palacios-Córdoba, Jose L., Valenzuela-Toledo, César A.

Understand

Since current challenges faced by $\Lambda$CDM might be hinting at new unravelled physics, here we investigate a plausible cosmological model where a vector field acts as source of dark energy.

In particular, we examine whether an energy-momentum exchange between dark energy and dark matter could provide an explanation for current discrepancies in cosmological parameters.
We carefully work out equations governing background and linear order perturbations and implement them in a Boltzmann code.
We found that a negative coupling makes the dark energy equation of state less negative and closer to a cosmological constant during the matter dominated epoch than an uncoupled vector dark energy model.