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L. Amendola, Coupled quintessence
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G. R. Farrar and P. J. E. Peebles, Interacting Dark Matter and Dark Energy
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Original
2012
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C. P. Ahn, R. Alexandroff, C. Allende Prieto, F. Anders, S. F. Anderson, T. Anderton, B. H. Andrews, É. Aubourg, S. Bailey, F. A. Bastien, and et al., The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment
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2014

Linear Perturbation constraints on Multi-coupled Dark Energy

Piloyan, Arpine, Marra, Valerio, Baldi, Marco et al.

Understand

The Multi-coupled Dark Energy (McDE) scenario has been recently proposed as a specific example of a cosmological model characterized by a non-standard physics of the dark sector of the universe that nevertheless gives an expansion history which does not significantly differ from the one of the standard $\Lambda $CDM model.

In this work, we present the first constraints on the McDE scenario obtained by comparing the predicted evolution of linear density perturbations with a large compilation of recent data sets for the growth rate $f\sigma_{8}$, including 6dFGS, LRG, BOSS, WiggleZ and VIPERS.
Confirming qualitative expectations, growth rate data provide much tighter bounds on the model parameters as compared to the extremely loose bounds that can be obtained when only the background expansion history is considered.
In particular, the $95\%$ confidence level on the coupling strength $|\beta |$ is reduced from $|\beta |\leq 83$ (background constraints only) to $|\beta |\leq 0.88$ (background and linear perturbation constraints).

Built on

H. A. Buchdahl, Non-linear Lagrangians and cosmological theory
1970
Earlier work this paper cites.
A. A. Starobinsky, A new type of isotropic cosmological models without singularity
1980
Earlier work this paper cites.
C. Wetterich, Cosmology and the Fate of Dilatation Symmetry
1988
Earlier work this paper cites.
B. Ratra and P. J. E. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field
1988
Earlier work this paper cites.
C. Wetterich, The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’
1995
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
Supernova Cosmology Project
1999
Earlier work this paper cites.
L. Amendola, Coupled quintessence
2000
Earlier work this paper cites.
G. Dvali, G. Gabadadze, and M. Porrati, 4-D gravity on a brane in 5-D Minkowski space
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, Essentials of k-essence
2001
Earlier work this paper cites.
R. Caldwell, A Phantom menace?
2002
Earlier work this paper cites.
G. R. Farrar and P. J. E. Peebles, Interacting Dark Matter and Dark Energy
2004
Earlier work this paper cites.