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We use the effective field theory of dark energy (EFT of DE) formalism to constrain dark energy models belonging to the Horndeski class with the recent Planck 2015 CMB data.
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G. W. Horndeski, Int. J. Theor. Phys. 10
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A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis and R. Rattazzi, “Causality, analyticity and an IR obstruction to UV completion,” JHEP 0610
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A. Hojjati, L. Pogosian and G. B. Zhao, “Testing gravity with CAMB and CosmoMC,” JCAP 1108
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G. Gubitosi, F. Piazza and F. Vernizzi, “The Effective Field Theory of Dark Energy,” JCAP 1302
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J. Bel, C. Marinoni, B. R. Granett, L. Guzzo, J. A. Peacock, and E. Branchini et al
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J. Bloomfield, “A Simplified Approach to General Scalar-Tensor Theories,” JCAP 1312
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A. Lewis, “Efficient sampling of fast and slow cosmological parameters,” Phys. Rev. D 87
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