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2015

Constraints on deviations from ${\Lambda}$CDM within Horndeski gravity

Bellini, Emilio, Cuesta, Antonio J., Jimenez, Raul et al.

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Recent anomalies found in cosmological datasets such as the low multipoles of the Cosmic Microwave Background or the low redshift amplitude and growth of clustering measured by e.g., abundance of galaxy clusters and redshift space distortions in galaxy surveys, have motivated explorations of models beyond standard $\Lambda$CDM.

Of particular interest are models where general relativity (GR) is modified on large cosmological scales.
Here we consider deviations from $\Lambda$CDM+GR within the context of Horndeski gravity, which is the most general theory of gravity with second derivatives in the equations of motion.
We adopt a parametrization in which the four additional Horndeski functions of time $\alpha_i(t)$ are proportional to the cosmological density of dark energy $\Omega_{DE}(t)$.

Constraints on deviations from ${\Lambda}$CDM within Horndeski gravity · Around

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