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Then

J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, New Class of Consistent Scalar-Tensor Theories
Original
2015
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Original
2015
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A. Barreira, M. Cautun, B. Li, C. M. Baugh, and S. Pascoli, Weak lensing by voids in modified lensing potentials

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2017

Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data

Renk, Janina, Zumalacárregui, Miguel, Montanari, Francesco et al.

Understand

Cosmological models with Galileon gravity are an alternative to the standard $\Lambda {\rm CDM}$ paradigm with testable predictions at the level of its self-accelerating solutions for the expansion history, as well as large-scale structure formation.

Here, we place constraints on the full parameter space of these models using data from the cosmic microwave background (CMB) (including lensing), baryonic acoustic oscillations (BAO) and the Integrated Sachs-Wolfe (ISW) effect.
We pay special attention to the ISW effect for which we use the cross-spectra, $C_\ell^{\rm T g}$, of CMB temperature maps and foreground galaxies from the WISE survey.
The sign of $C_\ell^{\rm T g}$ is set by the time evolution of the lensing potential in the redshift range of the galaxy sample: it is positive if the potential decays (like in $\Lambda {\rm CDM}$), negative if it deepens.