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Large-scale structure phenomenology of viable Horndeski theories · Around

2017

Large-scale structure phenomenology of viable Horndeski theories

Peirone, Simone, Koyama, Kazuya, Pogosian, Levon et al.

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Phenomenological functions $\Sigma$ and $\mu$, also known as $G_{\rm light}/G$ and $G_{\rm matter}/G$, are commonly used to parameterize modifications of the growth of large-scale structure in alternative theories of gravity.

We study the values these functions can take in Horndeski theories, i.e.
the class of scalar-tensor theories with second order equations of motion.
We restrict our attention to models that are in a broad agreement with tests of gravity and the observed cosmic expansion history.

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