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2015

Semi-dynamical perturbations of unified dark energy

Lombriser, Lucas, Taylor, Andy

Understand

Linear cosmological perturbations of a large class of modified gravity and dark energy models can be unified in the effective field theory of cosmic acceleration, encompassing Horndeski scalar-tensor theories and beyond.

The fully available model space inherent to this formalism cannot be constrained by measurements in the quasistatic small-scale regime alone.
To facilitate the analysis of modifications from the concordance model beyond this limit, we introduce a semi-dynamical treatment extrapolated from the evolution of perturbations at a pivot scale of choice.
At small scales, and for Horndeski theories, the resulting modifications recover a quasistatic approximation but account for corrections to it near the Hubble scale.