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Cosmological perturbations in mimetic Horndeski gravity

TLDR
In this article, the authors study linear scalar perturbations around a flat FLRW background in mimetic Horndeski gravity and obtain the equation of motion for the comoving curvature perturbation.
Abstract
We study linear scalar perturbations around a flat FLRW background in mimetic Horndeski gravity. In the absence of matter, we show that the Newtonian potential satisfies a second-order differential equation with no spatial derivatives. This implies that the sound speed for scalar perturbations is exactly zero on this background. We also show that in mimetic $G^3$ theories the sound speed is equally zero. We obtain the equation of motion for the comoving curvature perturbation (first order differential equation) and solve it to find that the comoving curvature perturbation is constant on all scales in mimetic Horndeski gravity. We find solutions for the Newtonian potential evolution equation in two simple models. Finally we show that the sound speed is zero on all backgrounds and therefore the system does not have any wave-like scalar degrees of freedom.

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Citations
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Journal ArticleDOI

Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics

TL;DR: Mimetic gravity is a Weyl-symmetric extension of General Relativity, related to the latter by a singular disformal transformation, wherein the appearance of a dust-like perfect fluid can mimic cold dark matter at a cosmological level as discussed by the authors.
Journal ArticleDOI

Living with ghosts in Horava-Lifshitz gravity

TL;DR: In this article, the authors considered the projectable Horava-Lifshitz model and showed that the decay rate of photons is tiny in a wide range of phenomenologically acceptable parameters.
Journal ArticleDOI

Alive and well: mimetic gravity and a higher-order extension in light of GW170817

TL;DR: In this article, a higher-order extension of the original mimetic theory, appearing in the low-energy limit of projectable Hořava-Lifshitz gravity, is considered.
Journal ArticleDOI

Instabilities in Mimetic Matter Perturbations

TL;DR: In this paper, the authors study cosmological perturbations in mimetic matter scenario with a general higher derivative function and calculate the quadratic action and show that both the kinetic term and the gradient term have the wrong sings.
References
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Book

Theory of Cosmological Perturbations

TL;DR: In this paper, the authors present in a manifestly gauge-invariant form the theory of classical linear gravitational perturbations in part I, and a quantum theory of cosmological perturbation in part II.
Journal ArticleDOI

Second-order scalar-tensor field equations in a four-dimensional space

TL;DR: In this article, the second-order Euler-Lagrange tensors are derived from a Lagrangian which is at most of second order in the derivatives of the field functions.
Journal ArticleDOI

From k-essence to generalized Galileons

TL;DR: In this article, the most general scalar field theories with second-order field equations are derived from linear combinations of Lagrangians made by multiplying a particular form of the Galileon Lagrangian by an arbitrary scalar function of the field and its first derivatives.
Journal ArticleDOI

Generalized G-Inflation —Inflation with the Most General Second-Order Field Equations—

TL;DR: In this paper, the generalized Galileons were used as a framework to develop the most general single-field inflation models ever, Generalized G-inflation, containing yet further generalization of Ginf lation, as well as previous examples such as k-inflation, extended inflation, and new Higgs inflation as special cases.
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