2015
DOI: 10.48550/arxiv.1512.09118
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Many Faces of Mimetic Gravity

Katrin Hammer,
Alexander Vikman

Abstract: We consider the recently introduced mimetic gravity, which is a Weyl-symmetric extension of the General Relativity and which can play a role of an imperfect fluid-like Dark Matter with a small sound speed. In this paper we discuss in details how this higherderivative scalar-tensor theory goes beyond the construction by Horndeski, keeping only one scalar degree of freedom on top of two standard graviton polarizations. In particular, we consider representations of the theory in different sets of Weyl-invariant v… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
52
0

Year Published

2016
2016
2023
2023

Publication Types

Select...
6
4

Relationship

2
8

Authors

Journals

citations
Cited by 36 publications
(52 citation statements)
references
References 22 publications
(36 reference statements)
0
52
0
Order By: Relevance
“…The mass scale M is introduced to keep the canonical dimensions of the noncanonical scalar field ϕ. This action (2.1) also naturally appears [7][8][9] in the so-called mimetic gravity [10,11]. For later it is useful to note that the mass scale M can be assumed to be a function of the field ϕ, so that one can allow for a function…”
Section: Modelmentioning
confidence: 99%
“…The mass scale M is introduced to keep the canonical dimensions of the noncanonical scalar field ϕ. This action (2.1) also naturally appears [7][8][9] in the so-called mimetic gravity [10,11]. For later it is useful to note that the mass scale M can be assumed to be a function of the field ϕ, so that one can allow for a function…”
Section: Modelmentioning
confidence: 99%
“…[20][21][22][23][24][25][26][27][28][29][30][31][32][33][34][35][36], for recent developments in mimetic gravity see Refs. [37][38][39][40][41][42][43], for the Hamiltonian analysis of mimetic gravity see Refs. [44][45][46], and for a review see Ref.…”
mentioning
confidence: 99%
“…Now we can follow a similar procedure as in [26] and [13] and promote the scalar ϕ to an independent dynamical variable in order to eliminate the higher derivatives from the action. On this path we introduce a Lagrange multiplier, λ, enforcing the definition (2.19) so that the action (2.18) transforms into…”
Section: Gauge Invariant Variables and Scalar-vector-tensor Formulationmentioning
confidence: 99%

Axionic cosmological constant

Hammer,
Jirousek,
Vikman
2020
Preprint
Self Cite