pith. sign in

arxiv: 1408.3561 · v3 · pith:TPRPOW7Znew · submitted 2014-08-15 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph

Mimetic F(R) gravity: inflation, dark energy and bounce

classification ✦ hep-th astro-ph.COgr-qchep-ph
keywords theorygravitymimeticinflationuniverseaccelerationbounceconvenient
0
0 comments X
read the original abstract

We propose the mimetic $F(R)$ theory and investigate the early-time and late-time acceleration in such theory. It is demonstrated that inflation consistent with observable data may be realized in such theory. The reconstruction of realistic $\Lambda$CDM era is also possible as well as the unification of early-time inflation with late-time acceleration or bounce universe. It is stressed that specific universe evolution is governed by mimetic $F(R)$ theory which is different from convenient $F(R)$ gravity. The corresponding examples are presented. Mimetic $F(R)$ gravity is generalized by the addition of the scalar potential in the formulation of convenient $F(R)$ gravity with specific Lagrange multiplier constraint. It is demonstrated that such theory may admit the arbitrary universe evolution via the corresponding choice of the scalar potential and/or function $F(R)$.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.