Abstract

In the context of Einstein gravity, if the null energy condition (NEC) is satisfied, the energy density in expanding space-times always decreases while in contracting space-times the energy density grows and the universe eventually collapses into a singularity. In particular, no non-singular bounce is possible. It is, though, an open question if this energy condition can be violated in a controlled way, i.e., without introducing pathologies, such as unstable negative-energy states or an imaginary speed of sound. In this paper, we will re-examine the claim that the recently proposed mimetic scenario can violate the NEC without pathologies. We show that mimetic cosmology is prone to gradient instabilities even in cases when the NEC is satisfied (except for trivial examples). Most interestingly, the source of the instability is always the Einstein-Hilbert term in the action. The matter stress-energy component does not contribute spatial gradient terms but instead makes the problematic curvature modes dynamical. We also show that mimetic cosmology can be understood as a singular limit of known, well-behaved theories involving higher-derivative kinetic terms and discuss ways of removing the instability.

Highlights

  • The null energy condition (NEC) is assumed in general relativity, high-energy physics, and cosmology

  • We were interested in the question whether mimetic cosmology opens up a new way to stably violate the null energy condition

  • We have found that the mimetic theory suffers from a gradient instability even if the null energy condition is satisfied

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Summary

Introduction

The null energy condition (NEC) is assumed in general relativity, high-energy physics, and cosmology. A successful transition to the high-energy expanding phase requires the Hubble parameter to grow, eventually hit zero, switch sign and continue to grow until a high enough energy ∼ H2 is reached for standard big-bang evolution to follow This approach has the advantage that it does not require knowledge of quantum gravity but one can safely rely on the low-energy effective theory. Obviously, this type of non-singular bounce involves a NEC violating form of stress-energy so that it stands or fails depending on whether it is possible to violate the NEC without pathologies.

Basics of mimetic cosmology
Linear stability analysis
N2 φ 2
Spatially-flat gauge
Co-moving gauge
Mimetic cosmology as a singular limit of higherderivative theories
Discussion
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