Viable Mimetic Completion of Unified Inflation-Dark Energy Evolution in Modified Gravity
arXiv:1608.07806 · doi:10.1103/PhysRevD.94.104050
Abstract
In this paper, we demonstrate that a unified description of early and late-time acceleration is possible in the context of mimetic gravity. We study the inflationary era in detail and demonstrate that it can be realized even in mimetic gravity where traditional gravity fails to describe the inflation. By using standard methods we calculated the spectral index of primordial curvature perturbations and the scalar-to-tensor ratio. We use two gravity models and as it turns out, for both the models under study the observational indices are compatible with both the latest Planck and the BICEP2/Keck array data. Finally, the graceful exit from inflation is guaranteed by the existence of growing curvature perturbations when the slow-roll era ends.
PRD Accepted
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