Abstract

Using our anholonomic frame deformation method, we show how generic off-diagonal cosmological solutions depending, in general, on all spacetime coordinates and undergoing a phase of ultra-slow contraction can be constructed in massive gravity. In this paper, there are found and studied new classes of locally anisotropic and (in)homogeneous cosmological metrics with open and closed spatial geometries. The late time acceleration is present due to effective cosmological terms induced by nonlinear off-diagonal interactions and graviton mass. The off-diagonal cosmological metrics and related Stückelberg fields are constructed in explicit form up to nonholonomic frame transforms of the Friedmann–Lamaître–Robertson–Walker (FLRW) coordinates. We show that the solutions include matter, graviton mass and other effective sources modeling nonlinear gravitational and matter fields interactions in modified and/or massive gravity, with polarization of physical constants and deformations of metrics, which may explain certain dark energy and dark matter effects. There are stated and analyzed the conditions when such configurations mimic interesting solutions in general relativity and modifications and recast the general Painlevé–Gullstrand and FLRW metrics. Finally, we elaborate on a reconstruction procedure for a subclass of off-diagonal cosmological solutions which describe cyclic and ekpyrotic universes, with an emphasis on open issues and observable signatures.

Highlights

  • The idea that graviton may have a nontrivial mass was proposed by Fierz and Pauli work [1] (for recent reviews and related f(R) modifications, see [2])

  • The key steps in elaborating a modern version of a ghost free massive gravity theory were made in a series of papers: The so–called vDVZ discontinuity problem was solved using the Vainshtein mechanism [3], or following more recent approaches based on DGP model [4]

  • None solution was found for another problem with ghosts because at nonlinear order in massive gravity appears a sixth scalar degree of freedom as a ghost

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Summary

Introduction

The idea that graviton may have a nontrivial mass was proposed by Fierz and Pauli work [1] (for recent reviews and related f(R) modifications, see [2]). In our works [10, 9], we proved that it is possible to decouple and solve the gravitational field equations for a large class of gravity theories in very general forms (with coefficients of off–diagonal metrics and generalized connections depending on all spacetime variables).

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