Cosmological Solution Moduli of Bigravity
arXiv:1503.02811 · doi:10.1088/1475-7516/2015/09/062
Abstract
We construct the complete set of metric-configuration solutions of the ghost-free massive bigravity for the scenario in which the g-metric is the Friedmann-Lemaitre-Robertson-Walker (FLRW) one, and the interaction Lagrangian between the two metrics contributes an effective ideal fluid energy-momentum tensor to the g-metric equations. This set corresponds to the exact background cosmological solution space of the theory.
33 pages
References in corpus (15)
- Resummation of Massive Gravity
- Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
- On couplings to matter in massive (bi-)gravity
- Stable and unstable cosmological models in bimetric massive gravity
- Viable cosmology in bimetric theory
- Viable cosmological solutions in massive bimetric gravity
- Massive gravity from bimetric gravity
- FRW Cosmological Perturbations in Massive Bigravity
- Particular Solutions in Bimetric Theory and Their Implications
- Cosmological perturbations in massive gravity with doubly coupled matter
- Null Energy Condition violations in bimetric gravity
- Gordon and Kerr-Schild ansatze in massive and bimetric gravity
- Properties of Bigravity Solutions in a Solvable Class
- Effective Matter Cosmologies of Massive Gravity I: Non-Physical Fluids
- Effective Matter Cosmologies of Massive Gravity: Physical Fluids