arXiv · 1206.3496
Growth Histories in Bimetric Massive Gravity
Abstract
We perform cosmological perturbation theory in Hassan-Rosen bimetric gravity for general homogeneous and isotropic backgrounds. In the de Sitter approximation, we obtain decoupled sets of massless and massive scalar gravitational fluctuations. Matter perturbations then evolve like in Einstein gravity. We perturb the future de Sitter regime by the ratio of matter to dark energy, producing quasi-de Sitter space. In this more general setting the massive and massless fluctuations mix. We argue that in the quasi-de Sitter regime, the growth of structure in bimetric gravity differs from that of Einstein gravity.
Explore related subjects
Keep this discovery
Marcus Berg, Igor Buchberger, Jonas Enander, Edvard Mortsell, Stefan Sjors. 2012-06-15. Growth Histories in Bimetric Massive Gravity. https://doi.org/10.1088/1475-7516%2F2012%2F12%2F021
Cite the original work for its findings. Save a collection to share your selection of sources.