FRW Cosmology in Ghost Free Massive Gravity

By D. Comelli, M. Crisostomi, L. Pilo, Fabrizio Nesti. 2011

145 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/44a6a16c62796254057d59a9ad86608bd0b6c5e7

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

On couplings to matter in massive (bi-)gravity (2014, background): “[44, 52–76]), with more success in its quasi-dilaton and bi-gravity extensions (see Refs.”
Cosmology and Fundamental Physics with the Euclid Satellite (2012, background): “The cosmology of bi-gravity was investigated for instance in [1215, 1217, 336] and subsequent literature (see [390] and [1216] for a review.”
Bimetric gravity is cosmologically viable (2015, methodology): “expansion history, even in the absence of vacuum energy [14–20].”
Cosmological tests of modified gravity (2015, background): “In this case, it is possible to find FRW solutions for both of the metrics [145, 146, 147].”
Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality (2012, methodology): “We have additionally assumed the same spatial curvature for the two metrics (k = −1, 0,+1) [28].”
Heavy spin-2 Dark Matter (2016, unknown): “[43–45].”
Cosmological stability bound in massive gravity and bigravity (2013, background): “One simple resolution is to look at massive gravity theories with an FRW reference metric [57] or for bigravity theories in which FRW solutions are allowed [21, 24, 24, 25, 30, 36, 47].”
Testing modified gravity at cosmological distances with LISA standard sirens (2019, background): “This information about homogeneous configurations is sufficient for the scope of this work, more details can be found in [139–142].”
Massive Gravity (2014, background): “2 Bi-gravity Cosmological solutions in bi-gravity have been considered in [474, 479, 104, 106, 8, 475, 478, 9, 7, 62].”