2021 Preprint
Combining cosmological and local bounds on bimetric theory
Abstract: Ghost-free bimetric theory describes two nonlinearly interacting spin-2 fields, one massive and one massless, thus extending general relativity. We confront bimetric theory with observations of Supernovae type 1a, Baryon Acoustic Oscillations and the Cosmic Microwave Background in a statistical analysis, utilising the recently proposed physical parametrisation. This directly constrains the physical parameters of the theory, such as the mass of the spin-2 field and its coupling to matter. We find that all model…
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“…The presence of the massless graviton allows gravitational wave observations to be satisfied without severely restricting the parameter space of the theory [7], as opposed to many other modified gravity models. Bimetric gravity is also compatible with cosmological observations like the cosmic microwave background (CMB), type Ia supernovae (SNIa), and baryon acoustic oscillations (BAO) [8][9][10][11][12][13][14][15] and it exhibits a screening mechanism that restores general relativity results on solar-system scales [16][17][18][19][20][21]. Among the interesting properties of the theory are:…”
Section: Introductionmentioning
confidence: 53%
“…The presence of the massless graviton allows gravitational wave observations to be satisfied without severely restricting the parameter space of the theory [7], as opposed to many other modified gravity models. Bimetric gravity is also compatible with cosmological observations like the cosmic microwave background (CMB), type Ia supernovae (SNIa), and baryon acoustic oscillations (BAO) [8][9][10][11][12][13][14][15] and it exhibits a screening mechanism that restores general relativity results on solar-system scales [16][17][18][19][20][21]. Among the interesting properties of the theory are:…”
Section: Introductionmentioning
confidence: 53%
