Bimetric Gravity, Variable Speed of Light Cosmology and Planck2013
J. W. Moffat

TL;DR
This paper presents a bimetric gravity model with a variable speed of light that aligns with Planck 2013 data, solving key cosmological problems without inflation or multiverse assumptions.
Contribution
It introduces a novel bimetric gravity framework with variable light speed that matches observed CMB fluctuations and addresses horizon, flatness, and fine-tuning issues.
Findings
Scalar spectral index n_s ≈ 0.96
Running of spectral index α_s ≈ 8×10^{-4}
Model fits Planck 2013 CMB data
Abstract
A bimetric gravity model with a variable speed of light is shown to be in agreement with the results reported from the Planck satellite in 2013. The predicted scalar mode spectral index is and its running is when the fundamental length scale in the model is fixed to be , where is the Planck length , giving the observed CMB fluctuations: . The enlarged lightcone ensures that horizon and flatness problems are solved. The model is free from many of the fine-tuning problems of the inflationary models and the fluctuations that form the seeds of structure formation do not lead to a chaotic inhomogeneous universe and the need for a multiverse.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
