Bimetric Gravity, Variable Speed of Light Cosmology and Planck2013

preprint2013arXivOpen access

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 ns≈0.96n_s\approx 0.96 and its running is αs≈8×10−4α_s\approx 8\times 10^{-4} when the fundamental length scale ℓ0\ell_0 in the model is fixed to be ℓ0≈105ℓP\ell_0\approx 10^5\ell_P, where ℓP\ell_P is the Planck length ℓP=1.62×10−33 cm\ell_P=1.62\times 10^{-33}\,{\rm cm}, giving the observed CMB fluctuations: δH≈10−5δ_H\approx 10^{-5}. 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.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.