Cosmological bounds on open FLRW solutions of massive gravity

preprint2015arXivOpen access

Abstract

In this work we have analysed some cosmological bounds concerning an open FLRW solution of massive gravity. The constraints with recent observational H(z)H(z) data were found and the best fit values for the cosmological parameters are in agreement with the ΛΛCDM model, and also point to a nearly open spatial curvature, as expected from the model. The graviton mass dependence with the constant parameters α3α_3 and α4α_4, related to the additional lagrangians terms of the model, are also analysed, and we have obtained a strong dependence with such parameters, although the condition mg≃H0−1m_g\simeq H_0^{-1} seems dominant for a long range of the parameters α3α_3 and α4α_4.

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.