A Test of Horava Gravity: The Dark Energy

TL;DR

This paper tests a modified version of Horava gravity in a cosmological setting, analyzing its compatibility with current dark energy observations and deriving constraints on its parameters.

Contribution

It introduces an IR modification to Horava gravity and evaluates its consistency with observational data, providing new constraints on dark energy parameters.

Findings

IR modified Horava gravity aligns with current observational data

Constraints on dark energy parameters w_0 and w_a are derived

Future refined data can test the theory's validity

Abstract

Recently Horava proposed a renormalizable gravity theory with higher spatial derivatives in four dimensions which reduces to Einstein gravity with a non-vanishing cosmological constant in IR but with improved UV behaviors. Here, I consider a non-trivial test of the new gravity theory in FRW universe by considering an IR modification which breaks "softly" the detailed balance condition in the original Horava model. I separate the dark energy parts from the usual Einstein gravity parts in the Friedman equations and obtain the formula of the equations of state parameter. The IR modified Horava gravity seems to be consistent with the current observational data but we need some more refined data sets to see whether the theory is really consistent with our universe. From the consistency of our theory, I obtain some constraints on the allowed values of w_0 and w_a in the Chevallier, Polarski, and Linder's parametrization and this may be tested in the near future, by sharpening the data sets.