Emergent universe in Hor̆ava gravity

Details Emergent universe in Hor̆ava gravity Emergent universe in Hor̆ava gravity

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.331..665m&link_type=abstract

Astrophysics and Space Science, Volume 331, Issue 2, pp.665-671

Astronomy and Astrophysics

Astrophysics

5

Emergent Universe, Hor̆Ava Gravity

Scientific paper

Recently Hor̆ava has proposed a non-relativistic renormalisable gravity theory with higher spatial derivatives in four dimensions which reduces to Einstein's gravity at large distances with a non-vanishing cosmological constant but with improved UV behaviour. In this paper, we have considered the Friedman-Lemaître-Robertson-Walker cosmological model in Hor̆ava gravity and the emergent scenario for all values of the spatial curvature k (=0,±1) has been studied. As a result, there are constraints on the parameters involved.

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