pith. sign in

arxiv: 0801.4526 · v2 · submitted 2008-01-29 · ✦ hep-th · astro-ph· gr-qc

Pseudo-redundant vacuum energy

classification ✦ hep-th astro-phgr-qc
keywords energymodelsconstantcosmologicalcouplingcurvaturedarkgravity
0
0 comments X
read the original abstract

We discuss models that can account for today's dark energy. The underlying cosmological constant may be Planck scale but starts as a redundant coupling which can be eliminated by a field redefinition. The observed vacuum energy arises when the redundancy is explicitly broken, say by a non-minimal coupling to curvature. We give a recipe for constructing models, including R + 1/R type models, that realize this mechanism and satisfy all solar system constraints on gravity. A similar model, based on Gauss-Bonnet gravity, provides a technically natural explanation for dark energy and exhibits an interesting see-saw behavior: a large underlying cosmological constant gives rise to both low and high curvature solutions. Such models could be statistically favored in the string landscape.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.