pith. sign in

arxiv: hep-th/0310296 · v2 · submitted 2003-10-31 · ✦ hep-th · astro-ph· gr-qc

Quantum effects and stability of chameleon cosmology

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

One possibility to explain the current accelerated expansion of the universe may be related with the presence of cosmologically evolving scalar whose mass depends on the local matter density (chameleon cosmology). We point out that matter quantum effects in such scalar-tensor theory produce the chameleon scalar field dependent conformal anomaly. Such conformal anomaly adds higher derivative terms to chameleon field equation of motion. As a result, the principal possibility for instabilities appears. These instabilities seem to be irrelevant at small curvature but may become dangerous in the regions where gravitational field is strong.

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.