Stochastic dark energy from inflationary quantum fluctuations
Abstract
We study the quantum backreaction from inflationary fluctuations of a very light, non-minimally coupled spectator scalar and show that it is a viable candiate for dark energy. The problem is solved by suitably adapting the formalism of stochastic inflation. This allows us to self-consistently account for the backreaction on the background expansion rate of the Universe where its effects are large. This framework is equivalent to that of semiclassical gravity in which matter vacuum fluctuations are included at the one loop level, but purely quantum gravitational fluctuations are neglected. Our results show that dark energy in our model can be characterized by a distinct effective equation of state parameter (as a function of redshift) which allows for testing of the model at the level of the background.
Keywords
Cite
@article{arxiv.1710.07824,
title = {Stochastic dark energy from inflationary quantum fluctuations},
author = {Dražen Glavan and Tomislav Prokopec and Alexei A. Starobinsky},
journal= {arXiv preprint arXiv:1710.07824},
year = {2018}
}
Comments
32 pages, 5 figures; published version, significant changes