arXiv · 0903.0631
Non-Gaussianity in a Matter Bounce
Abstract
A nonsingular bouncing cosmology in which the scales of interest today exit the Hubble radius in a matter-dominated contracting phase yields an alternative to inflation for producing a scale-invariant spectrum of adiabatic cosmological fluctuations. In this paper we identify signatures in the non-Gaussianities of the fluctuations which are specific to this scenario and allow it to be distinguished from the results of inflationary models.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Yi-Fu Cai, Wei Xue, Robert Brandenberger, Xinmin Zhang. 2009-03-08. Non-Gaussianity in a Matter Bounce. https://doi.org/10.1088/1475-7516%2F2009%2F05%2F011
Cite the original work for its findings. Save a collection to share your selection of sources.