arXiv · hep-th/0702165
A smooth bouncing cosmology with scale invariant spectrum
Abstract
We present a bouncing cosmology which evolves from the contracting to the expanding phase in a smooth way, without developing instabilities or pathologies and remaining in the regime of validity of 4d effective field theory. A nearly scale invariant spectrum of perturbations is generated during the contracting phase by an isocurvature scalar with a negative exponential potential and then converted to adiabatic. The model predicts a slightly blue spectrum, n_S >~ 1, no observable gravitational waves and a high (but model dependent) level of non-Gaussianities with local shape. The model represents an explicit and predictive alternative to inflation, although, at present, it is clearly less compelling.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Paolo Creminelli, Leonardo Senatore. 2007-11-01. A smooth bouncing cosmology with scale invariant spectrum. https://doi.org/10.1088/1475-7516%2F2007%2F11%2F010
Cite the original work for its findings. Save a collection to share your selection of sources.