Inflation and the Origin of Large-Scale Structure

Details Inflation and the Origin of Large-Scale Structure Inflation and the Origin of Large-Scale Structure

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..736...71w&link_type=abstract

PHI IN THE SKY: The Quest for Cosmological Scalar Fields. AIP Conference Proceedings, Volume 736, pp. 71-83 (2004).

Mathematics

Logic

Particle-Theory And Field-Theory Models Of The Early Universe, Superclusters, Large-Scale Structure Of The Universe, Field Theory

Scientific paper

Primordial perturbations in the density of radiation and matter can be related to vacuum fluctuations of scalar fields during inflation in the very early universe. In the standard inflaton scenario this inevitably leads to a Gaussian distribution of adiabatic density perturbations, but alternative models such as the curvaton scenario or inhomogeneous reheating can yield non-Gaussian or non-adiabatic signatures.

Affiliated with

Also associated with

No associations

Rating

Inflation and the Origin of Large-Scale Structure does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Inflation and the Origin of Large-Scale Structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inflation and the Origin of Large-Scale Structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1008695