Adiabatic Gravitational Perturbation Growth During Preheating

Details Adiabatic Gravitational Perturbation Growth During Preheating Adiabatic Gravitational Perturbation Growth During Preheating

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cosm.conf..330m&link_type=abstract

COSMO-2000 . Proceedings of the Fourth International Workshop on Particle Physics and the Early Universe . Held 4-8 September 20

Physics

Scientific paper

The early Universe inflation11 is well known as a promising theory to explain the origin of large scale structure of the Universe, that is, an established causal theory for the origin of primordial density fluctuations which may interpret the observed density inhomogeneities and cosmic microwave fluctuations in the very early Universe. This theoretical framework can solve the early universe pressing problems in the standard Hot Big Bang theory1. In the single field inflation model, we study the possibilitis of parametric amplification of the gravitational perturbation, and we find that there is no additional growth of the super-horizon modes during reheating beyond the usual predictions by giving a general analytic explanation as well as the numerical results for it.

Affiliated with

Also associated with

No associations

Rating

Adiabatic Gravitational Perturbation Growth During Preheating 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 Adiabatic Gravitational Perturbation Growth During Preheating, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Adiabatic Gravitational Perturbation Growth During Preheating will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487469