High Density Preheating Effects on Q-ball Decays and MSSM Inflation

Details High Density Preheating Effects on Q-ball Decays and MSSM Inflation High Density Preheating Effects on Q-ball Decays and MSSM Inflation

2005-10-14

arxiv.org/abs/hep-ph/0510186v1

Phys.Rev.Lett. 96 (2006) 031303

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages

Scientific paper

10.1103/PhysRevLett.96.031303

Non-perturbative preheating decay of post-inflationary condensates often results in a high density, low momenta, non-thermal gas. In the case where the non-perturbative classical evolution also leads to Q-balls, this effect shields them from instant dissociation, and may radically change the thermal history of the universe. For example, in a large class of inflationary scenarios, motivated by the MSSM and its embedding in string theory, the reheat temperature changes by a multiplicative factor of $10^{12}$.

Affiliated with

Also associated with

No associations

Rating

High Density Preheating Effects on Q-ball Decays and MSSM Inflation 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 High Density Preheating Effects on Q-ball Decays and MSSM Inflation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Density Preheating Effects on Q-ball Decays and MSSM Inflation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-222655