Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2007-07-13
JCAP0708:003,2007
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, no figure, added references
Scientific paper
10.1088/1475-7516/2007/08/003
We consider a curvaton scenario in which the late-time domination and the generation of the curvature perturbation is achieved by a non-oscillatory (NO) curvaton potential. Instead of considering the conventional curvaton oscillation, we consider ``weak trapping'' after preheating, which modifies the evolution of the curvaton density after preheating. The primordial isocurvature perturbation related to the curvaton is once converted into the fluctuation of the number density of the preheat field through inhomogeneous preheating. Then the evolution of the curvatons and the preheat field is controlled by the preheat-field number density. The density of these fields decreases slightly slower than the standard matter density which suggests that these fields will grow with time. Finally, the preheat field decays to reheat the Universe leaving behind the curvature perturbation. In our scenario the task of the standard curvaton is not executed solely by the curvaton itself but is partially shared with the preheat field. NO curvatons can be considered as the hybrid version of the quintessential inflationary model.
No associations
LandOfFree
NO Curvatons or Hybrid Quintessential 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 NO Curvatons or Hybrid Quintessential Inflation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NO Curvatons or Hybrid Quintessential Inflation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-60234