Generation of dark radiation in the bulk inflaton model

Details Generation of dark radiation in the bulk inflaton model Generation of dark radiation in the bulk inflaton model

2003-01-05

arxiv.org/abs/gr-qc/0301010v3

Phys.Rev. D67 (2003) 104007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, no figures, references added, presentation improved, final version to be published in PRD

Scientific paper

10.1103/PhysRevD.67.104007

We investigate the dynamics of a bulk scalar field with various decay channels in the Randall-Sundrum infinite braneworld scenario. A bulk scalar field in this scenario has a quasi-localized mode which dominates the late-time behavior near the brane. As for this mode, an interesting point is the presence of dissipation caused by the escape of the energy in the direction away from the brane, even if the bulk scalar field does not have the interaction with the other bulk fields in the bulk and fields on the brane. We can interpret that this lost energy is transfered to the dark radiation. We show that such an effective 4-dimensional description for a bulk scalar field is valid including the various processes of energy dissipation.

Affiliated with

Also associated with

No associations

Rating

Generation of dark radiation in the bulk inflaton model 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 Generation of dark radiation in the bulk inflaton model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Generation of dark radiation in the bulk inflaton model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-220020