Inflationary perturbations with multiple scalar fields

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

11 pages, 2 figures. Talk given at COSMO-01 Workshop, Rovaniemi, Finland, August 30 - September 4, 2001

Scientific paper

The calculation of scalar gravitational and matter perturbations during multiple-field inflation valid to first order in slow roll is discussed. These fields may be the coordinates of a non-trivial field manifold and hence have non-minimal kinetic terms. A basis for these perturbations determined by the background dynamics is introduced, and the slow-roll functions are generalized to the multiple-field case. Solutions for a perturbation mode in its three different behavioural regimes are combined, leading to an analytic expression for the correlator of the gravitational potential. Multiple-field effects caused by the coupling to the field perturbation perpendicular to the field velocity can even contribute at leading order. This is illustrated numerically with an example of a quadratic potential. (The material here is based on previous work by the authors presented in hep-ph/0107272.)

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Inflationary perturbations with multiple scalar fields 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 Inflationary perturbations with multiple scalar fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inflationary perturbations with multiple scalar fields will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-118080

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.