Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario

Details Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvd..58j3518b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 58, Issue 10, 15 November 1998, id. 103518

Physics

21

Particle-Theory And Field-Theory Models Of The Early Universe, Background Radiations

Scientific paper

A new model of warm inflation without slow-roll conditions for the scalar field is studied. Classicality conditions that must be satisfied to have an effective stochastic approach in the warm inflation scenario are analyzed for a general coarse-grained field, defined with a function that describes the long wavelength suppression. The theory can predict the spectral density of the fluctuations of the field which can be compared with the COBE data.

Affiliated with

Also associated with

No associations

Rating

Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario 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 Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-804899