Document Type
Article
Date
10-17-2003
Language
English
Disciplines
Physics
Description/Abstract
I discuss a mechanism that renders the spectral index of the primordial spectrum and the inflationary stage independent of each other. If a scalar field acquires an appropriate time-dependent mass, it is possible to generate an adiabatic, Gaussian scale invariant spectrum of density perturbations during any stage of inflation. As an illustration, I present a simple model where the time-dependent mass arises from the coupling of the inflaton to a second scalar. The mechanism I propose might help to implement a successful inflationary scenario in particle physics theories that do not yield slow-roll potentials.
Recommended Citation
Armendariz-Picon, Christian, "Liberating the Inflaton from Primordial Spectrum Constraints" (2003). Physics - All Scholarship. 218.
https://surface.syr.edu/phy/218
Source
Harvested from Arxiv.org
Additional Information
7 two-column pages, 1 figure. Uses RevTeX4 More information at http://arxiv.org/abs/astro-ph/0310512