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.

Additional Information

7 two-column pages, 1 figure. Uses RevTeX4 More information at http://arxiv.org/abs/astro-ph/0310512

Source

Harvested from Arxiv.org

Included in

Physics Commons

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