Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-10-17
JCAP 0403 (2004) 009
Astronomy and Astrophysics
Astrophysics
7 two-column pages, 1 figure. Uses RevTeX4
Scientific paper
10.1088/1475-7516/2004/03/009
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.
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