Scalar perturbation spectra from warm inflation
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- 29 April 2004
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 69 (8), 083525
- https://doi.org/10.1103/physrevd.69.083525
Abstract
We present a numerical integration of the cosmological scalar perturbation equations in warm inflation. The initial conditions are provided by a discussion of the thermal fluctuations of an inflaton field and thermal radiation using a combination of thermal field theory and thermodynamics. The perturbation equations include the effects of a damping coefficient and a thermodynamic potential V. We give an analytic expression for the spectral index of scalar fluctuations in terms of a new slow-roll parameter constructed from A series of toy models, inspired by spontaneous symmetry breaking and a known form of the damping coefficient, lead to a spectrum with on large scales and on small scales.
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