Constraints on variations in inflaton decay rate from modulated preheating
Arindam Mazumdar, Kamakshya Prasad Modak

TL;DR
This paper investigates how modulated preheating can contribute to CMB perturbations, finding that its impact is limited to less than 15% of total perturbations unless parameters are finely tuned, especially if the modulating field is dark matter.
Contribution
It introduces constraints on the contribution of modulated preheating to CMB perturbations, considering the role of the modulating scalar as dark matter or not.
Findings
Modulated preheating can contribute up to 15% of CMB perturbations.
Fine tuning is required if the modulating scalar is dark matter.
Constraints on non-gaussianity and iso-curvature perturbations are established.
Abstract
Modulated (p)reheating is thought to be an alternative mechanism for producing super-horizon curvature perturbations in CMB. But large non-gaussianity and iso-curvature perturbations produced by this mechanism rule out its acceptability as the sole process responsible for generating CMB perturbations. We explore the situation where CMB perturbations are mostly generated by usual quantum fluctuations of inflaton during inflation, but a modulated coupling constant between inflaton and a secondary scalar affects the preheating process and produces some extra curvature perturbations. If the modulating scalar field is considered to be a dark matter candidate, coupling constant between the fields has to be unnaturally fine tuned in order to keep the local-form non-gaussianity and the amplitude of iso-curvature perturbations within observational limit; otherwise parameters of the models have…
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