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arXiv · 2305.07695

Dissipative Inflation via Scalar Production

Paolo Creminelli·Soubhik Kumar·Borna Salehian·Luca Santoni
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Abstract

We describe a new mechanism that gives rise to dissipation during cosmic inflation. In the simplest implementation, the mechanism requires the presence of a massive scalar field with a softly-broken global $U(1)$ symmetry, along with the inflaton field. Particle production in this scenario takes place on parametrically sub-horizon scales, at variance with the case of dissipation into gauge fields. Consequently, the backreaction of the produced particles on the inflationary dynamics can be treated in a \textit{local} manner, allowing us to compute their effects analytically. We determine the parametric dependence of the power spectrum which deviates from the usual slow-roll expression. Non-Gaussianities are always sizeable whenever perturbations are generated by the noise induced by dissipation: $f_{\rm NL}^{\rm eq} \gtrsim {O}(10)$.

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Paolo Creminelli, Soubhik Kumar, Borna Salehian, Luca Santoni. 2023-05-12. Dissipative Inflation via Scalar Production. https://arxiv.org/abs/2305.07695

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