Curvature Perturbations from Broken Symmetries
Edward W. Kolb, Antonio Riotto, Alberto Vallinotto
TL;DR
This work addresses how curvature perturbations can arise after slow-roll inflation in a multi-field setting with a broken global symmetry. It develops a general framework in which isocurvature fluctuations in the angular direction convert into curvature perturbations through inhomogeneous preheating, yielding $\zeta \approx \alpha \frac{\partial \ln(n_{\chi})}{\partial \phi_{\perp}} \delta\phi_{\perp}$ and a power spectrum $\mathcal{P}_{\zeta}(k)$ tied to the spectrum of $\delta\phi_{\perp}$. Applying the mechanism to a broken $U(1)$ potential with instant preheating, the authors derive explicit expressions for the preheating variables $|\phi_*|$ and $|\dot{\phi}_*|$, show how $\delta\theta_0$ modulates $n_{\chi}$, and obtain $\mathcal{P}_{\zeta}(k)$ with a nearly flat tilt $n-1 \approx 2\eta_1[1 - x\cos^2(\theta_0)]$, where $\eta_1 = m^2/(3H^2)$ and $x$ measures symmetry breaking. The results imply that broken-symmetry preheating can be a dominant source of curvature perturbations under certain conditions and provides a link between inflationary fluctuations and post-inflationary dynamics, akin to curvaton scenarios but without an external field.
Abstract
We present a new general mechanism to generate curvature perturbations after the end of the slow-roll phase of inflation. Our model is based on the simple assumption that the potential driving inflation is characterized by an underlying global symmetry which is slightly broken.
