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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.

Curvature Perturbations from Broken Symmetries

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 and a power spectrum tied to the spectrum of . Applying the mechanism to a broken potential with instant preheating, the authors derive explicit expressions for the preheating variables and , show how modulates , and obtain with a nearly flat tilt , where and 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.

Paper Structure

This paper contains 8 sections, 48 equations, 4 figures.

Figures (4)

  • Figure 1: Two background trajectories arising from fluctuations in the initial conditions in the case in which the background field space is two dimensional. Also shown are the equipotential contours (units of $10^{-16} M_p^4$). The potential used in this figure is the one given in Eq. (\ref{['App:V']}) and further analyzed in Sec. \ref{['sect:Application']}, which is characterized by a global $U(1)$ broken symmetry. In this case, and for illustration purposes only, the symmetry breaking parameter has been arbitrarily set to $x=0.15$.
  • Figure 2: Values of $f(\theta_0)$ obtained through numerical simulation and using the approximate expression given in Eq. (\ref{['App:deltanchinchi2']}) for a value of the symmetry breaking parameter of $x=0.05$ and for a coupling constant $g=0.01$.
  • Figure 3: Values of $|\phi_*|/(|\phi_0|\pi x /2\sqrt{2})$ obtained through numerical simulation and using the above approximate expression Eq. (\ref{['Append:lapprox']}) for a value of the symmetry breaking parameter of $x=0.05$.
  • Figure 4: Values of $|\dot{\phi}_*|/|\dot{\tilde{\phi}}_*|$ obtained through numerical simulation and using the approximate expression Eq. (\ref{['Append:m3']}) for a value of the symmetry breaking parameter of $x=0.05$.