Non-Gaussianity in Curvaton Models with Nearly Quadratic Potential
Kari Enqvist, Sami Nurmi
TL;DR
This paper investigates how small departures from a purely quadratic curvaton potential affect primordial non-Gaussianity. Using the separate-universe framework, the authors derive the curvature perturbation $\zeta$ to second order and show that the non-Gaussianity parameter $f_{NL}$ acquires a potential-dependent term that vanishes for a strictly quadratic potential. By introducing a near-quadratic self-interaction $\lambda m^{4-n}_{\sigma}\sigma^n$, they compute the induced corrections to the curvaton oscillation amplitude and obtain an analytic expression for $f_{NL}$, revealing that $|f_{NL}|$ can be suppressed (or enhanced) relative to the quadratic case depending on the exponent $n$ and the correction size $s$. In the limit of small curvaton energy density $r\ll1$, the potential correction can allow $|f_{NL}|$ to be much less than unity, relaxing the usual lower bound on $r$ and showing that current non-Gaussianity constraints do not generically rule out curvaton models without specifying higher-order terms in the potential.
Abstract
We consider curvaton models with potentials that depart slightly from the quadratic form. We show that although such a small departure does not modify significantly the Gaussian part of the curvature perturbation, it can have a pronounced effect on the level of non-Gaussianity. We find that unlike in the quadratic case, the limit of small non-Gaussianity, $|f_{NL}|\ll1$, is quite possible even with small curvaton energy density $r\ll1$ . Furthermore, non-Gaussianity does not imply any strict bounds on $r$ but the bounds depend on the assumptions about the higher order terms in the curvaton potential.
