Signatures of Non-Gaussianity in the Curvaton Model
Kari Enqvist, Tomo Takahashi
TL;DR
The paper investigates primordial non-Gaussianity in the curvaton model when the curvaton potential includes non-quadratic terms. Using the $ abla N$ formalism, it derives expressions for the bispectrum and trispectrum parameters, showing that $f_{ m NL}$ can be driven to very small values while the trispectrum parameter $g_{ m NL}$ becomes large and negative for small $r$, making the trispectrum a key observable. The authors demonstrate that $g_{ m NL}$ directly measures deviations from a purely quadratic potential, predicting magnitudes around $|g_{ m NL}|\,\sim\,O(10^4)-O(10^5)$ in plausible scenarios, with $ au_{ m NL}$ tied to $f_{ m NL}$ via $ au_{ m NL}=\frac{36}{25} f_{ m NL}^2$. These results imply that future observations, including Planck, could test MSSM-inspired curvaton models by targeting the trispectrum rather than the bispectrum.
Abstract
We discuss the signatures of non-Gaussianity in the curvaton model where the potential includes also a non-quadratic term. In such a case the non-linearity parameter f_NL can become very small, and we show that non-Gaussianity is then encoded in the non-reducible non-linearity parameter g_NL of the trispectrum, which can be very large. Thus the place to look for the non-Gaussianity in the curvaton model may be the trispectrum rather than the bispectrum. We also show that g_NL measures directly the deviation of the curvaton potential from the purely quadratic form. While g_NL depends on the strength of the non-quadratic terms relative to the quadratic one, we find that for reasonable cases roughly g_NL\sim O(-10^4)-O(-10^5), which are values that may well be accessible by future observations.
