Primordial trispectra and CMB spectral distortions

TL;DR

This paper investigates how primordial non-Gaussianity parameters $g_{ m NL}$ and $ au_{ m NL}$ influence the $TT ext{-} extmu$ bispectrum in the CMB, suggesting potential detection with future experiments.

Contribution

It provides a detailed analysis of the $TT ext{-} extmu$ bispectrum's dependence on primordial trispectrum parameters and compares full calculations with physical expectations.

Findings

Both $g_{ m NL}$ and $ au_{ m NL}$ contribute to the $TT ext{-} extmu$ signal.

The $TT ext{-} extmu$ bispectrum can potentially detect $g_{ m NL} ext{~and}~ au_{ m NL}$ with future experiments.

The $ ext{ extmu} ext{ extmu}$ auto-correlation is only sensitive to $ au_{ m NL}$.

Abstract

We study the $TT\mu$ bispectrum, generated by correlations between Cosmic Microwave Background temperature (T) anisotropies and chemical potential ($\mu$) distortions, and we analyze its dependence on primordial local trispectrum parameters $g_{\rm NL}$ and $\tau_{\rm NL}$. We cross-check our results by comparing the full bispectrum calculation with the expectations from a general physical argument, based on predicting the shape of $\mu$-T correlations from the couplings between short and long perturbation modes induced by primordial non-Gaussianity. We show that $both$ $g_{\rm NL}$ and $\tau_{\rm NL}$-parts of the primordial trispectrum source a non-vanishing $TT\mu$ signal, contrary to the $\mu\mu$ auto-correlation function, which is sensitive only to the $\tau_{\rm NL}$-component. A simple Fisher matrix-based forecast shows that a futuristic, cosmic-variance dominated experiment could in principle detect $g_{\rm NL} \sim 0.4$ and $\tau_{\rm NL} \sim 40$ using $TT\mu$.