Primordial trispectra and CMB spectral distortions

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 $g_{\mathrm{N}\mathrm{L}}$ and ${\tau }_{\mathrm{N}\mathrm{L}}$. 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 $both$ $g_{\mathrm{N}\mathrm{L}}$ and ${\tau }_{\mathrm{N}\mathrm{L}}$-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 ${\tau }_{\mathrm{N}\mathrm{L}}$-component. A simple Fisher matrix-based forecast shows that a futuristic, cosmic-variance dominated experiment could in principle detect $g_{\mathrm{N}\mathrm{L}}\sim 0.4$ and ${\tau }_{\mathrm{N}\mathrm{L}}\sim 40$ using $TT\mu$.