Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB $E$-mode and $\mu$-distortion anisotropies

Abstract

Multi-field inflation models and non-Bunch-Davies vacuum initial conditions both predict sizeable non-Gaussian primordial perturbations and anisotropic $\mu$-type spectral distortions of the cosmic microwave background (CMB) blackbody. While CMB anisotropies allow us to probe non-Gaussianity at wavenumbers $k\simeq 0.05\mathrm{Mp}{\mathrm{c}}^{-1}$, $\mu$-distortion anisotropies are related to non-Gaussianity of primordial perturbation modes with much larger wavenumbers, $k\simeq 740\mathrm{Mp}{\mathrm{c}}^{-1}$. Through cross-correlations between CMB and $\mu$-distortion anisotropies, one can therefore shed light on the aforementioned inflation models. We investigate the ability of a future CMB satellite imager like LiteBIRD to measure $\mu T$ and $\mu E$ cross-power spectra between anisotropic $\mu$-distortions and CMB temperature and $E$-mode polarization anisotropies in the presence of foregrounds, and derive LiteBIRD forecasts on $f_{\mathrm{NL}}^{\mu }(k\simeq 740\mathrm{Mp}{\mathrm{c}}^{-1})$. We show that $\mu E$ cross-correlations with CMB polarization provide more constraining power on $f_{\mathrm{NL}}^{\mu }$ than $\mu T$ cross-correlations in the presence of foregrounds, and the joint combination of $\mu T$ and $\mu E$ observables adds further leverage to the detection of small-scale primordial non-Gaussianity. We find that LiteBIRD would detect $f_{\mathrm{NL}}^{\mu }=4500$ at $5\sigma$ significance after foreground removal, and achieve a minimum error of $\sigma (f_{\mathrm{NL}}^{\mu }=0)\simeq 800$ at 68\% CL by combining CMB temperature and polarization. Due to the huge dynamic range of wavenumbers between CMB and $\mu$-distortion anisotropies, such large $f_{\mathrm{NL}}^{\mu }$ values would still be consistent with current CMB constraints in the case of very mild scale-dependence of primordial non-Gaussianity. Anisotropic spectral distortions thus provide a new path, complementary to CMB $B$-modes, to probe inflation with LiteBIRD.

17 pages, 11 figures, updated to match version accepted by MNRAS

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Cited by in corpus (2)

• CMB spectral distortions revisited: a new take on $\mu$ distortions and primordial non-Gaussianities from FIRAS data
• Non-Gaussianity constraints from Planck spectral distortion cross-correlations