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Can the CMB be Odd? Effect of a Parity-Violating Matter 4-Point Function on the Low-â„“\ell CMB Trispectrum

Published 20 Oct 2025 in astro-ph.CO | (2510.18065v1)

Abstract: Here we explore from a theoretical perspective the sensitivity of the primary CMB anisotropy trispectrum to parity violation (PV) in large-scale structure (LSS). We focus on the Sachs-Wolfe term, which dominates at $\ell &lt; 40$, after which the Doppler term takes over. We consider a model where the PV is only present out to some maximal scale RR of order a few hundred Mpc/hh, consistent with what recent LSS 4PCF measurements seem to indicate. We find that the odd CMB trispectrum must be suppressed by at least one factor of R/χ<em>R/\chi_<em>\simeq1%,with1\%, with \chi_$ the distance to last scattering, relative to the input matter 4PCF. Thus, a non-detection of PV in the CMB trispectrum is \textit{not necessarily inconsistent} with a genuine detection of PV in the LSS 4PCF.

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