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We consider the polarized Sunyaev-Zel'dovich (pSZ) effect for a tomographicprobe of cosmic birefringence, including all relevant terms of the pSZ effectin the cosmic microwave background (CMB) observables, some of which wereignored in the previous works. The pSZ effect produces late-time polarizationsignals from the scattering of the local temperature quadrupole seen by anelectron. We forecast the expected constraints on cosmic birefringence at thelate time of the universe with the pSZ effect. We find that the birefringenceangles at $2\lesssim z\lesssim 5$ are constrained at a subdegree level by thecross-correlations between CMB $E$- and $B$-modes or between CMB $B$-modes andremote quadrupole $E$-modes using data from LiteBIRD, CMB-S4, and LSST. Inparticular, the cross-correlation between large-scale CMB $B$-modes andremote-quadrupole $E$-modes has a much smaller bias from the Galacticforegrounds and is useful to cross-check the results from the $EB$ powerspectrum.

Cosmic birefringence tomography with polarized Sunyaev Zel'dovich effect