Boost operator approach to the relativistic polarized SZ effect

ABSTRACT We extend the recent boost operator formalism for relativistic Compton scattering calculations to also account for polarization. This allows us to provide general, exact expressions for the polarized Sunyaev–Zeldovich (SZ) effect sourced both kinematically and from intrinsic anisotropies of the Cosmic Microwave Background. The results are given in terms of rational operator functions that can be used to generate distortion spectra that describe the general SZ signal, reproducing the classical polarized SZ results in the appropriate limits. Our derivation allows for clear separation of physical effects in the generation of polarized SZ, and beyond the SZ application provides a general description of the Compton collision term in the Doppler-dominated regime. Through direct computation of important example cases we further illustrate the power of this new method.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-02-17
DOI
https://doi.org/10.1093/mnras/stag331
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Boost operator approach to the relativistic polarized SZ effect

Erik Rosenberg, Jens Chluba
Monthly Notices of the Royal Astronomical Society
Dark Matter and Cosmic Phenomena
article

Boost operator approach to the relativistic polarized SZ effect

Erik Rosenberg, Jens Chluba
article en

Abstract

ABSTRACT We extend the recent boost operator formalism for relativistic Compton scattering calculations to also account for polarization. This allows us to provide general, exact expressions for the polarized Sunyaev–Zeldovich (SZ) effect sourced both kinematically and from intrinsic anisotropies of the Cosmic Microwave Background. The results are given in terms of rational operator functions that can be used to generate distortion spectra that describe the general SZ signal, reproducing the classical polarized SZ results in the appropriate limits. Our derivation allows for clear separation of physical effects in the generation of polarized SZ, and beyond the SZ application provides a general description of the Compton collision term in the Doppler-dominated regime. Through direct computation of important example cases we further illustrate the power of this new method.

Monthly Notices of the Royal Astronomical SocietyVol. 547(2)
University of Manchester (GB)
Openalex Percentile: Top 51%
Dark Matter and Cosmic Phenomena
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