paper

Interpreting map-based / spectral properties of CMB foregrounds

arXiv:2603.02177 · doi:10.1093/mnras/stag1432

Abstract

Map-space / decompositions of linear polarization are attractive for foreground and CMB analyses because they separate parity families: -family patterns directly contaminate primordial tensor searches, while -family patterns trace coherent Galactic structures. However, the / transform is not fully local and can induce apparent spectral complexity even when the underlying sky is spectrally simple in . We quantify this effect for synchrotron emission using complex log--Taylor and moment expansions for , its spin-preserving projections and , and its more standard scalar projections and . We relate the coefficients of these expansions to physical mechanisms such as line-of-sight mixing, synchrotron ageing, and Faraday effects. Using simple sky models, we show how and reorganize the spectral behaviour of into parity families with a clear geometric meaning. They retain interpretable amplitudes and angles and satisfy the closure relation , which extends to all moment orders. By contrast, scalar quantities such as and show larger induced variability of effective spectral parameters and enhanced spectral complexity, while lacks interpretable polarization amplitude and angle. Finally, we present simple CMB-oriented applications: three-frequency diagnostics to test whether the sky is better described by a power law in or by separate effective laws in , and idealized ILC and masking examples showing that the preferred map-space field depends on where foreground simplicity and residual contamination reside. This framework provides practical diagnostics for choosing foreground modelling, cleaning, and masking strategies in Galactic and CMB -mode analyses.

29 pages, 20 figures. Accepted for publication in MNRAS