Wide-angle effects in multi-tracer power spectra with Doppler corrections

We examine the computation of wide-angle corrections to the galaxy power spec-trum including redshift-space distortions and relativistic Doppler corrections, and also includ-ing multiple tracers with differing clustering, magnification and evolution biases. We show that the inclusion of the relativistic Doppler contribution, as well as radial derivative terms, are crucial for a consistent wide-angle expansion for large-scale surveys, both in the single and multi-tracer cases. We also give for the first time the wide-angle cross-power spectrum associated with the Doppler magnification-galaxy cross correlation, which has been shown to be a new way to test general relativity. In the full-sky power spectrum, the wide-angle expansion allows integrals over products of spherical Bessel functions to be computed analyt-ically as distributional functions, which are then relatively simple to integrate over. We give for the first time a complete discussion and new derivation of the finite part of the divergent integrals of the form f0 infinity drrnje(kr)jj,(qr), which are necessary to compute the wide-angle corrections when a general window function is included. This facilitates a novel method for integrating a general analytic function against a pair of spherical Bessel functions.

Automated summary

This paper examines the computation of wide-angle corrections to the galaxy power spectrum, considering redshift-space distortions and relativistic Doppler corrections. It also includes multiple tracers with varying clustering, magnification, and evolution biases. The study emphasizes the importance of including the relativistic Doppler contribution and radial derivative terms for a consistent wide-angle expansion in large-scale surveys. Additionally, the authors present the wide-angle cross-power spectrum associated with the Doppler magnification-galaxy cross-correlation, which offers a new approach to test general relativity. The paper also introduces a method to analytically compute integrals involving products of spherical Bessel functions in the full-sky power spectrum.