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

Abstract

We examine the computation of wide-angle corrections to the galaxy power spectrum including redshift-space distortions and relativistic Doppler corrections, and also including 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 analytically 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 ${\int }_0^{\infty }\mathrm{d}r{r}^n{j}_{\ell }(kr)j_{{\ell }^{\prime }}(qr)$, 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.

41 pages and 2 figures. V3 has substantial improvements and new results. V4 is to appear in JCAP

References in corpus (6)

• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• The observed galaxy power spectrum in General Relativity
• Modeling relativistic contributions to the halo power spectrum dipole
• Magnification and evolution biases in large-scale structure surveys
• Constraining spatial curvature with large-scale structure
• Wide-angle and relativistic effects in Fourier-space clustering statistics

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• Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys
• Detecting Relativistic Doppler in Galaxy Clustering with Tailored Galaxy Samples
• Multi-tracing the primordial Universe with future surveys
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• Multipoles of the galaxy bispectrum on a light cone: wide-separation and relativistic corrections
• Large-scale Modeling of the Observed Power Spectrum Multipoles
• Cosmic magnification in beyond-Horndeski gravity