ed in Section 4.1 , including gravitational lensing, the Vishniac effect accounting for matter velocities and flows into local potential wells, and the Sunyaev-Zel’dovich (SZ) (Section 4.5.4 ) distortions from the Compton scattering of CMB photons by electrons in the hot cluster medium) can also be fairly significant.
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Computational Cosmology: From the Early Universe to the Large Scale Structure.
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