aFermilab Particle Astrophysics Center, Box 500, Batavia, IL 60510, USA;bInstitut d’Astrophysique de Paris, 98 bis Blvd Arago, 75014 Paris, France
Abstract:
Here is discussed various ways by which the cosmic microwave background (CMB) radiation can be use to measure the velocities of matter in the universe. We include some new statistical techniques for using the kinetic Sunyaev–Zel’dovich (kSZ) effect and integrated Sachs–Wolfe (ISW) effect to determine velocities by correlating wide area CMB maps with overlapping large-scale structure (LSS) surveys.