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We analyze the d’Alembert equation in the Goedel-type spacetimes with spherical and Lobachevsky sections (with sufficiently rapid rotation). By separating the and dependence we reduce the problem to a group-theoretical one. In the spherical case solutions have discrete frequencies, and involve spin-weighted spherical harmonics. In the Lobachevsky case we give simple formulas for obtaining all the solutions belonging to the sectors of the irreducible unitary representations of the reduced Lorentz group. The wave equation enforces restrictions on and the allowed (here: continuous) spectrum of frequencies.

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