Large amplitude waves in magnetized plasmas, generated either by external
pumps or internal instabilities, can scatter via three-waves interactions.
While three-wave scatterings in either forward or backward geometry are
well-known, what happens when waves propagate at angles with one another in
magnetized plasmas remains largely unknown, mainly due to the analytical
difficulty of this problem. In this paper, we overcome this analytical
difficulty and find a convenient formula for three-wave coupling coefficients
in cold, uniform, magnetized plasmas in the most general geometry. This is
achieved by systematically solving the fluid-Maxwell model to second order
using a multiscale perturbative expansion. The general formula for the coupling
coefficient becomes transparent when we reformulate it as the S matrix element
of a quantized Lagrangian. Using the quantized Lagrangian, it is possible to
bypass the perturbative solution and directly obtain the nonlinear coupling
coefficient from the linear response of plasmas. To illustrate how to evaluate
the cold coupling coefficient, we give a set of examples where the
participating waves are either quasi-transverse or quasi-longitudinal. In these
examples, we determine the angular dependence of three-wave scattering, and
demonstrate that backscattering is not necessarily the strongest scattering
channel in magnetized plasmas, in contrast to what happens in unmgnetized
plasmas. Our approach gives a more complete picture, beyond the simple
collimated geometry, of how injected waves can decay in magnetic confinement
devices, as well as how lasers can be scattered in magnetized plasma targets