Fig. A.1

Geometry between the skewed disk plane and the equatorial plane of a black hole. The boundary of the disk is a ring, at which equal mass test particles are injected continuously. At the initial position, indicated by p, there are two orthonormal tetrads, i.e., {p, er,eθ,eφ} and {p, }. To compute the constants of motion, we need to transform the initial physical velocities of a particle
, which are specified by {p,
}, into {p, er,eθ,eφ}.
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