Fig. 1

Motion of r illustrated schematically. It has been projected onto the equatorial plane of the black hole. The radial turning points are rtp1 and rtp2 between which the motion is confined. Point P indicates the position for a given p. The whole integral path is not monotonous and should be divided into several sections, each with a maximum proper length, such as DA, DG, HG, HI, PI. From the definitions of I0αr,I1αr, and I2αr (see text), one obtains ,
,
,
, and
, etc.
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