Choose spin orientation so that ; the printed threshold assumes nonzero positive . Put and . The axial metric has components and determinant . Conserved energy and timelike normalization give
Eliminating gives the Kerr axial timelike effective potential
It extends through the zeros of in the regular original coordinates. Since , reaching zero requires . At equality the infalling orbit reaches zero with zero radial velocity and turns back, because the nearby negative sheet is forbidden. Along the axis zero is regular, unlike the off-axis ring.
For , and the global maximum is . If , an inward particle has no negative-sheet turning point. It passes through zero and continues toward , another asymptotically flat end, with and infinite proper time to infinity. It first crosses the outer and inner horizons. Perturbative Cauchy-horizon instability can invalidate this ideal Kerr axial analytic extension physically.
Figure 1.
Conformal blocks of the Kerr axis with an energetic timelike orbit continuing to negative-r infinity
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This is the two-dimensional axis restriction. The dashed curve is regular; the four-dimensional ring lies off-axis and is not an axial singular boundary.