Work in the Boyer-Lindquist coordinates exterior , away from the axes. There , , and
Inverting the block of the Kerr metric gives
Thus has , and the smooth nonvanishing timelike vector field defines a time orientation. Choose it future-directed, matching increasing near infinity. For every nonzero future causal vector , the Lorentzian inner product satisfies , hence
So increases strictly along every regular future causal curve in this exterior. Notice that itself can be spacelike in the Kerr ergoregion; the timelike object used here is . Direct substitution also gives .
For a regular causal curve, orient its tangent toward the future; reversing its parametrization does not change . Since , use as parameter and set . The causal inequality gives
Both transverse terms are nonnegative in the exterior, so necessarily
Because and the discriminant is , this is equivalent to
Equality requires and a null tangent. The limiting vectors are the two local azimuthal null directions; a curve following one at constant radius need not be a null geodesic. For a curve with radial or polar motion these angular bounds are necessary, while the full causal inequality can impose stricter bounds.
In the open exterior Kerr ergoregion, and
Since ,
so even the lower permitted angular velocity is positive. Every regular causal trajectory in the ergoregion has : it must co-rotate with the Kerr black hole. At the outer stationary-limit surface , the lower bound is zero; strict positivity is asserted in the open ergoregion. The sign reverses if the orientation of is reversed.

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