Work in the Boyer-Lindquist coordinates exterior , away from the axes. There , , andInverting the block of the Kerr metric givesThus 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 , henceSo 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 givesBoth transverse terms are nonnegative in the exterior, so necessarilyBecause and the discriminant is , this is equivalent toEquality 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, andSince ,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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