Kerr spin produces longer or shorter proper infall times than Schwarzschild for equatorial geodesics, with the difference encoded in the Raychaudhuri integrand via expansion and shear.
Volonteri, Astronomy and Astrophysics Review18, 279 (2010)
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Covariant interpretation of proper infall times in Kerr spacetime
Kerr spin produces longer or shorter proper infall times than Schwarzschild for equatorial geodesics, with the difference encoded in the Raychaudhuri integrand via expansion and shear.