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.
Chandrasekhar,The Mathematical Theory of Black Holes(Oxford University Press, 1983)
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2years
2026 2representative citing papers
citing papers explorer
-
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.
- Breaking Parameter Degeneracies in a Magnetically Charged Black Hole Embedded in a Hernquist Dark-Matter Halo: A Multi-Observable Analysis