Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2001-03-05
Phys.Rev.Lett.83:5423-5426,1999
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
10 pages, Latex; This version is almost identical to the one previously published in Phys. Rev. Lett
Scientific paper
10.1103/PhysRevLett.83.5423
We calculate the asymptotic behavior of the curvature scalar $(Riemann)^2$ near the null weak singularity at the inner horizon of a generic spinning black hole, and show that this scalar oscillates infinite number of times while diverging. The dominant parallelly-propagated Riemann components oscillate in a similar manner. This oscillatory behavior, which is in a remarkable contrast to the monotonic mass-inflation singularity in spherical charged black holes, is caused by the dragging of inertial frames due to the black- hole's spin.
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