Regularization of the Teukolsky Equation for Rotating Black Holes
arXiv:gr-qc/9707017 · doi:10.1103/PhysRevD.56.6363
Abstract
We show that the radial Teukolsky equation (in the frequency domain) with sources that extend to infinity has well-behaved solutions. To prove that, we follow Poisson approach to regularize the non-rotating hole, and extend it to the rotating case. To do so we use the Chandrasekhar transformation among the Teukolsky and Regge-Wheeler-like equations, and express the integrals over the source in terms of solutions to the homogeneous Regge-Wheeler-like equation, to finally regularize the resulting integral. We then discuss the applicability of these results.
14 pages, 1 Table, REVTEX
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