Wave equations in conformally separable, accreting, rotating black holes

Abstract

The Teukolsky wave equations governing fields of spin 0, $\frac{1}{2}$, 1, $\frac{3}{2}$, and 2 are generalized to the case of conformally separable solutions for accreting, rotating black holes.

arXiv commentv1: 25 pages. v2: minor updates to agree with published version; 26 pages

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Cited by in corpus (2)

• Hawking radiation inside a rotating black hole
• Backreaction from quantum fluxes at the Kerr inner horizon