Wave equations in conformally separable, accreting, rotating black holes
Andrew J. S. Hamilton, Tyler McMaken
TL;DR
This paper generalizes the Teukolsky wave equations to conformally separable solutions for accreting, rotating black holes, expanding the mathematical framework for analyzing various field spins in such spacetimes.
Contribution
It introduces a new formulation of wave equations applicable to accreting, rotating black holes with conformal separability, extending previous models.
Findings
Generalized Teukolsky equations for conformally separable black holes
Applicable to fields of spins 0, 1/2, 1, 3/2, and 2
Provides a foundation for future analytical and numerical studies
Abstract
The Teukolsky wave equations governing fields of spin 0, , 1, , and 2 are generalized to the case of conformally separable solutions for accreting, rotating black holes.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Pulsars and Gravitational Waves Research · Geophysics and Sensor Technology