Intrinsic characterization of the separation constant for spin one and gravitational perturbations in Kerr geometry

DOI10.1098/rspa.1996.0050zbMath0867.53068OpenAlexW2068291581MaRDI QIDQ4716826

George C. Williams, Willard jun. Miller, Ernest G. Kalnins

Publication date: 11 August 1997

Published in: Proceedings of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1098/rspa.1996.0050

zbMATH Keywords

separation of variablesgravitational perturbationsKerr geometryHertz potential formalism

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (3)

Debye potentials for Maxwell and Dirac fields from a generalization of the Killing–Yano equation ⋮ Generalized hidden symmetries and the Kerr-Sen black hole ⋮ On the stability of the massive scalar field in Kerr space-time

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