Phys. Rev. Lett. 32, 243 (1974) - Axisymmetric Stability of Kerr Black Holes

Axisymmetric Stability of Kerr Black Holes

John L. Friedman and Bernard F. Schutz, Jr.

Phys. Rev. Lett. 32, 243 – Published 4 February 1974

Abstract

A variational expression is used to prove that all axisymmetric modes of the Kerr sequence of rotating black holes are stable.

Received 30 November 1973

DOI:https://doi.org/10.1103/PhysRevLett.32.243

©1974 American Physical Society

Authors & Affiliations

John L. Friedman and Bernard F. Schutz, Jr.

Yale University, New Haven, Connecticut 06520

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Issue

Vol. 32, Iss. 5 — 4 February 1974

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