Mach's Principle, the Kerr Metric, and Black-Hole Physics

Brendan B. Godfrey
Phys. Rev. D 1, 2721 – Published 15 May 1970
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Abstract

The generalized Kerr solution is tentatively accepted as the description for the state of a charged rotating mass which has undergone complete gravitational collapse. Mass accretion by such a system is demonstrated to damp out the rotation. Even the most favorable selective capture of matter leaves the angular momentum bounded by m2, precisely the upper limit that the Kerr geometry can accommodate without change of character. Mach's principle, exemplified by the rotation of inertial frames, is employed to obtain approximate expressions for perihelion precession of satellites, deflection of light trajectories, and the rotation of polarization of light. Results are compared with exact expressions, when available.

  • Received 2 October 1969

DOI:https://doi.org/10.1103/PhysRevD.1.2721

©1970 American Physical Society

Authors & Affiliations

Brendan B. Godfrey*

  • Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08540

  • *National Science Foundation Predoctoral Fellow, 1967-1970.

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Vol. 1, Iss. 10 — 15 May 1970

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