The black hole and the pea

Neil J. Cornish and Norman E. Frankel
Phys. Rev. D 56, 1903 – Published 15 August 1997
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Abstract

Like a fairy-tale princess, trajectories around black holes can be sensitive to small disturbances. We describe how a small disturbance can lead to erratic orbits and an increased production of gravitational waves.

  • Received 13 June 1996

DOI:https://doi.org/10.1103/PhysRevD.56.1903

©1997 American Physical Society

Authors & Affiliations

Neil J. Cornish

  • DAMTP, University of Cambridge, Silver Street, Cambridge CB3 9EW, United Kingdom

Norman E. Frankel

  • School of Physics, University of Melbourne, Parkville 3052, Victoria, Australia

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Issue

Vol. 56, Iss. 4 — 15 August 1997

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