Chaos in the Einstein-Yang-Mills Equations

John D. Barrow and Janna Levin
Phys. Rev. Lett. 80, 656 – Published 26 January 1998
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Abstract

Yang-Mills color fields evolve chaotically in an anisotropically expanding universe. The chaotic behavior differs from that found in anisotropic mixmaster universes. The universe nears isotropy at late times, approaching the mean expansion rate of a radiation-dominated universe. However, small chaotic oscillations of the shear and color stresses continue indefinitely. An invariant characterization of the chaos is provided by means of fractal basin boundaries.

  • Received 17 June 1997

DOI:https://doi.org/10.1103/PhysRevLett.80.656

©1998 American Physical Society

Authors & Affiliations

John D. Barrow1 and Janna Levin2

  • 1Astronomy Centre, University of Sussex, Brighton BN1 9QJ, United Kingdom
  • 2Center for Particle Astrophysics, Le Conte Hall, University of California at Berkeley, Berkeley, California 94720-7304

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Vol. 80, Iss. 4 — 26 January 1998

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