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S duality at the black hole threshold in gravitational collapse

Douglas M. Eardley, Eric W. Hirschmann, and James H. Horne
Phys. Rev. D 52, R5397(R) – Published 15 November 1995
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Abstract

We study gravitational collapse of the axion-dilaton field in classical low energy string theory, at the threshold for black hole formation. A new critical solution is derived that is spherically symmetric and continuously self-similar. The universal scaling and echoing behavior discovered by Choptuik in gravitational collapse appears in a somewhat different form. In particular, echoing takes the form of SL(2,R) rotations (cf., S duality). The collapse leaves behind an outgoing pulse of axion-dilaton radiation, with nearly but not exactly flat spacetime within it.

  • Received 22 May 1995

DOI:https://doi.org/10.1103/PhysRevD.52.R5397

©1995 American Physical Society

Authors & Affiliations

Douglas M. Eardley

  • Institute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030

Eric W. Hirschmann

  • Department of Physics, University of California, Santa Barbara, California 93106-9530

James H. Horne

  • Department of Applied Mathematics and Theoretical Physics, Silver St., Cambridge CB3 9EW, United Kingdom

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Vol. 52, Iss. 10 — 15 November 1995

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