Sonic black holes in dilute Bose-Einstein condensates

L. J. Garay, J. R. Anglin, J. I. Cirac, and P. Zoller
Phys. Rev. A 63, 023611 – Published 17 January 2001
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Abstract

The sonic analog of a gravitational black hole in dilute-gas Bose-Einstein condensates is investigated. It is shown that there exist both dynamically stable and unstable configurations which, in the hydrodynamic limit, exhibit behaviors completely analogous to that of gravitational black holes. The dynamical instabilities involve the creation of quasiparticle pairs in positive and negative energy states. We illustrate these features in two qualitatively different one-dimensional models, namely, a long, thin condensate with an outcoupler laser beam providing an “atom sink,” and a tight ring-shaped condensate. We also simulate the creation of a stable sonic black hole by solving the Gross-Pitaevskii equation numerically for a condensate subject to a trapping potential which is adiabatically deformed. A sonic black hole could, in this way, be created experimentally with state-of-the-art or planned technology.

  • Received 30 May 2000

DOI:https://doi.org/10.1103/PhysRevA.63.023611

©2001 American Physical Society

Authors & Affiliations

L. J. Garay1,2, J. R. Anglin1,3, J. I. Cirac1, and P. Zoller1

  • 1Institut für Theoretische Physik, Universität Innsbruck, Technikerstrasse 25, A-6020 Innsbruck, Austria
  • 2Instituto de Matemáticas y Física Fundamental, CSIC, C/ Serrano 121, E-28006 Madrid, Spain
  • 3Institute for Theoretical Atomic and Molecular Physics, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02135

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Vol. 63, Iss. 2 — February 2001

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