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Bogoliubov Theory of acoustic Hawking radiation in Bose-Einstein Condensates

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arxiv 0907.4305 v1 pith:NY26UJQB submitted 2009-07-24 cond-mat.quant-gas

Bogoliubov Theory of acoustic Hawking radiation in Bose-Einstein Condensates

classification cond-mat.quant-gas
keywords hawkinganalyticalbogoliubovbose-einsteincondensatecondensatesdensityhorizon
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We apply the microscopic Bogoliubov theory of dilute Bose-Einstein condensates to analyze quantum and thermal fluctuations in a flowing atomic condensate in the presence of a sonic horizon. For the simplest case of a step-like horizon, closed-form analytical expressions are found for the spectral distribution of the analog Hawking radiation and for the density correlation function. The peculiar long-distance density correlations that appear as a consequence of the Hawking emission features turns out to be reinforced by a finite initial temperature of the condensate. The analytical results are in good quantitative agreement with first principle numerical calculations.

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Cited by 2 Pith papers

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  1. Exploring Event Horizons and Hawking Radiation through Deformed Graphene Membranes

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    Simulations indicate that negative-curvature graphene membranes can form stable analogue horizons whose local density of states exhibits thermal character at a few tens of Kelvin.

  2. Decrease of the entanglement entropy of the Hawking radiation induced by backreaction in the Bose-Einstein condensate

    hep-th 2026-04 unverdicted novelty 4.0

    Backreaction in a BEC analog black hole causes the entanglement entropy of Hawking radiation to decrease for sufficiently low energy modes across a wide parameter range.