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Stationary acoustic black hole solutions in Bose-Einstein condensates and their Borel analysis

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arxiv 2411.06678 v2 pith:LQTOWAJH submitted 2024-11-11 cond-mat.quant-gas gr-qcmath-phmath.MPquant-ph

classification cond-mat.quant-gasgr-qcmath-phmath.MPquant-ph
keywords solutionsblackspeedholesoundacousticbose-einsteincondensate
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In this article, we study the dynamics of a Bose-Einstein condensate (BEC) with the idea of finding solutions that could possibly correspond to a so-called acoustic (or Unruh) black/white holes. Those are flows with horizons where the speed of the flow goes from sub-sonic to super-sonic. This is because sound cannot go back from the supersonic to the subsonic region. The speed of sound plays the role of the speed of light in a gravitational black hole, an important difference being that there are excitations that can go faster than the speed of sound and therefore can escape the sonic black hole. Here, the motion of the BEC is described by the Gross-Pitaevskii Equation (GPE). More concretely, we discuss singular Stationary solutions of Gross-Pitaevskii equation in 2D (with Circular symmetry) and 3D (with Spherical symmetry). We use these solutions to study the local speed of sound and magnitude of flow velocity of the condensate to see whether they cross, indicating the potential existence of a sonic analog of a black/white hole. We discuss numerical techniques used and also study the semi-analytical Laplace-Borel resummation of asymptotic series solutions to see how well they agree with numerical solutions. We also study how the resurgent transseries plays a role in these solutions.

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  1. Acoustic black holes, white holes, and wormholes in Bose-Einstein condensates in two dimensions

    cond-mat.quant-gas 2024-12 conditional novelty 6.0 of 10

    Stationary Gross-Pitaevskii solutions on a funnel-like metric produce sonic black/white hole and wormhole analogues with closed-form Hawking temperatures for uniform-density cases.

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