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    Sonic black holes with thick horizons in BECs

    Daniel Peñalver1,*, Marco De Vito1,†, Roberto Balbinot2,‡, and Alessandro Fabbri1,§

    • *Contact author: Daniel.Penalver@ific.uv.es
    • †Contact author: mardevi@ific.uv.es
    • ‡Contact author: Roberto.Balbinot@bo.infn.it
    • §Contact author: afabbri@ific.uv.es

    Phys. Rev. D 114, 065030 – Published 29 September, 2026

    DOI: https://doi.org/10.1103/8hsh-96jl

    Abstract

    We consider simple one dimensional models of acoustic black holes formed by Bose-Einstein condensates where the flow is stepwise homogeneous. We concentrate on the case in which an extended sonic region is present, i.e., a region where the flow velocity equals exactly the speed of sound. These models can be thought of as acoustic black holes with a thick horizon. Particular attention is devoted to the number of created particles and to the density-density correlation functions, these latter being at present time the experimental tool to identify Hawking-like radiation in acoustic black holes.

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