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Analog Hawking radiation from a spin-sonic horizon in a two-component Bose–Einstein condensate
[Rayonnement de Hawking par l’horizon analogue de spin dans un condensat de Bose–Einstein à deux composantes]
Comptes Rendus. Physique, Online first (2024), pp. 1-36.

Nous étudions théoriquement l’émission de Hawking stimulée et spontanée à partir d’un horizon analogue pour les modes de spin dans un condensat de Bose–Einstein à deux composants, avec et sans couplage cohérent entre les deux composants. Nous mettons en évidence les avantages conceptuels et pratiques que ces systèmes offrent pour l’observation expérimentale du phénomène, à savoir la possibilité d’avoir des excitations élémentaires massives et l’accessibilité expérimentale des différentes quadratures des excitations de spin. Plus specifiquement, nous allons au-delà des régimes relativistes précédemment abordés dans la littérature, et identifions des observables qui montrent une signature du processus de Hawking, ainsi que des caractéristiques supplémentaires associées à la nature massive des modes, telles que des ondulations. Les calculs semi-analytiques des propriétés de reflexion et transmission de l’horizon et des fonctions de corrélation à deux points du rayonnement émis dans un cadre stationnaire idéal sont confirmés par des simulations numériques dépendantes du temps basées sur les théories de Gross–Pitaevskii et de Bogoliubov.

We theoretically study stimulated and spontaneous Hawking emission from an analog horizon for spin modes in a two-component Bose–Einstein condensate, both with and without a coherent coupling between the two components. We highlight the conceptual and practical advantages that these systems offer to the experimental observation of the phenomenon, namely the possibility of working with massive elementary excitations and the experimental accessibility of the different quadratures of the spin excitations. In particular, we go beyond the relativistic regimes previously addressed in the literature, and identify various observables that show a signature of the Hawking process, as well as additional features associated with the massive nature of the modes, such as undulations. Semi-analytical calculations of the scattering properties of the horizon and of two-point correlation functions of the emitted radiation in an ideal stationary setup are supported by time-dependent numerical simulations based on Gross–Pitaevskii and Bogoliubov theory.

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DOI : 10.5802/crphys.226
Keywords: Hawking radiation, Analog gravity, Two-component Bose–Einstein condensate
Mots-clés : Rayonnement de Hawking, Gravité analogue, Condensats de Bose–Einstein à deux composantes

Anna Berti 1 ; Lennart Fernandes 2, 3 ; Salvatore Butera 4 ; Alessio  Recati 1 ; Michiel Wouters 3 ; Iacopo Carusotto 1

1 Pitaevskii BEC Center, INO-CNR and Dipartimento di Fisica, University of Trento, Italy
2 Center for Quantum Phenomena, Department of Physics, New York University, USA
3 Theory of Quantum and Complex Systems, University of Antwerp, Belgium
4 School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
Licence : CC-BY 4.0
Droits d'auteur : Les auteurs conservent leurs droits
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     author = {Anna Berti and Lennart Fernandes and Salvatore Butera and Alessio ~Recati and Michiel Wouters and Iacopo Carusotto},
     title = {Analog {Hawking} radiation from a spin-sonic horizon in a two-component {Bose{\textendash}Einstein} condensate},
     journal = {Comptes Rendus. Physique},
     publisher = {Acad\'emie des sciences, Paris},
     year = {2024},
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Anna Berti; Lennart Fernandes; Salvatore Butera; Alessio  Recati; Michiel Wouters; Iacopo Carusotto. Analog Hawking radiation from a spin-sonic horizon in a two-component Bose–Einstein condensate. Comptes Rendus. Physique, Online first (2024), pp. 1-36. doi : 10.5802/crphys.226.

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