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Main Authors: Berti, Anna, Fernandes, Lennart, Butera, Salvatore Giulio, Recati, Alessio, Wouters, Michiel, Carusotto, Iacopo
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2408.17292
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author Berti, Anna
Fernandes, Lennart
Butera, Salvatore Giulio
Recati, Alessio
Wouters, Michiel
Carusotto, Iacopo
author_facet Berti, Anna
Fernandes, Lennart
Butera, Salvatore Giulio
Recati, Alessio
Wouters, Michiel
Carusotto, Iacopo
contents 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 massive nature of 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.
format Preprint
id arxiv_https___arxiv_org_abs_2408_17292
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Analog Hawking radiation from a spin-sonic horizon in a two-component Bose-Einstein condensate
Berti, Anna
Fernandes, Lennart
Butera, Salvatore Giulio
Recati, Alessio
Wouters, Michiel
Carusotto, Iacopo
Quantum Gases
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 massive nature of 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.
title Analog Hawking radiation from a spin-sonic horizon in a two-component Bose-Einstein condensate
topic Quantum Gases
url https://arxiv.org/abs/2408.17292