Correlation properties of a one-dimensional repulsive Bose gas at finite temperature

We present a comprehensive study shedding light on how thermal fluctuations affect correlations in a Bose gas with contact repulsive interactions in one spatial dimension. The pair correlation function, the static structure factor, and the one-body density matrix are calculated as a function of the...

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Bibliographic Details
Authors: Rosi, Giulia de|||0000-0003-3236-0628, Rota, Riccardo, Astrakharchik, Grigori|||0000-0003-0394-8094, Boronat Medico, Jordi|||0000-0002-0273-3457
Format: article
Publication Date:2023
Country:España
Institution:Universitat Politècnica de Catalunya (UPC)
Repository:UPCommons. Portal del coneixement obert de la UPC
Language:English
OAI Identifier:oai:upcommons.upc.edu:2117/386957
Online Access:https://hdl.handle.net/2117/386957
https://dx.doi.org/10.1088/1367-2630/acc6e6
Access Level:Open access
Keyword:Bose-Einstein gas
Monte Carlo method
Bose-Einstein condensation
One-dimensional Bose gases
Temperature
Correlations
Pair correlation function
Static structure factor
One-body density matrix
Path Integral Monte Carlo
Montecarlo, Mètode de
Condensació de Bose-Einstein
Àrees temàtiques de la UPC::Física::Termodinàmica
Description
Summary:We present a comprehensive study shedding light on how thermal fluctuations affect correlations in a Bose gas with contact repulsive interactions in one spatial dimension. The pair correlation function, the static structure factor, and the one-body density matrix are calculated as a function of the interaction strength and temperature with the exact ab-initio Path Integral Monte Carlo method. We explore all possible gas regimes from weak to strong interactions and from low to high temperatures. We provide a detailed comparison with a number of theories, such as perturbative (Bogoliubov and decoherent classical), effective (Luttinger liquid) and exact (ground-state and thermal Bethe Ansatz) ones. Our Monte Carlo results exhibit an excellent agreement with the tractable limits and provide a fundamental benchmark for future observations which can be achieved in atomic gases, cavity quantum-electrodynamic and superconducting-circuit platforms.