Thermalization in Quantum Fluids of Light: A Convection-Diffusion Equation

Fuente: arXiv
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Main Authors: Shishkov, Vladislav Yu., Panyukov, Ivan V., Andrianov, Evgeny S., Zasedatelev, Anton V.
Format: Preprint
Published: 2025
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author Shishkov, Vladislav Yu.
Panyukov, Ivan V.
Andrianov, Evgeny S.
Zasedatelev, Anton V.
author_facet Shishkov, Vladislav Yu.
Panyukov, Ivan V.
Andrianov, Evgeny S.
Zasedatelev, Anton V.
contents We develop a microscopic theory for the dynamics of quantum fluids of light, deriving an effective kinetic equation in momentum space that takes the form of the convection-diffusion equation. In the particular case of two-dimensional systems with parabolic dispersion, it reduces to the Bateman--Burgers equation. The hydrodynamic analogy unifies nonlinear wave phenomena, such as shock wave formation and turbulence, with non-equilibrium Bose--Einstein condensation of photons and polaritons in optical cavities. We introduce the Reynolds number $(\textit{Re})$ and demonstrate that the condensation threshold corresponds exactly to a critical Reynolds number of unity $(\textit{Re}=1)$, beyond which $(\textit{Re} > 1)$ a shock-like front emerges in the momentum space, characterized by the Bose--Einstein distribution for the particle density in states with high momentum.
format Preprint
id arxiv_https___arxiv_org_abs_2501_10537
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Thermalization in Quantum Fluids of Light: A Convection-Diffusion Equation
Shishkov, Vladislav Yu.
Panyukov, Ivan V.
Andrianov, Evgeny S.
Zasedatelev, Anton V.
Quantum Gases
We develop a microscopic theory for the dynamics of quantum fluids of light, deriving an effective kinetic equation in momentum space that takes the form of the convection-diffusion equation. In the particular case of two-dimensional systems with parabolic dispersion, it reduces to the Bateman--Burgers equation. The hydrodynamic analogy unifies nonlinear wave phenomena, such as shock wave formation and turbulence, with non-equilibrium Bose--Einstein condensation of photons and polaritons in optical cavities. We introduce the Reynolds number $(\textit{Re})$ and demonstrate that the condensation threshold corresponds exactly to a critical Reynolds number of unity $(\textit{Re}=1)$, beyond which $(\textit{Re} > 1)$ a shock-like front emerges in the momentum space, characterized by the Bose--Einstein distribution for the particle density in states with high momentum.
title Thermalization in Quantum Fluids of Light: A Convection-Diffusion Equation
topic Quantum Gases
url https://arxiv.org/abs/2501.10537