Polynomial mixing for the weakly damped stochastic nonlinear Schrödinger equation on the whole space
Abstract
We consider the weakly damped stochastic nonlinear Schrödinger (NLS) equation on the real line, driven by a noise that is white in time and smooth in space. Assuming that the noise is sufficiently non-degenerate, we prove that the equation has a unique stationary measure in the class of probability measures concentrated on H2, and establish polynomial mixing in the dual-Lipschitz metric over H1. We do not impose any restriction on the size of the damping. The proof is based on a coupling argument, whose key ingredient is a Foiaş-Prodi-type estimate in the H1-norm, derived by means of a Lyapunov functional adapted to the linearized NLS dynamics. To compensate for the loss of compactness, we combine this estimate with a truncated Poincaré inequality and a space-time weight function quantifying the spatial decay of solutions.
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BibTeX
@misc{nersesyan2026polynomial,
title = {{Polynomial mixing for the weakly damped stochastic nonlinear Schrödinger equation on the whole space}},
author = {Vahagn Nersesyan and Tianyi Pan},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.08935},
eprint = {2609.08935},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.08935},
}
RIS
TY - UNPB
TI - Polynomial mixing for the weakly damped stochastic nonlinear Schrödinger equation on the whole space
AU - Vahagn Nersesyan
AU - Tianyi Pan
PY - 2026
DA - 2026/09/08
PB - arXiv
DO - 10.48550/arxiv.2609.08935
UR - https://arxiv.org/abs/2609.08935
AB - We consider the weakly damped stochastic nonlinear Schrödinger (NLS) equation on the real line, driven by a noise that is white in time and smooth in space. Assuming that the noise is sufficiently non-degenerate, we prove that the equation has a unique stationary measure in the class of probability measures concentrated on H^2, and establish polynomial mixing in the dual-Lipschitz metric over H^1. We do not impose any restriction on the size of the damping. The proof is based on a coupling argument, whose key ingredient is a Foiaş-Prodi-type estimate in the H^1-norm, derived by means of a Lyapunov functional adapted to the linearized NLS dynamics. To compensate for the loss of compactness, we combine this estimate with a truncated Poincaré inequality and a space-time weight function quantifying the spatial decay of solutions.
ER -