Effective dynamics of strongly dissipative Rydberg gases
M Marcuzzi, J Schick, B Olmos, I Lesanovsky

TL;DR
This paper derives effective classical and quantum models for strongly dissipative Rydberg gases, simplifying their dynamics and revealing the limits of classical approximations under different dissipation regimes.
Contribution
It introduces a systematic derivation of effective equations of motion for dissipative Rydberg gases, highlighting when classical rate equations are valid and when quantum coherences are preserved.
Findings
Effective classical rate equations describe the dynamics up to second order in dephasing.
Fourth order corrections break positivity, indicating limitations of classical descriptions.
Second order expansion in EIT systems retains quantum coherences.
Abstract
We investigate the evolution of interacting Rydberg gases in the limit of strong noise and dissipation. Starting from a description in terms of a Markovian quantum master equation we derive effective equations of motion that govern the dynamics on a "coarse-grained" timescale where fast dissipative degrees of freedom have been adiabatically eliminated. Specifically, we consider two scenarios which are of relevance for current theoretical and experimental studies --- Rydberg atoms in a two-level (spin) approximation subject to strong dephasing noise as well as Rydberg atoms under so-called electromagnetically induced transparency (EIT) conditions and fast radiative decay. In the former case we find that the effective dynamics is described by classical rate equations up to second order in an appropriate perturbative expansion. This drastically reduces the computational complexity of…
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