Sampling methods to describe superradiance in large ensembles of quantum emitters
Daniel Eyles, Emmanuel Lassalle, Adam Stokes, Ramón Paniagua-Domínguez, Ahsan Nazir
TL;DR
This work addresses the challenge of computing the two-time photon correlation $g^{(2)}(t,\tau)$ for large ensembles of quantum emitters by introducing two sampling-based approaches that bound $\mathcal{G}^{(2)}(t,0)$: pairwise sampling (an upper bound) and $m$-wise sampling (a lower bound). The authors develop the theoretical framework linking the master equation to correlation functions and then demonstrate, through benchmarks on inverted arrays and coherently driven lattices, that offset-corrected versions of both methods provide tight bounds across regimes. A key finding is an empirical crossover at $N \approx 2m$ where the optimal method switches between $m$-wise and pairwise sampling, refined by analytic offset corrections derived from the independent-emitter limit. Collectively, these tools enable accurate, bounding predictions of superradiant photon statistics in large ensembles and arbitrary EM environments, offering practical guidance for choosing sampling parameters in simulations.
Abstract
Superradiance is a quantum phenomenon in which coherence between emitters results in enhanced and directional radiative emission. Many quantum optical phenomena can be characterized by the two-time quantum correlation function $g^{(2)}(t,τ)$, which describes the photon statistics of emitted radiation. However, the critical task of determining $g^{(2)}(t,τ)$ becomes intractable for large emitter ensembles due to the exponential scaling of the Hilbert space dimension with the number of emitters. Here, we analyse and benchmark two approximate numerical sampling methods applicable to emitter arrays embedded within electromagnetic environments, which generally provide upper and lower bounds for $g^{(2)}(t,0)$. We also introduce corrections to these methods (termed offset corrections) that significantly improve the quality of the predictions. The optimal choice of method depends on the total number of emitters, such that taken together, the two approaches provide accurate descriptions across a broad range of important regimes. This work therefore provides new theoretical tools for studying the well-known yet complex phenomenon of superradiance in large ensembles of quantum emitters.
