Quantifying the breakdown of the rotating-wave approximation in single-photon superradiance
Mads Anders J{\o}rgensen, Martijn Wubs

TL;DR
This paper quantitatively analyzes how the rotating-wave approximation (RWA) affects the calculation of collective light emission in quantum emitters, revealing significant deviations in interaction strength and emission properties, especially for multiple emitters.
Contribution
It provides a detailed comparison between full light-matter interaction and RWA-based models, highlighting the conditions under which RWA introduces substantial errors in collective emission predictions.
Findings
RWA reduces interatomic interaction strength by up to a factor of two in free space.
Errors due to RWA can diverge in the near field for scalar models.
RWA impacts collective emission spectra and decay rates, especially for multiple emitters.
Abstract
We study quantitatively the breakdown of the rotating-wave approximation when calculating collective light emission by quantum emitters, in particular in the weak-excitation limit. Our starting point is a known multiple-scattering formalism where the full light-matter interaction leads to induced inter-emitter interactions described by the classical Green function of inhomogeneous dielectric media. When making the RWA in the light-matter interaction, however, these induced interactions differ from the classical Green function, and for free space we find a reduction of the interatomic interaction strength by up to a factor of two. By contrast, for the corresponding scalar model the relative RWA error for the inter-emitter interaction even diverges in the near field. For two identical emitters, the errors due to the RWA in collective light emission will show up in the emission spectrum,…
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