Abstract

It is interesting to observe that all optical materials with a positive refractive index have a value of index that is of order unity. Surprisingly, though, a deep understanding of the mechanisms that lead to this universal behavior seems to be lacking. Moreover, this observation is difficult to reconcile with the fact that a single, isolated atom is known to have a giant optical response, as characterized by a resonant scattering cross section that far exceeds its physical size. Here, we theoretically and numerically investigate the evolution of the optical properties of an ensemble of ideal atoms as a function of density, starting from the dilute gas limit, including the effects of multiple scattering and near-field interactions. Interestingly, despite the giant response of an isolated atom, we find that the maximum index does not indefinitely grow with increasing density, but rather reaches a limiting value $n\approx 1.7$. We propose an explanation based upon strong-disorder renormalization group theory, in which the near-field interaction combined with random atomic positions results in an inhomogeneous broadening of atomic resonance frequencies. This mechanism ensures that regardless of the physical atomic density, light at any given frequency only interacts with at most a few near-resonant atoms per cubic wavelength, thus limiting the maximum index attainable. Our work is a promising first step to understand the limits of refractive index from a bottom-up, atomic physics perspective, and also introduces renormalization group as a powerful tool to understand the generally complex problem of multiple scattering of light overall.

Highlights

  • One interesting observation is that all the optical materials that we know of, with a positive index of refraction at visible wavelengths, universally have an index of order unity, n ∼ Oð1Þ

  • In large-scale numerics, we find that the maximum index does not indefinitely grow with density, and it saturates to a maximum value of n ≈ 1.7, when the typical distance between atoms becomes smaller than the length scale associated with the resonant cross section, i.e., d < λ0

  • We have shown that despite the large resonant scattering cross section of a single atom, a dense atomic medium does not exhibit an anomalously large optical response

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Summary

INTRODUCTION

Our RG theory is based upon the key intuition gained in the collective scattering of just two atoms to build up an understanding of the many-atom problem in a hierarchical manner. (6) and (7) (with the near-field interactions of renormalized atoms suitably removed; see Appendix B) to calculate the maximum real index (optimized over detunings) as a function of density η of the ensemble with renormalized resonance frequencies. After the system is mapped to an inhomogeneously broadened distribution, PðωeffÞ, where near-field interactions and the influence of single neighbors are seen to be strongly reduced, one can apply a smooth medium approximation. We stress that the emergence of a finite bound to the maximum index predicted by Eq (10) can be directly related to the invariance of the distribution Pðωeff=ηÞ and to the linear growth of broadening with density

FORMAL THEORY OF MULTIPLE SCATTERING
COUPLED-DIPOLE SIMULATIONS
MICROSCOPIC JUSTIFICATION OF THE RG SCHEME
Comparison of eigenvalue distributions
Multipolar nature of collective modes
Near-field interaction involving renormalized atoms
Near-field vs far-field interactions
Linewidths in the RG prescription
CONCLUSIONS
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