Paraxial fluid of light in hot atomic vapors
Quentin Fontaine

TL;DR
This paper investigates superfluid behavior of light in hot rubidium vapors, demonstrating linear dispersion of density waves and conditions for superfluidity in a cavityless photon fluid system.
Contribution
It provides experimental evidence of superfluidity in a propagating photon fluid in hot atomic vapors, a cavityless system, through dispersion measurements and defect flow experiments.
Findings
Linear dispersion relation observed for small wave-vectors
Superfluid flow demonstrated by drag force cancellation
Photon fluid exhibits superfluid characteristics in hot rubidium vapors
Abstract
Quantum fluids of light are the photonic counterpart of Bose gases. They currently attract increasing interest since they are versatile and highly tunable systems for probing many-body physics quantum phenomena, such as superfluidity. Superfluid flow of light has already been reported in microcavity exciton-polariton condensates but clear observation of this phenomenon in cavityless systems, that is, for propagating photon fluids, remains elusive. In this thesis, we study the hydrodynamical properties of light propagating close to resonance in hot rubidium vapors. Whereas photons in air are not interacting with each other, the situation is different in rubidium vapors, as an effective interaction between them, mediated by the atomic ensemble, appears. The light behaves therefore as a fluid flowing in the plane perpendicular to the optical axis. The primary purpose of this thesis was to…
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Taxonomy
TopicsStrong Light-Matter Interactions · Cold Atom Physics and Bose-Einstein Condensates · Nonlinear Photonic Systems
