7 research outputs found

    Compensation of Beer-Lambert attenuation using non-diffracting Bessel beams

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    We report on a versatile method to compensate the linear attenuation in a medium, independently of its microscopic origin. The method exploits diffraction-limited Bessel beams and tailored on-axis intensity profiles which are generated using a phase-only spatial light modulator. This technique for compensating one of the most fundamental limiting processes in linear optics is shown to be efficient for a wide range of experimental conditions (modifying the refractive index and the attenuation coefficient). Finally, we explain how this method can be advantageously exploited in applications ranging from bio-imaging light sheet microscopy to quantum memories for future quantum communication networks

    Initiation à l'analyse spatiale à l'aide d'ArcView version 3.1

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    *INRA Centre de recherches de Nancy Laboratoire d'Intelligence Artificielle et Biométrie - 54280 Champenoux Diffusion du document : INRA Centre de recherches de Nancy Laboratoire d'Intelligence Artificielle et Biométrie - 54280 ChampenouxNational audienc

    Blast waves in a paraxial fluid of light

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    We study experimentally blast wave dynamics on a weakly interacting fluid of light. The fluid density and velocity are measured in 1D and 2D geometries. Using a state equation arising from the analogy between optical propagation in the paraxial approximation and the hydrodynamic Euler's equation, we access the fluid hydrostatic and dynamic pressure. In the 2D configuration, we observe a negative differential hydrostatic pressure after the fast expansion of a localized over-density, which is a typical signature of a blast wave for compressible gases. Our experimental results are compared to the Friedlander waveform hydrodynamical model. Velocity measurements are presented in 1D and 2D configurations and compared to the local speed of sound, to identify supersonic region of the fluid. Our findings show an unprecedented control over hydrodynamic quantities in a paraxial fluid of light

    Analogue cosmological particle creation in an ultracold quantum fluid of light

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    In inflationary cosmology, the rapid expansion of the early universe resulted in the spontaneous production of cosmological particles from vacuum fluctuations, observable today in the cosmic microwave background anisotropies. The analogue of cosmological particle creation in a quantum fluid could provide insight, but an observation has not yet been achieved. Here we report the spontaneous creation of analogue cosmological particles in the laboratory, using a quenched 3-dimensional quantum fluid of light. We observe acoustic peaks in the density power spectrum, in close quantitative agreement with the quantum-field theoretical prediction. We find that the long-wavelength particles provide a window to early times, and we apply this principle to the cosmic microwave background. This work introduces a new quantum fluid, as cold as an atomic Bose-Einstein condensate.Comment: 7 pages for the main text and 7 pages of supplementary materia

    De la carte des Naudin à la carte IGN : précision et déformations spatiales de la feuille de Nancy

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    *INRA Centre de Nancy (FRA) Diffusion du document : INRA Centre de Nancy (FRA)National audienc
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