Blast waves in a paraxial fluid of light
Murad Abuzarli, Tom Bienaim\'e, Elisabeth Giacobino, Alberto Bramati,, and Quentin Glorieux

TL;DR
This paper experimentally investigates blast wave dynamics in a paraxial fluid of light, revealing negative hydrostatic pressure signatures and comparing results with hydrodynamical models, demonstrating advanced control over optical fluid properties.
Contribution
It introduces experimental observation of blast wave phenomena in a paraxial fluid of light and compares measurements with hydrodynamic models, highlighting novel control over optical fluid dynamics.
Findings
Observation of negative hydrostatic pressure after localized over-density expansion
Comparison of velocity profiles with local speed of sound to identify supersonic regions
Demonstration of unprecedented control over hydrodynamic quantities in optical fluids
Abstract
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.
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