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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://repozitorij.uni-lj.si/IzpisGradiva.php?id=159634"><dc:title>Kelvin-Helmholtz instability as one of the key features for fast and efficient emulsification by hydrodynamic cavitation</dc:title><dc:creator>Boček,	Žan	(Avtor)
	</dc:creator><dc:creator>Petkovšek,	Martin	(Avtor)
	</dc:creator><dc:creator>Clark,	Samuel J.	(Avtor)
	</dc:creator><dc:creator>Fezzaa,	Kamel	(Avtor)
	</dc:creator><dc:creator>Dular,	Matevž	(Avtor)
	</dc:creator><dc:subject>emulsion</dc:subject><dc:subject>hydrodynamic cavitation</dc:subject><dc:subject>Kelvin-Helmholtz instability</dc:subject><dc:subject>Venturi microchannels</dc:subject><dc:description>The paper investigates the oil–water emulsification process inside a micro-venturi channel. More specifically, the possible influence of Kelvin-Helmholtz instability on the emulsification process. High-speed visualizations were conducted inside a square venturi constriction with throat dimensions of 450 µm by 450 µm, both under visible light and X-Rays. We show that cavity shedding caused by the instability results in the formation of several cavity vortices. Their rotation causes the deformation of the oil stream into a distinct wave-like shape, combined with fragmentation into larger drops due to cavitation bubble collapse. Later on, the cavity collapse further disperses the larger drops into a finer emulsion. Thus, it turns out that the Kelvin-Helmholtz instability is similarly characteristic for hydrodynamic cavitation emulsification inside a microchannel as is the Rayleigh-Taylor instability for acoustically driven emulsion formation.</dc:description><dc:date>2024</dc:date><dc:date>2024-07-16 14:07:16</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>159634</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
