<?xml version="1.0"?>
<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Optical responses from high entropy alloys</dc:title><dc:creator>Nominé,	Alexandre	(Avtor)
	</dc:creator><dc:creator>Solomonov,	Alexander I.	(Avtor)
	</dc:creator><dc:creator>Polanšek,	Juš	(Avtor)
	</dc:creator><dc:creator>Zavašnik,	Janez	(Avtor)
	</dc:creator><dc:creator>Cvelbar,	Uroš	(Avtor)
	</dc:creator><dc:creator>Milichko,	Valentin A.	(Avtor)
	</dc:creator><dc:subject>high entropy alloys</dc:subject><dc:subject>optical properties</dc:subject><dc:description>High-entropy alloys (HEAs) combine five or more elements in near-equiatomic ratios, opening an immense compositional space whose optical behaviour is still largely unknown. Phase-modulated ellipsometry on bulk CrMnFeCoNi (Cantor) shows that its intrinsic optical constants n, k, ε1, ε2 deviate strongly from the arithmetic mean of the constituent elements—by up to a factor of two beyond 1 µm—yet the derived functional responses, reflectance R and absorption coefficient α, are reproduced to within ~20 %. Cantor nanoparticles have been produced by nanosecond electric discharges in liquid nitrogen. Dark-field spectroscopy and Mie calculations reveal a dominant scattering mode near 100 nm that red-shifts and broadens with increasing size; the steady-state photothermal rise calculated from absorption cross-section σabs falls between those of the constituent pure metals.Generalising the averaging rule, we compute proxy values of R and α for 10 994 density-functional-theory-predicted HEAs. Successive optical, thermal and resource filters condense the space to 58 candidates at 355 nm and eight refractory alloys at 1064 nm, illustrating a “sustainable-by-design” route for future HEA photonics.</dc:description><dc:publisher>The Royal Society of Chemistry </dc:publisher><dc:date>2026</dc:date><dc:date>2026-09-10 09:38:00</dc:date><dc:type>Neznano</dc:type><dc:identifier>32403</dc:identifier><dc:identifier>UDK: 620.1/.2</dc:identifier><dc:identifier>ISSN pri članku: 1364-5498</dc:identifier><dc:identifier>DOI: 10.1039/D5FD00086F</dc:identifier><dc:identifier>COBISS_ID: 248791811</dc:identifier><dc:source>Združeno kraljestvo</dc:source><dc:language>sl</dc:language><dc:rights>© 2026 The Author(s).</dc:rights></metadata>
