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<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>A high-efficiency programmable modulator for extreme ultraviolet light with nanometre feature size based on an electronic phase transition</dc:title><dc:creator>Vaskivskyi,	Igor	(Avtor)
	</dc:creator><dc:creator>Mraz,	Anže	(Avtor)
	</dc:creator><dc:creator>Venturini,	Rok	(Avtor)
	</dc:creator><dc:creator>Jecl,	Gregor	(Avtor)
	</dc:creator><dc:creator>Vaskivskyi,	Yevhenii	(Avtor)
	</dc:creator><dc:subject>light modulators</dc:subject><dc:subject>extreme ultraviolet light</dc:subject><dc:subject>ultrafast photonics</dc:subject><dc:subject>condensed-matter physics</dc:subject><dc:description>The absence of efficient light modulators for extreme ultraviolet (EUV) and X-ray photons considerably limits their real-life application, particularly when even slight complexity of the beam patterns is required. Here we report on a novel approach to reversible imprinting of a holographic mask in an electronic Wigner crystal material with a sub-90-nm feature size. The structure is imprinted on a sub-picosecond timescale using EUV laser pulses, and acts as a high-efficiency diffraction grating that deflects EUV or soft X-ray light. The imprinted nanostructure is stable after the removal of the exciting beams at low temperatures, but can be easily erased by a single heating beam. Modelling shows that the efficiency of the device can exceed 1%, approaching state-of-the-art etched gratings, but with the benefit of being programmable and tunable over a large range of wavelengths. The observed effect is based on the rapid change of lattice constant upon transition between metastable electronically ordered phases in a layered transition metal dichalcogenide. The proposed approach is potentially useful for creating tunable light modulators in the EUV and soft X-ray spectral ranges.</dc:description><dc:date>2024</dc:date><dc:date>2024-11-12 13:44:27</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>164796</dc:identifier><dc:identifier>UDK: 53</dc:identifier><dc:identifier>ISSN pri članku: 1749-4893</dc:identifier><dc:identifier>DOI: 10.1038/s41566-024-01389-z</dc:identifier><dc:identifier>COBISS_ID: 186100483</dc:identifier><dc:language>sl</dc:language></metadata>
