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Autori principali: Desch, K., Ferrer-Ribas, E., Iguaz, F. J., von Oy, J., Quintana, A., Schiffer, T.
Natura: Preprint
Pubblicazione: 2026
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Accesso online:https://arxiv.org/abs/2605.12234
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author Desch, K.
Ferrer-Ribas, E.
Iguaz, F. J.
von Oy, J.
Quintana, A.
Schiffer, T.
author_facet Desch, K.
Ferrer-Ribas, E.
Iguaz, F. J.
von Oy, J.
Quintana, A.
Schiffer, T.
contents We present novel, ultra-thin, large-diameter silicon nitride windows for various soft X-ray applications. Together with the company NORCADA, we developed windows with 200 nm and 300 nm thickness withstanding pressure differences above 1 bar. The windows have an open diameter of 14 mm. They were intensively vacuum- and overpressure-tested, showing very good results. At a measurement campaign at the synchrotron radiation source SOLEIL in France, the transparency of the windows was measured over a range from 50 eV to 15 keV, giving results comparable with the expected transparencies.
format Preprint
id arxiv_https___arxiv_org_abs_2605_12234
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Characterization of large diameter ultra-thin vacuum windows for soft X-ray applications
Desch, K.
Ferrer-Ribas, E.
Iguaz, F. J.
von Oy, J.
Quintana, A.
Schiffer, T.
High Energy Physics - Experiment
Instrumentation and Detectors
We present novel, ultra-thin, large-diameter silicon nitride windows for various soft X-ray applications. Together with the company NORCADA, we developed windows with 200 nm and 300 nm thickness withstanding pressure differences above 1 bar. The windows have an open diameter of 14 mm. They were intensively vacuum- and overpressure-tested, showing very good results. At a measurement campaign at the synchrotron radiation source SOLEIL in France, the transparency of the windows was measured over a range from 50 eV to 15 keV, giving results comparable with the expected transparencies.
title Characterization of large diameter ultra-thin vacuum windows for soft X-ray applications
topic High Energy Physics - Experiment
Instrumentation and Detectors
url https://arxiv.org/abs/2605.12234