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Reachable Extreme Ultraviolet Wavelengths According to Elements / Atomic Data

Identifieur interne : 001761 ( Istex/Curation ); précédent : 001760; suivant : 001762

Reachable Extreme Ultraviolet Wavelengths According to Elements / Atomic Data

Auteurs : D. Kilbane [Irlande (pays), France] ; F. De Dortan [Irlande (pays), France] ; G. O'Sullivan [Irlande (pays), France] ; V. Zakharov [Irlande (pays), France]

Source :

Short Wavelength Laboratory Sources: Principles and Practices ; 2015.

RBID : ISTEX:6A39DA789243E5761278846596FA3D69EC38090C

English descriptors

Abstract

Extreme ultraviolet and soft X-ray sources have been identified, using the FAC relativistic code, as emission arising from 4d–4f and 4p–4d transitions in palladium-like to rubidium-like ions of lanthanum through actinium. The spectra of these strong emitters are seen to separate and move to shorter wavelength as the nuclear charge increases. The emission was comparable from each source and was characterized using the unresolved transition array model. In future applications such as microscopy, spectroscopy and lithography, these radiation sources may be generated by employing the laser-produced plasma technique.

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https://api.istex.fr/document/6A39DA789243E5761278846596FA3D69EC38090C/fulltext/pdf

DOI: 10.1039/9781849735018-00042

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ISTEX:6A39DA789243E5761278846596FA3D69EC38090C

Le document en format XML

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<affiliation><mods:affiliation>b Department of Ultraintense Lasers, Division of High Power Systems/PALS Centre, Institute of Physics of the Czech Academy of Science Na Slovance 2. 182 21 Prague 8 Czech Republic</mods:affiliation>
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<term>Atomic number</term>
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<term>Phys lett</term>
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<term>Short wavelength laboratory sources</term>
<term>Shorter wavelength</term>
<term>Shorter wavelengths</term>
<term>Spectral width</term>
<term>Spontaneous emission</term>
<term>Statistical weight</term>
<term>Strong emitters</term>
<term>Terbium</term>
<term>Theoretical calculations</term>
<term>Unresolved transition array</term>
<term>Upper level</term>
<term>Water window</term>
<term>Wavelength</term>
<term>Wavelength range</term>
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<term>Atomic number</term>
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<term>Einstein coefficient</term>
<term>Emitter</term>
<term>Gadolinium</term>
<term>Kilbane</term>
<term>Klapisch</term>
<term>Lanthanide series</term>
<term>Lanthanum</term>
<term>Laser</term>
<term>Lithography</term>
<term>Nuclear charge</term>
<term>Phys</term>
<term>Phys lett</term>
<term>Radiation sources</term>
<term>Same range</term>
<term>Short wavelength laboratory sources</term>
<term>Shorter wavelength</term>
<term>Shorter wavelengths</term>
<term>Spectral width</term>
<term>Spontaneous emission</term>
<term>Statistical weight</term>
<term>Strong emitters</term>
<term>Terbium</term>
<term>Theoretical calculations</term>
<term>Unresolved transition array</term>
<term>Upper level</term>
<term>Water window</term>
<term>Wavelength</term>
<term>Wavelength range</term>
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<front><div type="abstract">Extreme ultraviolet and soft X-ray sources have been identified, using the FAC relativistic code, as emission arising from 4d–4f and 4p–4d transitions in palladium-like to rubidium-like ions of lanthanum through actinium. The spectra of these strong emitters are seen to separate and move to shorter wavelength as the nuclear charge increases. The emission was comparable from each source and was characterized using the unresolved transition array model. In future applications such as microscopy, spectroscopy and lithography, these radiation sources may be generated by employing the laser-produced plasma technique.</div>
</front>
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Reachable Extreme Ultraviolet Wavelengths According to Elements / Atomic Data

Reachable Extreme Ultraviolet Wavelengths According to Elements / Atomic Data

Source :

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Links to Exploration step

Le document en format XML

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