High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate

Space charge effects can distort the results of photoelectron spectroscopic measurements, and usually limit the allowable photon flux in an experiment. Here, the authors present an 18.4 MHz repetition rate high harmonic source in the 25–60 eV range, with a large count rate improvement over state-of-...

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Autores principales: T. Saule, S. Heinrich, J. Schötz, N. Lilienfein, M. Högner, O. deVries, M. Plötner, J. Weitenberg, D. Esser, J. Schulte, P. Russbueldt, J. Limpert, M. F. Kling, U. Kleineberg, I. Pupeza
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Lenguaje:EN
Publicado: Nature Portfolio 2019
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Acceso en línea:https://doaj.org/article/f66e140c97c34720b3c5ed73af8b5b11
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spelling oai:doaj.org-article:f66e140c97c34720b3c5ed73af8b5b112021-12-02T17:32:25ZHigh-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate10.1038/s41467-019-08367-y2041-1723https://doaj.org/article/f66e140c97c34720b3c5ed73af8b5b112019-01-01T00:00:00Zhttps://doi.org/10.1038/s41467-019-08367-yhttps://doaj.org/toc/2041-1723Space charge effects can distort the results of photoelectron spectroscopic measurements, and usually limit the allowable photon flux in an experiment. Here, the authors present an 18.4 MHz repetition rate high harmonic source in the 25–60 eV range, with a large count rate improvement over state-of-the-art attosecond setups under identical space charge conditions.T. SauleS. HeinrichJ. SchötzN. LilienfeinM. HögnerO. deVriesM. PlötnerJ. WeitenbergD. EsserJ. SchulteP. RussbueldtJ. LimpertM. F. KlingU. KleinebergI. PupezaNature PortfolioarticleScienceQENNature Communications, Vol 10, Iss 1, Pp 1-10 (2019)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
T. Saule
S. Heinrich
J. Schötz
N. Lilienfein
M. Högner
O. deVries
M. Plötner
J. Weitenberg
D. Esser
J. Schulte
P. Russbueldt
J. Limpert
M. F. Kling
U. Kleineberg
I. Pupeza
High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
description Space charge effects can distort the results of photoelectron spectroscopic measurements, and usually limit the allowable photon flux in an experiment. Here, the authors present an 18.4 MHz repetition rate high harmonic source in the 25–60 eV range, with a large count rate improvement over state-of-the-art attosecond setups under identical space charge conditions.
format article
author T. Saule
S. Heinrich
J. Schötz
N. Lilienfein
M. Högner
O. deVries
M. Plötner
J. Weitenberg
D. Esser
J. Schulte
P. Russbueldt
J. Limpert
M. F. Kling
U. Kleineberg
I. Pupeza
author_facet T. Saule
S. Heinrich
J. Schötz
N. Lilienfein
M. Högner
O. deVries
M. Plötner
J. Weitenberg
D. Esser
J. Schulte
P. Russbueldt
J. Limpert
M. F. Kling
U. Kleineberg
I. Pupeza
author_sort T. Saule
title High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
title_short High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
title_full High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
title_fullStr High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
title_full_unstemmed High-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 MHz pulse repetition rate
title_sort high-flux ultrafast extreme-ultraviolet photoemission spectroscopy at 18.4 mhz pulse repetition rate
publisher Nature Portfolio
publishDate 2019
url https://doaj.org/article/f66e140c97c34720b3c5ed73af8b5b11
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