High photon flux table-top coherent extreme-ultraviolet source
High photon flux with up to 10 12 photons in the 25–40 eV range has been achieved in a new table-top coherent extreme ultraviolet (EUV) source based on phase-matched high-harmonic generation using a fibre laser. Intense and compact EUV sources are needed for certain types of spectroscopic and imagin...
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Published in | Nature photonics Vol. 8; no. 10; pp. 779 - 783 |
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Main Authors | , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
London
Nature Publishing Group UK
01.10.2014
Nature Publishing Group |
Subjects | |
Online Access | Get full text |
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Summary: | High photon flux with up to 10
12
photons in the 25–40 eV range has been achieved in a new table-top coherent extreme ultraviolet (EUV) source based on phase-matched high-harmonic generation using a fibre laser. Intense and compact EUV sources are needed for certain types of spectroscopic and imaging applications.
High harmonic generation (HHG) enables extreme-ultraviolet radiation with table-top set-ups
1
. Its exceptional properties, such as coherence and (sub)-femtosecond pulse durations, have led to a diversity of applications
1
. Some of these require a high photon flux and megahertz repetition rates, for example, to avoid space charge effects in photoelectron spectroscopy
2
,
3
,
4
. To date, this has only been achieved with enhancement cavities
5
. Here, we establish a novel route towards powerful HHG sources. By achieving phase-matched HHG of a megahertz fibre laser we generate a broad plateau (25 eV–40 eV) of strong harmonics, each containing more than 1 × 10
12
photons s
–1
, which constitutes an increase by more than one order of magnitude in that wavelength range
6
,
7
,
8
. The strongest harmonic (H25, 30 eV) has an average power of 143 μW (3 × 10
13
photons s
–1
). This concept will greatly advance and facilitate applications in photoelectron or coincidence spectroscopy
9
, coherent diffractive imaging
10
or (multidimensional) surface science
2
. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 1749-4885 1749-4893 |
DOI: | 10.1038/nphoton.2014.214 |