Plasmonic generation of ultrashort extreme-ultraviolet light pulses
Ultrashort extreme-ultraviolet pulses are a key tool in time-resolved spectroscopy for the investigation of electronic motion in atoms 1 , 2 , molecules 3 and solids 4 . High-harmonic generation is a well-established process for producing ultrashort extreme-ultraviolet pulses by direct frequency upc...
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Veröffentlicht in: | Nature photonics 2011-11, Vol.5 (11), p.677-681 |
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Sprache: | eng |
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Zusammenfassung: | Ultrashort extreme-ultraviolet pulses are a key tool in time-resolved spectroscopy for the investigation of electronic motion in atoms
1
,
2
, molecules
3
and solids
4
. High-harmonic generation is a well-established process for producing ultrashort extreme-ultraviolet pulses by direct frequency upconversion of femtosecond near-infrared pulses
5
,
6
,
7
. However, elaborate pump–probe experiments performed on the attosecond timescale
8
,
9
require continuous efforts to improve the spatiotemporal coherence and also the repetition rate of the generated pulses. Here, we demonstrate a three-dimensional metallic waveguide for the plasmonic generation of ultrashort extreme-ultraviolet pulses by means of field enhancement using surface-plasmon polaritons. The intensity enhancement factor reaches a peak of ∼350, allowing generation up to the 43rd harmonic in xenon gas, with a modest incident intensity of ∼1 × 10
11
W cm
–2
. The pulse repetition rate is maintained as high as 75 MHz without external cavities. The plasmonic waveguide is fabricated on a cantilever microstructure and is therefore suitable for near-field spectroscopy with nanometre-scale lateral selectivity.
Researchers use plasmonic nanofocusing of near-infrared pulses in metallic tapered gap waveguides to generate ultrashort extreme-ultraviolet pulses. They calculate that the electromagnetic field intensity is around 350 times higher than that of a reference untapered waveguide, allowing harmonics up to the 43rd to be realized at a modest incident intensity of ∼10
11
W cm
−2
. |
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ISSN: | 1749-4885 1749-4893 |
DOI: | 10.1038/nphoton.2011.258 |