Power optimization of XUV frequency combs for spectroscopy applications [Invited]

D. C. Yost; A. Cingöz; K. Allison T. K. Allison; A. Ruehl; M. E. Fermann; I. Hartl; J. Ye

doi:10.1364/OE.19.023483

Power optimization of XUV frequency combs for spectroscopy applications [Invited]

D. C. Yost
, A. Cingöz
, K. Allison T. K. Allison
, A. Ruehl
, M. E. Fermann
, I. Hartl
, J. Ye

Chemistry

Stony Brook University

Research output: Contribution to journal › Article › peer-review

47 Scopus citations

Abstract

We address technical impediments to the generation of highphoton flux XUV frequency combs through cavity-enhanced high harmonic generation. These difficulties arise from mirror damage, cavity nonlinearity, the intracavity plasma generated during the HHG process, and imperfect phase-matching. By eliminating or minimizing each of these effects we have developed a system capable of generating > 200 μW and delivering ̃20 μW of average power for each spectrally separated harmonic (wavelengths ranging from 50 nm - 120 nm), to actual comb-based spectroscopy experiments.

Original language	English
Pages (from-to)	23483-23493
Number of pages	11
Journal	Optics Express
Volume	19
Issue number	23
DOIs	https://doi.org/10.1364/OE.19.023483
State	Published - Nov 7 2011

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AU - Yost, D. C.

AU - Cingöz, A.

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AU - Ruehl, A.

AU - Fermann, M. E.

AU - Hartl, I.

AU - Ye, J.

PY - 2011/11/7

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N2 - We address technical impediments to the generation of highphoton flux XUV frequency combs through cavity-enhanced high harmonic generation. These difficulties arise from mirror damage, cavity nonlinearity, the intracavity plasma generated during the HHG process, and imperfect phase-matching. By eliminating or minimizing each of these effects we have developed a system capable of generating > 200 μW and delivering ̃20 μW of average power for each spectrally separated harmonic (wavelengths ranging from 50 nm - 120 nm), to actual comb-based spectroscopy experiments.

AB - We address technical impediments to the generation of highphoton flux XUV frequency combs through cavity-enhanced high harmonic generation. These difficulties arise from mirror damage, cavity nonlinearity, the intracavity plasma generated during the HHG process, and imperfect phase-matching. By eliminating or minimizing each of these effects we have developed a system capable of generating > 200 μW and delivering ̃20 μW of average power for each spectrally separated harmonic (wavelengths ranging from 50 nm - 120 nm), to actual comb-based spectroscopy experiments.

UR - https://www.scopus.com/pages/publications/80755169425

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ER -

Power optimization of XUV frequency combs for spectroscopy applications [Invited]

Abstract

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