Abstract

We present a 9 GW peak power, three-cycle, 2.2 μm optical parametric chirped-pulse amplification source with 1.5% rms energy and 150 mrad carrier envelope phase fluctuations. These characteristics, in addition to excellent beam, wavefront, and pulse quality, make the source suitable for long-wavelength-driven high-harmonic generation. High stability is achieved by careful optimization of superfluorescence suppression, enabling energy scaling.

© 2009 Optical Society of America

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History
Original Manuscript: February 2, 2009
Manuscript Accepted: April 14, 2009
Revised Manuscript: April 1, 2009
Published: May 21, 2009

References

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Author Affiliations

J. Moses, S.-W. Huang, K.-H. Hong, O. D. Mücke, E. L. Falcão-Filho, A. Benedick, F. Ö. Ilday, F. X. Kärtner

Massachusetts Institute of Technology

A. Dergachev

Q-Peak

J. A. Bolger, B. J. Eggleton

University of Sydney

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