Journal
OPTICS LETTERS
Volume 34, Issue 11, Pages 1639-1641Publisher
OPTICAL SOC AMER
DOI: 10.1364/OL.34.001639
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Funding
- U.S. Air Force Office of Scientific Research (AFOSR) [FA9550-06-1-0468, FA9550-07-1-0014]
- Australian Research Council Centre of Excellence program
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We present a 9 GW peak power, three-cycle, 2.2 mu m 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. (C) 2009 Optical Society of America
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