| Home > Publications database > 7 $\mu$m, ultrafast, sub-millijoule-level mid-infrared optical parametric chirped pulse amplifier pumped at 2 $\mu$m > print |
| 001 | 316850 | ||
| 005 | 20250730111651.0 | ||
| 024 | 7 | _ | |a 10.1364/OPTICA.3.000147 |2 doi |
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| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Sanchez, D. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a 7 $\mu$m, ultrafast, sub-millijoule-level mid-infrared optical parametric chirped pulse amplifier pumped at 2 $\mu$m |
| 260 | _ | _ | |a Washington, DC |c 2016 |b OSA |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 520 | _ | _ | |a We present a novel all-fiber pumped optical parametric chirped pulse amplifier (OPCPA) architecture to generate self-carrier-to-envelope-phase stable, sub-eight-optical-cycle duration pulses at 7 μm wavelength approaching millijoulelevel pulse energy at 100 Hz repetition rate. The system yields a peak power of 1.1 GW and, if focused to the diffraction limit, would reach a peak intensity of 7 × 10$^{14}$ W∕cm$^2$. The OPCPA is pumped by a 2 μm Ho:YLF chirped pulse amplifier to leverage the highly efficient and broadband response of the nonlinear crystal ZGP. The 7 μm seed at 100 MHz is generated via difference frequency generation from an Er:Tm:Ho multi-arm fiber frequency comb, and a fraction of its output optically injects the Ho:YLF amplifier. Whilethe pulse bandwidth at 7 μm is perfectly suited for nonlinear and spectroscopic applications, current parameters offer, for the first time, to the best of our knowledge, the possibility to explore strong-field physics in an entirely new wavelength range with a ponderomotive force 77 times larger than from an 800 nm source. The overall OPCPA system is very compact and provides a new tool for investigations directly in the molecular fingerprint region of the electro-magnetic spectrum or to drive high harmonic generation to produce fully coherent x-rays in the multi-kiloelectron-volt range and possibly zeptosecond temporal waveforms. |
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| 700 | 1 | _ | |a Hemmer, M. |0 P:(DE-H253)PIP1023642 |b 1 |
| 700 | 1 | _ | |a Baudisch, M. |0 P:(DE-HGF)0 |b 2 |
| 700 | 1 | _ | |a Cousin, S. L. |0 P:(DE-HGF)0 |b 3 |
| 700 | 1 | _ | |a Zawilski, K. |0 P:(DE-HGF)0 |b 4 |
| 700 | 1 | _ | |a Schunemann, P. |0 P:(DE-HGF)0 |b 5 |
| 700 | 1 | _ | |a Chalus, O. |0 P:(DE-H253)PIP1020027 |b 6 |
| 700 | 1 | _ | |a Simon-Boisson, C. |0 P:(DE-HGF)0 |b 7 |
| 700 | 1 | _ | |a Biegert, J. |0 P:(DE-HGF)0 |b 8 |
| 773 | _ | _ | |a 10.1364/OPTICA.3.000147 |g Vol. 3, no. 2, p. 147 - |0 PERI:(DE-600)2779175-0 |n 2 |p 147 - 150 |t Optica |v 3 |y 2016 |x 2334-2536 |
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