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Numerical study of spatial chirp distortion in quasi-parametric chirped-pulse amplification

Published online by Cambridge University Press:  13 May 2022

Yirui Wang
Affiliation:
School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
Jing Wang*
Affiliation:
School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
Jingui Ma
Affiliation:
School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
Peng Yuan
Affiliation:
School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
Liejia Qian
Affiliation:
School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai 200240, China
*
Correspondence to: J. Wang, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China. Email: wangj1118@sjtu.edu.cn

Abstract

Optical parametric chirped-pulse amplification is inevitably subject to high-order spatial chirp, particularly under the condition of saturated amplification and a Gaussian pump; this corresponds to an irreversible spatiotemporal distortion and consequently degrades the maximum attainable focused intensity. In this paper, we reveal that such spatial chirp distortion can be significantly mitigated in quasi-parametric chirped-pulse amplification (QPCPA) with idler absorption. Simulation results show that the quality of focused intensity in saturated QPCPA is nearly ideal, with a spatiotemporal Strehl ratio higher than 0.98. As the seed bandwidth increases, the idler absorption spectrum may not be uniform, but the Strehl ratio in QPCPA can be still high enough due to stronger idler absorption.

Information

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2022. Published by Cambridge University Press in association with Chinese Laser Press
Figure 0

Figure 1 Comparison of the spatial chirp distortion of the amplified signal calculated for (a), (c) saturated OPCPA based on a 5-mm-thick YCOB crystal and (b), (d) saturated QPCPA based on a 15-mm-thick Sm3+:YCOB crystal. (a), (b) Intensity profiles in the spatial and spectral domain. (c), (d) Signal spectra at the beam center (x = 0) and beam edge (x = W0).

Figure 1

Figure 2 Comparison of the SR and spatiotemporal performance of OPCPA and QPCPA outputs. (a), (b) The evolutions of SR and signal efficiency with the crystal length. (c), (d) The compressed signal distribution in space and time. (e), (f) Three compressed signal pulses sampled at x = 0, 0.6W0 and W0, for OPCPA and QPCPA, respectively. Insets in (a) and (b) depict the spatiotemporal profiles of the focused signal, which were calculated with the crystal lengths of 5 and 15 mm, respectively. Simulation parameters were the same as those listed in Figure 1.

Figure 2

Figure 3 The dependence of SR performance on the idler absorption coefficient, seed bandwidth and pump intensity. (a) Calculated SR versus idler absorption coefficient for three seed bandwidths of 50, 100 and 200 nm under a fixed pump intensity of 80 GW/cm2. (b) Calculated SR versus pump intensity for three idler absorption coefficients of 0.3, 1, and 2 cm–1 under a fixed seed bandwidth of 100 nm.

Figure 3

Figure 4 Characterization of the spatiotemporal performance of QPCPA based on a real Sm3+:YCOB crystal. (a) The absorption spectrum of a real Sm3+:YCOB crystal, where the gray area of the spectrum is adopted in the simulation of QPCPA. (b) The evolutions of SR and signal efficiency with the crystal length under the condition of nonuniform idler absorption. The inset shows the spatiotemporal distribution of the compressed signal, which was calculated with the crystal length of 15 mm.