High-peak-power narrow-pulsed linearly polarized laser at ∼ 3 μm

被引:0
|
作者
Feng, Xiaoyue [1 ,2 ]
Xue, Yanyan [3 ]
Liu, Jingjing [1 ,2 ]
Tong, Luyang [1 ,2 ,4 ]
Hao, Qianqian [1 ,2 ,5 ]
Xu, Xiaodong [6 ]
Liu, Jie [1 ,2 ]
Xu, Jun [3 ]
机构
[1] Shandong Normal Univ, Shandong Prov Engn & Tech Ctr Light Manipulat, Sch Phys & Elect, Jinan 250358, Peoples R China
[2] Shandong Normal Univ, Sch Phys & Elect, Shandong Prov Key Lab Opt & Photon Device, Jinan 250358, Peoples R China
[3] Tongji Univ, Inst Adv Study, Sch Phys Sci & Engn, Shanghai 200092, Peoples R China
[4] Henan Acad Sci, Inst Phys, Zhengzhou 450046, Peoples R China
[5] Chinese Acad Sci, Xinjiang Tech Inst Phys & Chem, Res Ctr Crystal Mat, Urumqi 830011, Peoples R China
[6] Jiangsu Normal Univ, Sch Phys & Elect Engn, Jiangsu Key Lab Adv Laser Mat & Devices, Xuzhou 221116, Peoples R China
来源
OPTICS EXPRESS | 2024年 / 32卷 / 23期
基金
中国国家自然科学基金;
关键词
Q-SWITCHED HO; SPECTROSCOPIC PROPERTIES; SATURABLE ABSORBER; CRYSTAL;
D O I
10.1364/OE.542304
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
A hundred-watt-level peak-power linearly polarized Ho,Pr:GdScO3 laser with narrow pulses was first realized at similar to 3 mu m through a combination of theoretical simulation and experiment. This is the narrowest pulse width, and the highest peak power has been achieved in a passively pulsed Ho,Pr co-doped laser to date. We realized a linearly polarized narrow-pulsed laser at similar to 3 mu m, with a maximum peak power of 185 W and shortest pulse width of 42 ns. A further theoretical model was built by simulating the dynamic process of the mid-infrared (MIR) pulsed Ho,Pr:GdScO3 laser using coupled rate equations. The numerical simulation results were fundamentally in agreement with the experimental results, which verified the potential of Ho,Pr:GdScO3 crystals to produce sub-50-ns hundred-watt peak power MIR lasers. The results presented an effective way to achieve high-peak-power, narrow-pulse, and linearly-polarized lasers, which have significant research potential and promising applications in the MIR band. (c) 2024 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement
引用
收藏
页码:42165 / 42172
页数:8
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