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BaGa4Se7与KTiOAsO4光参量振荡产生中红外激光性能对比
引用本文:孔辉,卞进田,叶庆,姚吉勇,吴昌,孙晓泉.BaGa4Se7与KTiOAsO4光参量振荡产生中红外激光性能对比[J].红外与激光工程,2020,49(6):20190423-1-20190423-7.
作者姓名:孔辉  卞进田  叶庆  姚吉勇  吴昌  孙晓泉
作者单位:1.国防科技大学 脉冲功率激光技术国家重点实验室,安徽 合肥 230037
基金项目:脉冲功率激光技术国家重点实验室主任基金(SKL2019ZR03, SKL2019ZR06);安徽省自然科学基金(1908085MF199)
摘    要:BaGa4Se7(硒镓钡,简称BGSe)与KTiOAsO4(砷酸氧钛钾,简称KTA)均可在1.06 μm激光泵浦下产生中红外激光。首先仿真计算出两种非线性晶体的相位匹配曲线,结果显示:切割角为(56.3°, 0°)的BGSe晶体在I类相位匹配条件下和切割角为(90°, 0°)的KTA在II-A类相位匹配条件下均可产生~3.5 μm的闲频光。然后理论计算出BGSe (56.3°, 0°, I类)的有效非线性系数为?11.9 pm/V,KTA(90°, 0°,II-A类)的有效非线性系数为?3.2 pm/V;在其他条件相同的情况下,15 mm长BGSe (56.3°, 0°, I类) 的OPO振荡阈值是20 mm长KTA (90°, 0°, II-A类) OPO振荡阈值的35.11%。最后通过实验验证BGSe (56.3°, 0°, I类, 15 mm) 的振荡阈值小于KTA(90°, 0°, II-A类, 20 mm),输出的中红外激光能量大于KTA。因此,BGSe是一种极具应用前景的中红外非线性晶体。

关 键 词:BaGa4Se7    KTiOAsO4    光参量振荡    中红外激光
收稿时间:2019-12-26

Comparison of mid-infrared laser generated by optical parametric oscillation of BaGa4Se7 and KTiAsO4
Institution:1.State Key Laboratory of Pulsed Power Laser Technology, National University of Defense Technology, Hefei 230037, China2.Advanced Laser Technology Laboratory of Anhui Province, Hefei 230037, China3.Technical Institute of Physics and Chemistry, Chinese Academy of Sciences, Beijing 100190, China
Abstract:Both BaGa4Se7 (BGSe) and KTiAsO4 (KTA) can generate mid-infrared lasers pumped by 1.06 μm laser. Firstly, the phase matching curves of two kinds of non-linear crystals were simulated and calculated. The results show that BGSe with cutting angles of (56.3°, 0°) and KTA with cutting angle of (90°, 0°) can generate idle frequency light of ~3.5 micron under phase matching conditions of type I and type II-A, respectively. Then through theoretical calculation, the effective non-linear coefficients of BGSe (56.3°, 0°, type-I) is ?11.9 pm/V, and that of KTA (90°, 0°, type II-A) is ?3.2 pm/V. The OPO oscillation threshold of 15 mm long BGSe (56.3°, 0°, type-I) is 35.11% of that of 20 mm long KTA (90°, 0°, type II-A). Then, the experimental results show that the oscillation threshold of BGSe-OPO (56.3°, 0°, type-I, 15 mm) is smaller than that of KTA-OPO (90°, 0°, type-II-A, 20 mm). The output energy of BGSe (56.3°, 0°, type-I) is larger than that of KTA (90°, 0°, type II-A). Therefore, BGSe is a promising mid-infrared non-linear crystal.
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