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Absolute scale of second-order nonlinear-optical coefficients

机译:二阶非线性光学系数的绝对尺度

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The absolute scale of the second-order nonlinear-optical coefficients of several important nonlinear-optical materials has been obtained with improved accuracy. Second-harmonic generation, parametric fluorescence, and difference-frequency generation measurements have been made at several wavelengths in the near-infrared region. The second-harmonic generation measurement was performed at the fundamental wavelengths of 1.548, 1.533, 1.313, 1.064, and 0.852 mu m. The materials measured included congruent LiNbO3, 1%MgO:LiNbO3, 5%MgO:LiNbO3, LiTaO3, KNbO3, KTiOPO4, KH2PO4, quartz, GaAs, GaP, alpha-ZnS, CdS, ZnSe, and CdTe. We made the parametric fluorescence measurement to determine the nonlinear-optical coefficients of congruent LiNbO3 and 5%MgO:LiNbO3 at pump wavelengths of 0.532 and 0.488 mu m. We made the difference-frequency generation measurement for congruent LiNbO3 at a pump wavelength of 0.532 mu m. The second-harmonic generation, parametric fluorescence, and difference-frequency generation measurements yielded consistent data on the nonlinear-optical coefficients of the materials. We found that many of the currently accepted standard values are overestimated because of neglect of the multiple-reflection effect in (nearly) plane-parallel-plate samples. The dispersion of the nonlinear-optical coefficients showed that Miller's a is barely constant over the wavelength range measured and thus that Miller's rule is not so good as other methods for wavelength scaling of the nonlinear-optical coefficients. (C) 1997 Optical Society of America.
机译:几种重要的非线性光学材料的二阶非线性光学系数的绝对标度已经得到了提高。已经在近红外区域中的几个波长处进行了二次谐波生成,参数荧光和差频生成的测量。在1.548、1.533、1.313、1.064和0.852μm的基本波长下进行二次谐波产生测量。测得的材料包括全同的LiNbO3、1%MgO:LiNbO3、5%MgO:LiNbO3,LiTaO3,KNbO3,KTiOPO4,KH2PO4,石英,GaAs,GaP,α-ZnS,CdS,ZnSe和CdTe。我们进行了参数荧光测量,以确定在0.532和0.488μm的泵浦波长下,全LiNbO3和5%MgO:LiNbO3的非线性光学系数。我们在0.532μm的泵浦波长下对全LiNbO3进行了差频产生测量。次谐波产生,参数荧光和差频产生的测量结果得出了有关材料非线性光学系数的一致数据。我们发现,由于忽略了(几乎)平面平行板样品中的多重反射效应,许多当前接受的标准值被高估了。非线性光学系数的色散表明,在测量的波长范围内,米勒a几乎是恒定的,因此,米勒定律不如其他用于非线性光学系数的波长缩放的方法那么好。 (C)1997年美国眼镜学会。

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