Optical properties of InGaAsBi/GaAs strained quantum wells studied by temperature-dependent photoluminescence

The effect of bismuth on the optical properties of InGaAsBi/GaAs quantum well structures is investigated using the temperature-dependent photoluminescence from 12 K to 450 K.The incorporation of bismuth in the InGaAsBi quantum well is confirmed and found to result in a red shift of photoluminescence wavelength of 27.3 meV at 300 K.The photoluminescence intensity is significantly enhanced by about 50 times at 12 K with respect to that of the InGaAs quantum well due to the surfactant effect of bismuth.The temperature-dependent integrated photoluminescence intensities of the two samples reveal different behaviors related to various non-radiative recombination processes.The incorporation of bismuth also induces alloy non-uniformity in the quantum well,leading to an increased photoluminescence linewidth.     

New initial condition of the new agegraphic dark energy model

The initial condition Ω_de(z_ini)=n²(1+z_ini)^-2/4 at z_ini=2000 widely used to solve the differential equation of the density of the new agegraphic dark energy (NADE) Ω_de, makes the NADE model be a single-parameter dark-energy cosmological model. However, we find that this initial condition is only applicable in a flat universe with only dark energy and pressureless matter. In fact, in order to obtain more information from current observational data, such as the cosmic microwave background (CMB) and the baryon acoustic oscillations (BAO), we need to consider the contribution of radiation. For this situation, the initial condition mentioned above becomes invalid. To overcome this shortage, we investigate the evolutions of dark energy in the matter-dominated and the radiation-dominated epochs, and obtain a new initial condition Ω_de(z_ini)=n²(1+z_ini)^-2(1+√F(z_ini)²/4 at z_ini=2000, where F(z)≡Ω_r0(1+z)/[Ω_m0+Ω_r0(1+z)] with Ω_r0 and Ω_m0 being the current density parameters of radiation and pressureless matter, respectively. This revised initial condition is applicable for the differential equation of Ω_de obtained in the standard Friedmann-Robertson-Walker (FRW) universe with dark energy, pressureless matter, radiation, and even spatial curvature, and can still keep the NADE model being a single-parameter model. With the revised initial condition and the observational data of type Ia supernova (SNIa), CMB, and BAO, we finally constrain the NADE model. The results show that the single free parameter n of the NADE model can be constrained tightly.     

级联双稳Duffing系统的随机共振研究

研究了级联双稳Duffing系统的随机共振特性, 证明级联双稳Duffing系统变尺度系数、阻尼比和级数等参数的适当调节, 不仅可实现大参数信号的级联随机共振, 而且可优化单级双稳Duffing系统的随机共振特征, 即参数调节的级联双稳Duffing系统能实现比单级双稳Duffing系统更好的随机共振输出. 此外, 级联双稳Duffing系统对方波信号具有良好的滤波整形作用, 可用于实现含噪方波信号的波形恢复. 关键词： 级联双稳Duffing系统 随机共振 变尺度 参数调节     

紫色土土壤全氮和全磷含量的高光谱遥感预测

高光谱遥感技术是土壤养分预测的有效手段之一。以三峡库区王家沟小流域为研究区,在对土壤样本的理化性质和实验室反射光谱数据分析和测量的基础上,用偏最小二乘回归方法建立了紫色土土壤全氮和全磷含量的预测模型,并用33个水稻土土壤样本对紫色土土壤养分预测模型进行了验证。结果显示,紫色土土壤全氮预测模型得到的土壤样本预测值和实测值之间的总相关系数达到了0.672,而紫色土土壤全磷预测模型得到的相关系数只有0.498; 用紫色土土壤养分预测模型对水稻土土壤养分进行预测得到的相关系数分别为0.550和0.124。因此,用高光谱来预测紫色土土壤全氮含量具有一定的可行性,但高光谱对于紫色土全磷含量的预测效果相对较差;土壤养分预测模型在不同类型土壤之间并不具有很好的通用性。     

一种光谱分析中的降维方法

在可见/近红外光谱分析中,提取光谱数据中的有用信息是建立稳健准确模型的前提。ISOMAP是一种有效的提取数据本真维的降维方法,但对噪声和邻域参数都比较敏感。提出了一种改进的ISOMAP有监督降维方法,利用光谱数据本身的相关性指导邻域图的构建,降低对噪声和邻域参数的敏感程度,以正确表达数据的邻域结构。采用该方法对两组光谱数据降维并进行PLS建模,结果表明,改进后的算法消弱了邻域大小的影响,提取出的本真维数更小,同时提高了模型精度。     

色散补偿光子晶体光纤结构参数对其色散的影响

光子晶体光纤由于其灵活可调的色散特性用作色散补偿具有极大的应用潜力. 设计了一种色散补偿光子晶体光纤, 并运用频域有限差分法模拟了其色散特性,从理论上分析了其结构参数孔间距Λ和空气占空比d/Λ对该光子晶体光纤的色散系数的影响, 并且实际制备出了3种不同结构参数的光子晶体光纤. 通过对其色散曲线对比分析表明: 当光子晶体光纤孔间距在1 μm附近时, 其色散系数随着孔间距Λ和占空比d/Λ的增大而增加, 但对于孔间距Λ的变化比占空比d/Λ更为敏感, 并且随着孔间距Λ的增加,其对色散系数的影响能力逐渐减小. 设计并制备的光子晶体光纤在1550 nm处的色散系数为-241.5 ps·nm^-1·km^-1, 相对色散斜率为0.0018, 具有较好的色散补偿能力. 关键词： 色散 色散补偿 光子晶体光纤 结构参数     

面向微穿孔板吸声结构和吸声特性混合设计的软件平台

微穿孔板吸声结构是由微穿孔板与板后空腔组成的共振吸声结构,被认为是继多孔吸声材料之后发展起来的最有吸引力的吸声结构,其吸声特性与结构参数孔径d、板厚t、孔距b及空腔深度D有关,如何按需设计一个有效的微穿孔板吸声结构已成为目前研究的热点。本文从微穿孔板吸声结构和吸声特性混合设计的角度出发,使用面向对象的编程语言C++开发了微穿孔板吸声结构设计平台。与以往设计方法不同,本文开发的软件平台综合考虑了结构参数和吸声特性参数两方面的限制,根据实际应用要求平衡微穿孔板吸声结构的最大吸声系数与吸声带宽之间的制约关系,并以饱满的吸声曲线为目标,提供满足混合设计要求的优化结构参数。     

Extended breakdown of Simpleman approximation

In this letter, we solve three-dimensional time-dependent Newton equations for atoms interacting with a ten-cycle elliptically polarized laser pulse. The ionized electron momentum distributions show a tilt angle between the distribution density peak and the main polarization axis. The tilt angle’s behavior changes with an increasing laser intensity. We show that this behavior change is directly related to the release time of the electron from the atom.     

土壤水分对近红外光谱实时检测土壤全氮的影响研究

利用近红外光谱技术实时预测土壤全氮含量是精细农业的研究热点之一,但是由于土壤水分在近红外波段的吸收系数较高,影响了土壤全氮含量的实时预测精度。使用布鲁克MATRIX_I傅里叶近红外光谱分析仪对不同土壤水分的土壤样本进行了近红外光谱扫描,定性和定量的分析了土壤水分对近红外光谱的影响,并提出了一种消除土壤水分对土壤全氮含量预测影响的方法。近红外光谱扫描结果显示在同一全氮含量水平下,随着土壤水分含量的增加,光谱吸光度呈逐渐上升的趋势,且变化趋势为非线性。通过对1 450和1 940 nm两个水分吸收波段的差分处理,设计了水分吸收指数MAI（moisture absorbance index）,再对土壤按照水分含量梯度进行分类,提出了相应的修正系数。修正后的6个土壤全氮特征波段处(940,1 050,1 100,1 200,1 300和1 550 nm)的土壤吸光度值作为建模自变量,使用BP神经网络建立了土壤全氮预测模型,模型的R_C,R_V,RMSEC,RMSEP和RPD分别达到了0.86,0.81,0.06,0.05和2.75;与原始吸光度所建模型相比较模型精度得到了显著提高。实验结果表明本方法可以有效地消除土壤水分对近红外光谱检测土壤全氮含量预测的影响,为土壤全氮含量实时预测提供了理论和技术支持。