Overview: The space gravitational wave detection telescope is one of the core payloads of the gravitational wave detection satellite, simultaneously expanding and contracting the transmitted beam. Optical path stability is one of the core indices for the telescope, closely related to its structural stability. To meet the ultra-high path stability and structural stability requirements posed by the gravitational wave detection mission, it is essential to study the structural deformation measurement of the telescope. Currently, there are still several shortcomings in the research of multi-degree-of-freedom deformation measurement methods for gravitational wave detection telescopes, such as inaccurate selection of measurement points, inability to decouple multi-degree-of-freedom coupling, and unclear identification of error sources in multi-degree-of-freedom measurement. This paper deeply investigates the high-precision measurement of structural deformation of space-borne telescopes designed for space gravitational wave detection. It preliminarily establishes a framework and method system for measuring the structural deformation of space-borne telescopes, theoretically describing the measurement principle of the method. The feasibility of this method applied to space gravitational wave detection is verified through simulation analysis and error decomposition. The paper focuses on resolving the issue of decoupling multiple degrees of freedom, establishing a mathematical model using analytical methods, and conducting preliminary validation using Zemax. Finally, noise analysis of the measurement system is carried out, with experimental testing of the main noise components in the measurement system, validating the correctness of the theoretical noise model proposed in this paper. The experimental results show that near 1 Hz, the displacement noise background of the single-link interferometer is 100 pm/Hz^1/2. At 1 mHz in the low-frequency range, the displacement noise background reaches 10 nm/Hz^1/2. The noise level of the measurement system below 1 mHz is mainly limited by environmental temperature noise, while above 10 mHz, it is primarily constrained by laser frequency noise, phase acquisition background noise, and vibration noise. During the development phase of the space gravitational wave detection telescope, the research on this measurement method is expected to fulfill the telescope's multi-degree-of-freedom deformation measurement needs. It also provides data feedback for telescope design and offers guidance for the study of the telescope's optical path stability.

基于化学气相沉积（CVD）法制备的铯铅溴钙钛矿薄膜具有优异的光电特性，然而薄膜通常存在CsPbBr₃和CsPb₂Br₅两个不同的相结构区域。本文通过CVD法制备了铯铅溴钙钛矿薄膜，并利用X射线衍射（XRD）、扫描电镜（SEM）、电子能谱仪（EDS）及荧光光谱仪研究了反应气压与N₂流量对其中的CsPb₂Br₅相结构的影响。实验结果表明，反应气压的变化对CsPb₂Br₅相结构无影响；与此不同，随着N₂流量的减少，薄膜中部分CsPb₂Br₅相结构逐渐转变为CsPbBr₃相结构，其发光也由以~630 nm为主的宽带发射转变为以~530 nm为主的窄带发射。实验表明，N₂流量是调控CsPb₂Br₅相结构和发光特性的有效手段。

The prevalent fashion of executing Rydberg-mediated two- and multi-qubit quantum gates in neutral atomic systems is to pump Rydberg excitations using multistep piecewise pulses in the Rydberg blockade regime. Here, we propose to synthesize a Λ-type Rydberg antiblockade (RAB) of two neutral atoms using periodic fields, which facilitates one-step implementations of SWAP and controlled-SWAP (CSWAP) gates with the same gate time. Besides, the RAB condition is modified so as to circumvent the sensitivity of RAB-based gates to infidelity factors, including atomic decay, motional dephasing, and interatomic distance deviation. Our work makes up the absence of one-step schemes of Rydberg-mediated SWAP and CSWAP gates and may pave a way to enhance the robustness of RAB-based gates.

为了减少电缆沟盲目施工与偷盗等因素造成的损失和影响，引入一种智能的线路监控技术。该技术基于分布式光纤传感技术，利用BP神经网络对光纤传感器的四种常见的扰动信号进行模式识别。通过将光纤传感器得到的时域扰动信号用特定的程序处理后转换成图像，再经特定的图像处理流程后形成模式识别的样本。利用这些样本训练BP神经网络，并将训练好的模型应用到实际的电缆沟安全监控系统中进行测试。测试结果表明，电缆沟的总体识别成功率为98.16%，该识别方法还可以应用于光纤周界安防系统等领域。

Red-green-blue (RGB) full-color micro light-emitting diodes (μ-LEDs) fabricated from semipolar (20-21) wafers, with a quantum-dot photoresist color-conversion layer, were demonstrated. The semipolar (20-21) InGaN/GaN μ-LEDs were fabricated on large (4 in.) patterned sapphire substrates by orientation-controlled epitaxy. The semipolar μ-LEDs showed a 3.2 nm peak wavelength shift and a 14.7% efficiency droop under 200A/cm2 injected current density, indicating significant amelioration of the quantum-confined Stark effect. Because of the semipolar μ-LEDs’ emission-wavelength stability, the RGB pixel showed little color shift with current density and achieved a wide color gamut (114.4% NTSC space and 85.4% Rec. 2020).