生物小分子与铜锌超氧化物歧化酶相互作用的波谱学研究及其应用

本工作以ＥＳＲ和ＮＭＲ为主要手段，并结合其它生化方法，考察了氨基酸，核酸碱基，糖等生命基本物质，和抗坏血酸等生命必需物质与铜锌超氧化物歧化酶的相互作用，实验观测到氨基酸，核酸碱基和抗坏血酸在水溶液中可以与酶中的Ｃｕ＾２＋作用而使其脱离活性部位，以小分子络合物形式游离在溶液中，同时使酶失活

InAlAs量子点材料的AFM和拉曼散射研究

对分子束外延（MBE）自组织生长的InAlAs量子点材料进行了拉曼散射实验。结合原子力显微镜（AnD对量子点形貌观察的结果，分析了InAlAs量子点生长过程中尺寸、密度和均匀性的改变，并研究了三维岛的结构对拉曼谱线的影响。对InAlAs淀积厚度不同样品的拉曼谱分析表明，岛状结构的尺寸横纵比与类GaAsLO模和类AlAs LO模的半高全宽有密切关系。不同偏振下的拉曼实验证实了该结构中的光学声子在Z（X,X）Z偏振条件下为非拉曼活性

不同淀积厚度InAs量子点的喇曼散射

利用喇曼散射方法在77K温度下对不同淀积厚度的InAs/GaAs量子点材料进行了研究.在高于InAs体材料LO模的频率范围内观察到了量子点的喇曼特征峰,分析表明应变效应是影响QD声子频率的主要因素.实验显示,随着量子点层淀积厚度L的增加,InAs量子点的声子频率由于应变释放发生红移.在加入InAlAs应变缓冲层的样品中,类AlAs声子峰随L增大发生了蓝移,从侧面证实了InAs量子点层的应变释放过程

质子滴线附近的β缓发质子衰变

简要回顾了我们小组在 1996~2004 年中发表的有关质子滴线附近β缓发质子衰变的实验结果, 即运用氦喷嘴快速带传输系统 +“p-γ”符合方法, 在稀土区质子滴线附近首次观测了 9种新核素的β缓发质子衰变, 在 A= 90 核区的 N = Z线附近获得了 5 种核素的β缓发质子衰变的新数据. 同时着重补充了一些重要的实验技术细节. 汇总了这 14 种核素的半衰期、自旋、宇称、形变以及生成反应截面的实验结果, 并与流行的核模型理论预言进行了系统的对比讨论. 从中看出:(ⅰ) Mo, Rh 以及“等待点”核 Ru 和 Pd 半衰期的实验值比近期 M?ller 等 85 92 89 93人的宏观-微观理论预言值长 5~10 倍, 因而明显地影响天体 rp-过程的核素丰度;(ⅱ) 实验指认的质子滴线核 Ho 和 Pm 的自旋和宇称, 与流行理论预言不符, 142 128但用 Woods-Saxon-Strutinsky 方法计算得到的位能面可以解释自旋和宇称的实验值; (ⅲ) 实验估计的 9 种稀土核的生成截面比通用的 Alice和 HIVAP 程序的计算值要小 1～2 个数量级

JUNO Sensitivity on Proton Decay p→νˉK+p\to \bar\nu K^+ Searches

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this paper, the potential on searching for proton decay in $p\to \bar\nu K^+$ mode with JUNO is investigated.The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits to suppress the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar\nu K^+$ is 36.9% with a background level of 0.2 events after 10 years of data taking. The estimated sensitivity based on 200 kton-years exposure is $9.6 \times 10^{33}$ years, competitive with the current best limits on the proton lifetime in this channel

Prediction of Energy Resolution in the JUNO Experiment

International audienceThis paper presents the energy resolution study in the JUNO experiment, incorporating the latest knowledge acquired during the detector construction phase. The determination of neutrino mass ordering in JUNO requires an exceptional energy resolution better than 3% at 1 MeV. To achieve this ambitious goal, significant efforts have been undertaken in the design and production of the key components of the JUNO detector. Various factors affecting the detection of inverse beta decay signals have an impact on the energy resolution, extending beyond the statistical fluctuations of the detected number of photons, such as the properties of liquid scintillator, performance of photomultiplier tubes, and the energy reconstruction algorithm. To account for these effects, a full JUNO simulation and reconstruction approach is employed. This enables the modeling of all relevant effects and the evaluation of associated inputs to accurately estimate the energy resolution. The study reveals an energy resolution of 2.95% at 1 MeV. Furthermore, the study assesses the contribution of major effects to the overall energy resolution budget. This analysis serves as a reference for interpreting future measurements of energy resolution during JUNO data taking. Moreover, it provides a guideline in comprehending the energy resolution characteristics of liquid scintillator-based detectors