雨滴击溅与薄层水流混合侵蚀的输沙机理

【目的】针对雨滴击溅与薄层水流混合侵蚀过程输沙机理研究中存在的问题，研究雨滴击溅对坡面 径流输沙的影响。【方法】采用室内人工模拟降雨试验，以土娄土、黄绵土和黑垆土为供试土壤，在不同雨滴直径（直径 ２．２２，２．６８和３．０４ｍｍ）、不同坡度（０&deg;，２&deg;和４&deg;）和薄层水流厚度（０，２，４和６ｍｍ）条件下，分析单雨滴击溅时，泥沙溅 蚀量与水层厚度的关系；多雨滴击溅时，泥沙溅蚀量与薄层水流厚度的关系，分别对二者关系进行拟合；同时，对于多 雨滴击溅时，不同薄层水流厚度下黄绵土泥沙溅蚀量和雨滴动能的关系进行了分析。【结果】单雨滴击溅时，泥沙溅 蚀量随水层厚度的增加而减少，且雨滴直径越大其扰动水层厚度越大，当雨滴直径由２．２２ｍｍ增加到３．０４ｍｍ时， 平均扰动水层厚度由１０ｍｍ增加到１４．６７ｍｍ。多雨滴击溅时，在相同的坡度（０&deg;～４&deg;），不同土壤和雨滴直径下，随薄 层水流厚度的增加，泥沙溅蚀量呈先升后降趋势；当薄层水流厚度相同时，随雨滴直径的增加，泥沙溅蚀量呈增大趋 势。当雨滴动能不变时，泥沙溅蚀量随着薄层水流厚度的增加而增大；当薄层水流厚度一定时，泥沙溅蚀量随雨滴动 能的增加而增大。【结论】建立了单雨滴击溅和多雨滴击溅条件下扰动水层厚度关与泥沙溅蚀量的关系式。</p

用于飞行时间质谱仪的高压延时脉冲串发生器的研制

介绍了一种高压延时脉冲串发生器的原理和测试结果。该发生器使用简单的RC电路,通过延时调节、脉冲串产生和高压脉冲串产生三个步骤实现了0～±800V高压脉冲串的输出。此高压脉冲串上升沿小于100ns,可实现2μs～30ms的延时,产生的脉冲串总宽度可在1～10ms内调节,脉冲串内脉冲频率为1～10kHz可调,且产生的波形稳定,误差不超过1%,可用作垂直引入式飞行时间质谱仪里的推斥电源,用于离子的采样。同时介绍了电路各部分的调节方法、波形的输出及抖动情况,分析了误差的产生主要来自电路中电阻电容的不稳定性。提出了装置的不足之处及需要改进的地方

Amplitude analysis of the decays D0 → π+π−π+π− and D0 → π+π−π0π0*

Using e+e− annihilation data corresponding to an integrated luminosity of 2.93 fb−1 taken at the center-of-mass energy √s = 3.773 GeV with the BESIII detector, a joint amplitude analysis is performed on the decays D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η). The fit fractions of individual components are obtained, and large interferences among the dominant components of the decays D0 → a1(1260)π, D0 → π(1300)π, D0 → ρ(770)ρ(770), and D0 → 2(ππ)S are observed in both channels. With the obtained amplitude model, the CP-even fractions of D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η) are determined to be (75.2 ± 1.1stat. ± 1.5syst.) % and (68.9 ± 1.5stat. ± 2.4syst.)%, respectively. The branching fractions of D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η) are measured to be (0.688 ± 0.010stat. ± 0.010syst.)% and (0.951 ± 0.025stat. ± 0.021syst.)%, respectively. The amplitude analysis provides an important model for the binning strategy in measuring the strong phase parameters of D0 → 4π when used to determine the CKM angle γ(φ3) via the B− → DK− decay

Measurement of integrated luminosity of data collected at 3.773 GeV by BESIII from 2021 to 2024

We present a measurement of the integrated luminosity e+e- of collision data collected by the BESIII detector at the BEPCII collider at a center-of-mass energy of Ecm = 3.773 GeV. The integrated luminosities of the datasets taken from December 2021 to June 2022, from November 2022 to June 2023, and from October 2023 to February 2024 were determined to be 4.995±0.019 fb-1, 8.157±0.031 fb-1, and 4.191±0.016 fb-1, respectively, by analyzing large angle Bhabha scattering events. The uncertainties are dominated by systematic effects, and the statistical uncertainties are negligible. Our results provide essential input for future analyses and precision measurements

Determination of the number of ψ(3686) events taken at BESIII

The number of ψ(3686) events collected by the BESIII detector during the 2021 run period is determined to be (2259.3±11.1)×106 by counting inclusive ψ(3686) hadronic events. The uncertainty is systematic and the statistical uncertainty is negligible. Meanwhile, the numbers of ψ(3686) events collected during the 2009 and 2012 run periods are updated to be (107.7±0.6)×106 and (345.4±2.6)×106, respectively. Both numbers are consistent with the previous measurements within one standard deviation. The total number of ψ(3686) events in the three data samples is (2712.4±14.3)×10^

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