Testing the variation of the fine structure constant with strongly lensed gravitational waves

The possible variation of the electromagnetic fine structure constant, αe, at cosmological scales has aroused great interest in recent years. Strongly lensed gravitational waves(GWs) and their electromagnetic counterparts could be used to test this variation. Under the assumption that the speed of a photon can be modified,whereas the speed of a GW is the same as predicted by general relativity, and they both propagate in a flat FriedmanRobertson-Walker universe, we investigated the difference in time delays of the images and derived the upper bound of the variation of αe. For a typical lensing system in the standard cosmological models, we obtained B cosθ 1.85×10~(-5),where B is the dipolar amplitude and θ is the angle between observation and the preferred direction. Our result is consistent with the most up-to-date observations on αe. In addition, the observations of strongly lensed GWs and their electromagnetic counterparts could be used to test which types of alternative theories of gravity can account for the variation of α_e.     

BESⅢ端盖TOF时间分辨的束流测试

使用800MeV的电子束对BESⅢ端盖飞行时间探测器(TOF)模块的性能进行测试. 研究了塑料闪烁体的包装材料、光电倍增管(PMT)的工作电压、电子束入射位置对单个TOF模块的本征时间分辨的影响，并给出了测量时间与信号幅度和粒子击中位置的修正方法. 实验结果显示:使用Tyvek纸包装，闪烁体在安装PMT的一端有45°斜面, 电子击中在TOF模块不同位置其本征时间分辨在70—90ps范围内.     

聚氰基丙烯酸酯纳米颗粒的红外光谱及相关分析

在添加了稳定剂(Dextran)的基础上,采用乳液聚合的方法制备直径200nm左右的聚氰基丙烯酸酯纳米颗粒,利用TEM、IR研究了稳定剂Dextran与聚合物纳米颗粒的结合状态以及稳定剂稳定聚氰基丙烯酸酯的机理。结果表明,每个Dextran分子通过有效的羟基与氰基丙烯酸酯共价连接,导致Dextran与颗粒之间发生不可逆的粘附。     

暗物质寻找实验中CsI(Tl)晶体反符合探测器实验研究

一个正在建设的位于韩国Y2L地下实验室的低能暗物质探测实验中, 采用了CsI(Tl)晶体反符合探测器作为主动屏蔽体. 本工作对CsI(Tl)晶体反符合探测器的实验性能进行了研究. 通过FADC系统记录的脉冲波形数据, 研究了探测器的能量分辨率和波形甄别的能力; 研究相同能量γ射线入射到反符合探测器不同位置的相对光输出将有助于选择探测器的工作参数; 为了解晶体自身放射性对暗物质测量的影响, 利用低本底HPGe探测器对CsI(Tl)晶体内部的放射性进行了测量, 得到晶体内部Cs同位素的放射性活度. 探测器系统进行了约18d的试运行取数. 实验数据表明, CsI(Tl)晶体探测器的反符合效率约为31% HPGe探测器的本底计数率水平约为133cpd. 为了进行暗物质探测研究, 需要采取有效的方法进一步降低探测器的本底水平.     

Gravitational Deflection of Light in Rindler-Type Potential as a Possible Resolution to the Observations of Bullet Cluster 1E0657-558

The surface density Σ-map and the convergence κ-map of Bullet Cluster 1E0657-558 show that the center of baryonic matters separates from the center of gravitational force,and the distribution of gravitational force do not possess spherical symmetry.This hints that a modified gravity with difference to Newtonian inverse-square law at large scale,and less symmetry is worth investigating.In this paper,we study the dynamics in Randers-Finsler spacetime.The Newtonian limit and gravitational deflection of light in a Rindler-type potential is focused in particular.It is shown that the convergence in Finsler spacetime could account for the observations of Bullet Cluster.     

基于超声波多普勒法的流通截面分区流速测量的研究

传统的超声波多普勒流量计测量的结果是大面积区域内具有统计意义的平均流速,不能反映流速在流通截面上的分布,当雷诺数变化很大时,测量误差很大。基于超声波多普勒效应,本文首次提出了通过对测量信息窗区域的控制,来实现在管流内部进行流速分区测量,进而测量出流速在流通截面上的分布。研制出发射传感器和接收传感器,分别能够产生细长的发射声束和接收声束,使得信息窗区域面积得以控制在很小的范围内,约 2.1× 4.8 mm2,位置也被控制在设计值处,满足分区测量要求;在自行设计的模拟管道流动装置中,成功地进行了控制信息窗区域面积和位置的实验,测量值与设计值吻合很好。实现了管道流通截面上的流速分区测量。     

BESⅢ端盖TOF探测器的研制

针对BESⅢ端盖TOF的研制方案, 设计和制作了特殊构型的闪烁探测器. 研究了光电倍增管(R5924)和塑料闪烁体(BC404, BC408, EJ204)的性能. 测量了几种包装材料对单个闪烁探测器模块光收集和本征时间分辨的影响. 使用800MeV实验电子束对探测器模块的测量结果显示, 采用EJ204和BC404晶体其时间分辨小于80ps; 采用ESR材料包装可获得较大的输出信号, 提高了探测器的性能.     

Nonadiabatic Geometric Phase in Composite Systems and Its Subsystem

We point out that the time-dependent gauge transformation technique may be effective in investigating the nonadiabatic geometric phase of a subsystem in a composite system. As an example, we consider two uniaxially coupled spin -1/2 particles with one of particles driven by rotating magnetic field. The influences of coupling and precession frequency of the magnetic field on geometric phase are also discussed in detail.     

非对易相空间中的狄拉克振子的能级和Wigner函数

非对易几何、弦论和圈量子引力理论的发展,使非对易空间受到越来越多的关注.非对易量子理论不同于平常的量子理论,它是弦尺度下的特殊的物理效应,处理非对易量子力学问题需要特殊方法.本文首先介绍了Moyal方程与Wigner函数,利用Moyal-Weyl乘法与Bopp变换将H(x,p)变换成^H(^x,^p),考虑坐标—坐标、动量—动量的非对易性,实现对非对易相空间中星乘本征方程的求解.并利用非对易相空间量子力学的代数关系,讨论了非对易相空间中狄拉克振子的Wigner函数和能级,研究结果发现非对易相空间中狄拉克振子的能级明显依赖于非对易参数.     

Holographic Dark Energy Model is Consistent with Pantheon SN Ia Data

We constrain three cosmological models,i.e.,ACDM model, holographic dark energy(HDE) model and R_h = ct model by using the recent Pantheon compilation of type la supernovae(SN la), the direction measurements of Hubble parameter H(z), and the baryon acoustic oscillations(BAO). The spatial curvature is considered in the ACDM model and the HDE model. We show that the HDE model in a spatially flat and HDE dominate universe has the same behavior as Rh = ct model if the characteristic parameter of the HDE model C_0 approaches to infinity. Numerical results show that the ACDM model is the best favoured one among the three models. The HDE model is consistent with observational data, the best fitting value of C_0 is around 0.8, which implies that the Rh = ct model should be modified to be compatible with the present cosmological observational data. Combing all the datasets, we give strict constraint on the Hubble constant,where h_0=0.694 ± 0.020 for the ACDM model and h_0= 0.689 ±0.019 for the HDE model.Our results imply that the tension of Hubble constant between Planck collaborations and Riess et al. has been partially relaxed. The constraint on the spatial curvature is also given,where Ω_(k0) =-0.066 ± 0.165 for the ACDM model andΩ_(k0)=0.029 ± 0.067 for the HDE model.