HADAR实验对活动星系核伽马射线辐射观测的预期研究

HADAR (High Altitude Detection of Astronomical Radiation)是一个基于大气切伦科夫成像技术的地面望远镜阵列,其采用大口径折射式水透镜系统来收集大气切伦科夫光,以实现对10 GeV—10 TeV能量段的伽马射线和宇宙线的探测.HADAR具有低阈能和大视场的优势,因此可以对天区进行连续扫描和观测,在观测活动星系核(Active Galactic Nuclei,AGN)等银河系外伽马射线源方面具有明显优势.本文研究了HADAR实验对AGN的探测能力.基于费米望远镜(Fermi Large Area Telescope,Fermi-LAT)的AGN源能谱信息,将观测能量外推至甚高能能段,同时加入河外背景光的吸收效应,以计算HADAR对AGN源观测的统计显著性.研究结果显示,HADAR运行一年时间,预计将有31个Fermi-LAT AGN源以高于5倍显著性被观测到,其中大部分为蝎虎状天体类型.     

Opinion Spreading with Mobility on Scale-Free Networks

A continuum opinion dynamic model is presented based on two rules. The first one considers the mobilities of the individuals, the second one supposes that the individuals update their opinions independently. The results of the model indicate that the bounded confidence εc, separating consensus and incoherent states, of a scale-free network is much smaller than the one of a lattice. If the system can reach the consensus state, the sum of all individuals＇ opinion change Oc（t） quickly decreases in an exponential form, while if it reaches the incoherent state finally, Oc（t） decreases slowly and has the punctuated equilibrium characteristic.     

纤维素/聚硅氧烷离子液体混合气相色谱固定相的制备

纤维素是液相色谱中应用十分广泛的一类固定相,可是由于涂渍性能不佳,纤维素在气相色谱中的应用鲜有报道。本论文首先通过酯化反应合成了脂溶性较好的三醋酸纤维素（CTA）,然后与自制的聚硅氧烷离子液体（PIL-C12-NTf₂）混配,制备了含纤维素的气相色谱固定相（CTA@PIL-C12-NTf₂）,并涂渍了毛细管柱。其柱效为3165 plates/m（110 ℃,萘,k=4.95）。麦氏常数及溶剂化参数模型的测试结果证明,该固定相属中强极性固定相,主要作用力是氢键碱性作用和偶极作用。值得注意的是,引入纤维素可明显改善三取代芳香化合物位置异构体及壬烷（C9）同分异构体的分离选择性。此外,该固定相对正构烷烃、醇、脂肪酸酯及邻苯二甲酸酯等也具有良好的分离选择性。该研究不仅初步展现了纤维素在分离选择性上的特点,而且也为探索纤维素衍生物在气相色谱中的应用提供了一条新的途径。     

Lateral distribution of EAS muons measured for the primary cosmic ray energy around 100 TeV

The muonic component of the extensive air showers (EAS) is of great importance for the astroparticle physics. It carries the information about the properties of primary cosmic ray (CR) particles, such as their mass, and electromagnetic and hadronic nature. It provides a sensitive test for the hadronic interaction models, which are inevitable for describing the cascade shower development of cosmic rays in EAS experiments. The YangBaJing Hybrid Array (YBJ-HA) experiment has been in operation since the end of 2016. Surface detectors are used for the measurements of primary energy, angular direction and core position of a shower event, while underground muon detectors are used for measuring the density of muons at various locations. Using the data obtained by the YBJ-HA experiment,this work reports the first measurement of the lateral muon distribution for the primary cosmic ray energy in the 100TeV region. The punch-through effect is evaluated via MC simulation.     

SARS流行病传染动力学模型

建立了 SARS流行病的数学模型 ,根据部分国家和地区的 SARS疫情数据 ,计算出其模型参数 ,给出了各地 SARS疫情与模拟结果的比较图 ,模拟结果与实际疫情十分吻合 .分析了 SARS流行特征 ,并对疫情发展进行了预测 .     

Improvement of Synchronizability of Scale-Free Networks

We investigate the factors that affect synchronizability of coupled oscillators on scale-free networks. Using the memory Tabu search （MTS） algorithm, we improve the eigen-ratio Q of a coupling matrix by edge intercrossing. The numerical results show that the synchronizatlon-improved scale-free networks should have distinctive both small average distance and larger clustering coefficient, which are consistent with some real-world networks. Moreover, the synchronizability-improved networks demonstrate the disassortative coefficient.     

利用β射线测量镀膜密度

基于β射线在穿透物质后计数和能量均有所损失,我们利用相对论效应实验谱仪根据β射线计数衰减及能量损失测量铝镀膜密度.从结果可以看出,由于实验中β射线不能保证完全单能导致能量损失法的误差非常大,有待进一步完善,结果仅供参考.由计数衰减法测得样品铝镀膜的密度为(2.6±0.2)g/cm~2.