对加速器驱动洁净核能系统散裂靶问题的探讨

简述了加速器驱动洁净核能靶系统的研究现状和存在的问题，对进一步可开展的工作提出了建议． The present status of the study on the neutron production rate, the neutron energy spectrum and the radiative nuclear production from the target spallation in accelerator driven clean nuclear system is presented. The Monto Carlo simulation and the related physics are also discussed. Their further improvement and the suggestions for the work to be done in China are proposed.     

LVDS技术在数字电视码流传输卡中的应用

在数字电视码流传输卡中，为解决数据传输中高速率与低电压之间的矛盾，将数字电视码流以LVDS信号形式输入至机顶盒，在不依赖于特定供电电压的同时，实现了高速数据传输．本文基于DS90c031芯片，实现了TTL到LVDS电平的转换，方案可行，输出码率3～30Mb／s，码流连续、无误码。     

Fermi/GBM单峰长暴的FWHM相关关系研究

本文选取26个已知红移的单峰Fermi/GBM长暴,采用KRL模型拟合光变曲线计算出半峰全宽FWHM,探讨了FWHM相关的关系。发现伽马暴的FWHM与峰值能量Ep相关性不强,未明显发现之前利用BeppoSAX、Swift暴得到的结果。这意味着FWHM与峰值能量Ep的相关关系可能受探测仪器选择效应的影响。同时利用这些Fermi/GBM伽马暴样本,通过重新对FWHM与持续时间T做相关分析,结果发现,FWHM与T90、T50都存在较强的幂律关系,其相关系数分别为R=0.85、R=0.72。这表明FWHM与T90、T50存在这密切关系,同利用BeppoSAX、Swift暴得到的结果一致。     

从宋代“客星”到中国“天眼”中的脉冲星——“李约瑟难题”试答

 研究和分析了中国古代天文学的辉煌成就与当今中国“天眼”--500 m口径球面射电望远镜（FAST）科学目标--脉冲星的关系。针对宋朝天文学家记录的客星与FAST正在进行的脉冲星观测，详述了宋代客星记录在世界科技史上的贡献；介绍了脉冲星发现历史与基本天体物理特征，以及脉冲星作为FAST科学目标的意义。以客星到脉冲星的千年追寻为线索，探索和尝试回答“李约瑟难题”，认为现代科学是人类文明共同体的长期探索结晶，中国在科学早期的发育过程中播撒了创新火种，而西方在文艺复兴运动中不断完善了科学体系，其中东西方科技的交流与传播得益于蒙古帝国在丝绸之路的远征与开拓。     

胶体金免疫层析法快速检测腹泻性贝毒软海绵酸的研究

腹泻性贝毒是一类分布较广的赤潮毒素,严重威胁到人类的健康和安全。本文用胶体金标记利用细胞融合技术制备的抗软海绵酸单克隆抗体,使用卵清蛋白合成高偶联比的包被抗原,以硝酸纤维素膜为载体,利用免疫层析技术原理,建立了快速检测软海绵酸的免疫层析试纸条方法。方法检出限12 ng/mL(0.96纳克/条)。     

对水砂充填采煤方法几个问题的初步探讨

本文主要探讨降低充填成本和在水砂交填采煤工作面推行机械化问题,试图改进水砂充填采煤方法、提高其经济效益.     

飞碟飞行的力学原理

应用力学知识对飞碟的飞行原理进行了分析和讨论，较好地解释了其飞行现象。     

Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate

So far among the nineteen pairs of detected double neutron star (DNS) systems, it is a usual fact that the first-born recycled pulsar is detected, however the youngest DNS system PSR J1906+0746, with the characteristic age of 113 kyr, is one of the three detected DNS as a non-recycled and second-born NS, which is believed to be formed by an electron capture or a low energy ultra-stripped iron core-collapse supernova (SN) explosion. The SN remnant around PSR J1906+0746 is too dim to be observed by optical telescopes, then its x-ray flux limit has been given by Chandra. A reference pulsar PSR J1509-5850 with the young characteristic age of 154 kyr was chosen as an object of comparison, which has an SN remnant observed by Chandra and is believed to be formed by iron core SN explosion. We impose a restriction on the maximum kinetic energy of electron-capture (EC) SN explosion that induces the formation of PSR J1906+0746. The estimated result is (4-8)×10⁵⁰ erg (1 erg=10^-7 J), which is consistent with that of the published simulations of the EC process, i.e., a lower value than that of the conventional iron core SN explosion of (1-2)×10⁵¹ erg. As suggested, EC process for NS formation is pertained to the subluminous type Ic SN by the helium star with ONeMg core, thus for the first time we derived the kinetic energy of EC SN explosion of DNS, which may be reconciled with the recent observation of type Ic SN 2014ft with kinetic energy of 2×10⁵⁰ erg.     

17C反应截面测量及有限力程Glauber模型分析

用透射法测量了能量为79AMeV的¹⁷C在¹²C反应靶上的反应截面;利用有限力程Glauber模型对¹⁷C的密度分布进行了分析.由高能区(965AMeV)相互作用截面数据分析认为¹⁷C具有谐振子密度分布,但拟合本实验结果及高能区实验数据发现,¹⁷C的中子密度分布中存在一个尾巴;假设¹⁷C密度为芯核加单粒子密度分布形式,分析认为¹⁷C的价中子主要处于1d5/2?轨道.     

H粒子的能量

本文在H粒子是一个六夸克集团的假定下,考虑了s夸克与u、d夸克的质量差,用夸克势模型计算了H粒子最低态的能量,结果表明它是一个能量比(?)阀能高几百MeV的共振态。