Dark matter search with the CALET detector on-board ISS

The CALorimetric Electron Telescope, CALET, mission is proposed for the observation of high-energy electrons and gamma-rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe the electrons (without separation between e⁺ and e⁻) in 1 GeV–10 TeV and the gamma-rays in 20 MeV–several TeV with a high-energy resolution of 2% at 100 GeV, a good angular resolution of 0.06 degree at 100 GeV, and a high proton-rejection power of nearly 10⁶. The CALET has a geometrical factor of 1 m²sr, and the observation period is expected for more than three years. The very precise measurement of electrons enables us to detect a distinctive feature in the energy spectrum caused from WIMP dark matter in the Galactic halo. The excellent energy resolution of CALET, which is much better than GLAST or air Cherenkov telescopes over 10 GeV, enables us to detect gamma-ray lines in the sub-TeV region from WIMP dark matter annihilations. The CALET has, therefore, a unique capability to search for WIMP dark matter by the hybrid observations of electrons and gamma-rays.     

Dark matter and dark matter candidates

The nature and identity of the dark matter of the Universe is one of the most challenging problems facing modern cosmology. Only 5% of the energy density of the Universe can be associated with known forms of matter. Problems for baryonic and neutrino dark matter imply the necessity to search beyond the standard model for dark matter candidates. Emphasis is placed on the prospects for supersymmetric dark matter.     

AB beam propulsion for interplanetary flights

The author offers a revolutionary method—non-rocket transfer of energy and thrust into Space with a distance of millions of kilometers. The author has developed the theory and made the computations. The method is more efficient than transmission of energy by high-frequency waves. The method may be used for space launch and for accelerating the spaceship and probes for very high speeds, up to a relativistic speed by the current technology. The research also contains prospective projects which illustrate the possibilities of the suggested method.     

绿色切削中的MQL技术

重点介绍了MQL(Minimal Quantities of Lubricant)技术的研究现状、实际应用、环境及经济性能评价以及尚待进一步解决的问题。指出MQL与刀具技术、低温风冷和水雾冷却技术的结合使用将是未来难加工材料高速切削领域中的主要潮流。     

Dark Matter Searches

According to our present knowledge the matter/energy budget of the universe consists of 74% dark energy, 22% dark matter and 4% ordinary (or so-called baryonic) matter. While the dark energy cannot be detected directly, searches for dark matter are performed with earth-bound and space-borne detection devices, assuming that the dark matter consists of weakly interacting massive particles, the so-called WIMPs. An overview of the present experimental situation is given.     

Alternate models to dark energy

One of the unresolved questions currently in cosmology is that of the non-linear accelerated expansion of the universe. This has been attributed to the so called Dark Energy (DE). The accelerated expansion of the universe is deduced from measurements of Type Ia supernovae. Here we propose alternate models to account for the Type Ia supernovae measurements without invoking dark energy.     

转子叶片缘板阻尼结构设计方法

根据工程应用需求,从工程设计人员角度出发,阐明了结构设计参数、接触参数和动力学参数之间的相互影响关系。进一步建立了缘板阻尼结构的设计流程和优化方法,并给出了结构设计合理性的评估参数。某薄片式缘板阻尼结构的优化结果表明:通过优化缘板阻尼结构截面形状,可改善接触面应力的均匀程度,提高实际有效接触面积,实现在多个停留转速工况下更好的贴合状态,从而起到更好的振动抑制效果。      

具有干摩擦阻尼的叶片组振动的理论与实验研究

通过理论分析与实验研究,讨论带凸肩叶片的振动特性及其干摩擦阻尼效应。提出了适用于凸肩干摩擦的局部非线性特点的一种新的降阶方法,定义了无量纲干摩擦阻尼因子,用于度量干摩擦阻尼效果。最后,按照设计的实验方案,对带凸肩叶片组试件做了振动实验研究。     

旋转叶片干摩擦阻尼结构减振试验研究综述

研究航空发动机旋转叶片的振动特性及其振动抑制技术,对提高发动机的性能、结构完整性、工作可靠性具有重要意义。从旋转叶片干摩擦阻尼结构的减振试验装置、试验激励方法和动态特性测试等方面对旋转叶片干摩擦阻尼结构的减振试验进行了较为详细的综述,将旋转叶片干摩擦阻尼结构的减振试验分为非旋转试验和旋转试验两类,结合叶片干摩擦阻尼结构减振特性试验的研究现状,提出应在以下方面进行研究:在不旋转条件下,建立随叶片榫头结构、相邻叶片夹角变化的试验装置模型库;探索多叶片阻尼结构的高频激励耦合加载方法和振动响应测试方法;在旋转条件下,研究更符合开车环境的激励方式,发展使用应变片和传感器的高分辨率的振动响应测试方法。     

基于电磁干风洞的大柔性结构准模态试验研究

结构的频率是结构的重要动力学特性,对于飞行器来说,当机翼等大型结构在非定常气动力作用下发生变形时,其频率也会发生变化。本文介绍了一种地面电磁干风洞试验方法,利用电磁场和安培力实现气动力的模拟,在不接触模型的情况下对模型进行静动态加载。基于这种新的试验技术,建立了一种地面电磁干风洞实验方法,利用电磁场和安培力实现气动力的模拟,可有效实现对模型结构的非接触式静态和动态气动力跟随加载。利用该实验系统,研究了静动态条件下,结构质量、刚度分布对飞机内载荷的影响;结构变形对结构动力学特征的影响。结果表明,结构的弯曲变形会影响结构的弯曲和扭转频率,结构的质量和刚度分布会对结构内载荷产生较大影响。这种新的试验方法有利于研究大柔性结构的气动弹性特性,对新型飞机的设计和研制具有重要意义。