A self-powered and sensitive terahertz photodetection based on PdSe2

With the rapid development of terahertz technology, terahertz detectors are expected to play a key role in diverse areas such as homeland security and imaging, materials diagnostics, biology, medical sciences, and communication. Whereas self-powered, rapid response, and room temperature terahertz photodetectors are confronted with huge challenges. Here, we report a novel rapid response and self-powered terahertz photothermoelectronic (PTE) photodetector based on a low-dimensional material: palladium selenide (PdSe₂). An order of magnitude performance enhancement was observed in photodetection based on PdSe₂/graphene heterojunction that resulted from the integration of graphene and enhanced the Seebeck effect. Under 0.1-THz and 0.3-THz irradiations, the device displays a stable and repeatable photoresponse at room temperature without bias. Furthermore, rapid rise (5.0 μs) and decay (5.4 μs) times are recorded under 0.1-THz irradiation. Our results demonstrate the promising prospect of the detector based on PdSe₂ in terms of air-stable, suitable sensitivity and speed, which may have great application in terahertz detection.     

热泵型纯电动客车空调结霜特性实验研究

针对热泵型纯电动客车空调系统在冬季低温高湿环境下,车外换热器易结霜而造成系统制热性能严重衰减的问题,开发了一种带有经济器的补气型纯电动客车热泵空调系统,对车外管翅式换热器结霜特性进行了实验研究。结果表明,当车外换热器完全结霜后,系统制热量和COP均大幅下降。由于采用中压补气技术,系统仍能稳定运行,当车外温度为0、-10、-20℃时,结霜过程中系统制热量分别降低了5、3.2、2.3 kW,COP分别降低了1.1、0.7、0.45,且车外空气相对湿度越大,系统制热性能衰减越严重。     

定曲率螺旋盘管式汽车尾气余热回收装置的性能研究

为研究汽车尾气余热回收装置不同参数对其性能的影响,对汽车尾气余热回收装置定曲率螺旋盘管换热器建立三维仿真模型,研究了雷诺数在4 000～14 000的范围内,定曲率螺旋盘管换热器盘管直径和螺旋直径两个几何参数对阻力和换热性能的影响。结果表明:改变换热器盘管直径,对换热器流动阻力性能影响不大,换热量随着换热器盘管直径的增加而增加;螺旋直径为70 mm时流动阻力增量最大,换热量随着螺旋直径的减小而增大。     

薄板试样斜断口形成机制及损伤断裂过程分析

为分析不同材料和尺寸的薄板试样在室温下拉伸破坏后均形成与横截面夹角在20°~25°之间斜断口的原因,首先用统计方法对试样内随机分布微缺陷进行讨论,提出一种在宏观尺度上材料内微缺陷分布局部非均匀简化模型的假设.应用含孔材料损伤本构模型对含有不同方向微缺陷分布局部非均匀薄带区域的16MnNb薄板试样变形至破坏全过程进行数值模拟.结果表明,斜断口形成主要是由于试样内在与横截面夹角小于45°的带形区域内微缺陷分布局部非均匀造成,且与该带形区域在试样中位置无关;由于考虑微缺陷分布局部非均匀,得到试样的斜断口形成过程与试验现象完全一致;同时结合试验断口形貌,对变形过程中颈缩截面内损伤演化和破坏过程进行研究,进一步解释薄板试样的损伤破坏机制.     

复合材料层合板的低速冲击损伤及其剩余压缩强度研究

本文采用理论和实验方法研究了复合材料层合板的低速冲地及其剩余压缩强度。文中利用有限元方法和能量转换原理计算了层合板受到低速冲击的受载最危险状态，以及此时的应力分布；并用Ｔｓａｉ－Ｗｕ张量准则判断损伤情况，对产生损伤的单元进行相应的刚度折减，且作重复计算直至不产生新的损伤为止；最后，对受冲击的层合板还进行剩余压缩强度计算。在实验中，采用激光全息无损检测法测量了层合板的冲击损伤，并对受冲击的层合板进行     

4106航空润滑油拖动特性研究

采用高速球-盘式拖动力试验装置测定了4106航空润滑油在不同载荷、滚动速度、入口油温及滑滚比下的拖动系数,分析了润滑油的拖动特性,建立了拖动系数的简单计算公式.结果表明:4106航空润滑油的拖动系数随着载荷变化出现转折;在高速和高压条件下,4106航空润滑油呈现非牛顿特性;当入口油温较低时润滑油的热效应较显著;随着载荷增大,入口油温和滚动速度对拖动系数的影响减小;理论计算结果同实测值吻合良好.     

正交异性板条的渐近分析

本文阐明由三维薄弹性体的渐近分析导出各级精度板壳理论的基本方法。将多尺度分析用于板的内部区域和边界层区域导出应力,应变和位移等物理量的不同的无量纲小厚度参数ε的渐近展开式。与工程的方法不同,推导仅基于ε→0的渐近分析,对板的变形不做任何假定。给出正交异性板的平面应变渐近展开的具体列式,仅有一些常数待定。结果表明,内域解渐近级数的首项正是熟知的Kirchhoff板理论解。本文为内域解和边界层解的渐近匹配,从而正确表述圣维南原理并用以建立各级渐近解的边界条件进而求解的研究做好了准备。     

光子晶体光纤的布里渊增益谱特性

研究内全反射型光子晶体光纤(TIR-PCF)的结构参数对光纤布里渊增益、布里渊峰的个数以及相对峰值强度等布里渊增益谱(BGS)特性的影响。分析全反射型光子晶体光纤中的声光耦合效应,利用有限元分析方法,求解光纤中的光场和声场分布及其对应的BGS,探究空气孔层数、孔间距和孔直径等PCF参数对BGS的影响,获得布里渊增益和声学模式个数随孔间距和孔直径变化的规律。提出一种空气孔直径由内到外逐渐变大的、具有类似渐变折射率分布的新型光子晶体光纤结构。设计峰值强度差为8 dB的双峰BGS的光子晶体光纤,可将其用于基于布里渊拍频谱(BBS)的光纤传感系统中,使传感系统的信噪比提升2.5倍。     

A corresponding-state approach to quark-cluster matter

The state of super-dense matter is essential for us to understand the nature of pulsars; however, non- perturbative quantum chromodynamics makes it very difficult to make direct calculations of the state of cold matter at realistic baryon number densities inside compact stars. Nevertheless, from an observational point of view, it is conjectured that pulsars could be made up of quark clusters since the strong coupling between quarks might render the quarks to be grouped in clusters. In this paper, we attempt to find an equation of state of condensed quark-cluster matter in a phenomenological way. Supposing that the quark-clusters could be analogized to inert gases, we apply here the corresponding-state approach to derive the equation of state of quark-cluster matter, as was similarly demonstrated for nuclear and neutron-star matter in the 1970s. According to the calculations that we have presented, the quark-cluster stars, which are composed of quark-cluster matter, could have a high maximum mass that is consistent with observations and, in turn, further observations of pulsar mass could also place a constraint on the properties of quark-cluster matter. We will also briefly discuss the melting heat during the solid-liquid phase conversion and its related astrophysical consequences.