单层FeSe薄膜/氧化物界面高温超导

单层FeSe/SrTiO₃界面增强超导的发现为理解高温超导机理提供了一个新的途径,也为实现新的高温超导体开拓了新思路.本文通过在SrTiO₃（001）表面高温沉积Mg进而沉积单层FeSe薄膜,制备出了FeSe/MgO双层/SrTiO₃异质结.利用扫描隧道显微镜研究了异质结的电学及超导特性,观测到约14–15 meV的超导能隙,比体相FeSe超导能隙值增大了5–6倍,与K掺杂双层FeSe/SrTiO₃的超导能隙值相当.这一结果可理解为能带弯曲造成的界面电荷转移和界面处电声耦合共同作用导致的超导增强.FeSe/MgO界面是继FeSe/TiO₂之后的一个新界面超导体系,为研究界面高温超导机理提供了新载体.     

包含暗物质的强子夸克混合星

研究了含有暗物质的夸克核心混合星的观测属性。用相对论平均场理论和有效质量口袋模型分别描述夸克核心的混合星物质内强子相和夸克相,用Gibbs相平衡条件描述强子-夸克混合相,研究了由于包含强、弱相互作用的费米子暗物质对混合星质量、半径、引力红移、自转频率和转动惯量等整体观测属性的影响。结果表明,在强、弱相互作用下,暗物质粒子质量大于等于0.5 GeV时暗物质会使混合星的状态方程比无暗物质时有一定软化,相应的混合星最大质量减少。当调节暗物质粒子质量研究表明,随着暗物质粒子质量的增大,夸克核心的混合星物质的状态方程变软,混合星的质量、半径变小,并且引力红移、自转频率和转动惯量等整体观测属性也明显依赖于暗物质粒子的质量。当暗物质粒子质量0.1 GeV时,包含强、弱作用暗物质的混合星质量达到2.0 M_⊙和2.8 M_⊙（其中M_⊙为太阳质量）,说明大质量脉冲星PSR J1859-0131和J1931-01可能是包含小质量暗粒子暗物质的强子夸克的混合星。整体观测属性的计算结果均在中子星的天文观察数据范围内,也说明强子夸克的混合星内可能包含暗物质。The observational properties of quark core hybrid star contain dark matter are studied. The influences of containing of strongly or weakly interacting dark matter to global observational features of hybrid stars, mass, radius, gravitational red-shift, rotational period and moment of inertia are studied by using relativistic mean field theory to describe hadron phase, effective mass bag model to quark phase, and Gibbs phase equilibrium conditions to hadron-quark mixed phase respectively. Our results indicate that, both in the strong and weak interacting case, the equation of state for hybrid star matter contain dark matter become softer than that of without dark matter while the mass of dark matter particles larger than 0.5 GeV, which leads to the decrease of the mass and corresponding radius of hybrid star. With the increase of the dark matter particle mass, the equation of state for hybrid star matter become softer, this cause the decrease of the mass and radius of hybrid star obviously. The gravitational red-shift and the rotational period, obviously increase of the moment of inertia of the hybrid stars are influenced by the dark matter particle mass. When the dark matter particle mass is equal to 0.1 GeV, the masses of the star with strong and weak interacting dark matter reach to 2.0 M_⊙ and 2.8 M_⊙(M_⊙ is the solar mass), this result indicates that the giant mass PSR, J1859-0131 and J1931-01, can be a hadron-quark hybrid star and containing dark matter with small dark particle mass. The computational results of all above global observational features of hybrid stars are in the range of astronomical observation data, these also indicate that hybrid star with quark core may contains dark matter.     

微/纳米多层金刚石自支撑膜的制备及生长特性的研究

在30kW级直流电弧等离子喷射化学气相沉积装置下,采用Ar-H2-CH4混合气体,通过控制工艺参数,在钼衬底上分别制备了普通微米自支撑膜及多层金刚石自支撑膜并对其进行研究.结果显示,同普通微米膜相比,多层膜体是由微米晶金刚石层和纳米晶金刚石层组成,表面光滑,微米层与纳米层间具有相互嵌套式的界面;多层膜中各层膜体的内应力沿生长方向有明显变化,出现一个从压应力到拉应力变化的过程;在沉积过程中,随着层数变化,膜体的生长速率也发生相应的变化.     

Dynamic coloration of polymerized cholesteric liquid crystal networks by infiltrating organic compounds

We demonstrate the dynamic coloration of polymerized cholesteric liquid crystal(PCLC) networks templated by the“wash-out/refill” method in the presence of organic compounds. The reflection colors were modulated by two key approaches, that is, the injection of mutually soluble organic fluids into a microfluidic channel and the diffusion of volatile organic compounds(VOCs). The reversible tuning of reflected colors with central wavelengths between ～450 nm and ～600 nm was achieved by alternative in...     

采集时间对油料光谱分析仪测量重复性的影响

分别从积分次数、积分时间及两者不同组合3个方面考察了采集时间对油料光谱分析仪测定Ag、B、Ba等21种元素测量重复性的影响。结果表明，积分时间、积分次数及两者不同组合均会对21种元素测量重复性产生规律性影响，但对不同元素的影响并不完全相同。在积分次数固定时，随着积分时间的增加，Ca、Cr、Mg、Mn、Si、Sn在积分时间为800 ms时，其光强信号的相对标准偏差最小；Ag、Al、B、Ba、Cd、Fe、Mo、Na、P、Pb、V、Zn在积分时间为1 000 ms时，其光强信号的相对标准偏差最小；Cu、Ni、Ti光强信号的相对标准偏差随着积分时间的增加逐渐下降。在积分时间固定时，随着积分次数的增加，除Cd、Cu、Mg、Mo外，其余17种元素在积分次数为20～25时，其光强信号的相对标准偏差均达到最小水平。在采集时间固定为20 000 ms时，Al、B、Ba、Cd、Cr、Fe、Mg、Mn、Ni、P、Pb、Si、Sn 13种元素在积分时间为800 ms、积分次数为25次的条件下，其光强信号的相对标准偏差最小，除Cd元素外，其余12种元素光强信号的相对标准偏差均小于3.5%(n=10)。该研究结果...     

基于支持向量机的低分辨核磁共振氢谱法快速预测喷气燃料密度

密度是喷气燃料生产、储运、加注过程中重要的质量指标。为了实现喷气燃料密度的快速、准确测定，提出了一种基于支持向量机（SVM）的低分辨核磁共振氢谱法预测喷气燃料密度。采集喷气燃料样品密度数据和低分辨核磁共振氢谱，利用网格寻优算法和训练集内部五折交叉验证方法优化建模参数。以均方误差和相关系数为指标，通过正交试验对影响模型性能的数据预处理方法进行优化，并对谱图特征的提取方式进行考察。在优化条件下建立的定量分析模型比偏最小二乘法模型预测准确度更高。所建模型对6个油样的预测值与标准值的相对偏差均低于0.3%，模型可应用于喷气燃料密度的快速分析。     

Optical Neural Network Architecture for Deep Learning with Temporal Synthetic Dimension

The physical concept of synthetic dimensions has recently been introduced into optics. The fundamental physics and applications are not yet fully understood, and this report explores an approach to optical neural networks using synthetic dimension in time domain, by theoretically proposing to utilize a single resonator network, where the arrival times of optical pulses are interconnected to construct a temporal synthetic dimension.The set of pulses in each roundtrip therefore provides the sites ...