Evolving into Magnetars from Normal Pulsars with a Low Braking Index

Anomalous x-ray pulsars （AXPs） and soft gamma-ray repeaters （SCRs） are believed to be candidates for magnetars, and they are powered by the decay of ultra-strong magnetic fields of〉 1014 C. From the modified spin-down relation of pulsars P ∝P^2-n, we find that the Vela pulsar would evolve into the classes of magnetars under some assumptions that pulsars lose their rotational energy only by magnetic dipole radiation and the braking index is a constant. Our rough calculation indicates that only pulsars with n - 1.3 - 1.6 can evolve into magnetars. Pulsars like Vela with a low braking index may be the progenitors of AXPs and SCRs. Regarding the mechanism evolved into magnetars, we suggest that pulsars＇ surface magnetic field component may be increased by frequent glitches.     

高压剪切作用下三水铝石的结构稳定性

利用旋转式金刚石对顶砧压机(RDAC)结合显微激光拉曼光谱和微区X射线衍射,研究了三水铝石(γ-Al(OH)₃)在高压剪切作用下的结构稳定性。常温加压至1.5 GPa,旋转180°后,γ-Al(OH)₃的结构开始转变。初始样品在高波数段的4个羟基伸缩振动峰(3363、3434、3524和3618 cm^-1)相继消失,出现3303和3560 cm^-12个新峰。低波数段拉曼谱强度明显减弱,无非晶态宽峰;Al-O-Al变形振动双峰(568、539 cm^-1)和Al-O伸缩振动肩峰(321和307cm^-1)分别融合为一个振动峰;4个羟基变形振动峰(1052、1018、981和922 cm^-1)仍然可见。继续加压至3.5 GPa,旋转360°后卸至常压,高波数段新出现的两个羟基伸缩振动峰、原Al-O-Al变形振动峰和Al-O伸缩振动峰仍然可见。对比准静水压条件下γ-Al(OH)₃高压相的拉曼谱和相转变压力(约2.7 GPa),认为常温高压剪切作用下γ-Al(OH)₃脱羟基生成了H₂O和H₃O^-₂。卸压样品微区的X射线衍射谱进一步揭示,在高压剪切作用下,γ-Al(OH)₃的(OH)-Al-(OH)配位八面体骨架被破坏,沿c轴方向原子叠加的层间距缩小,对称性增强。这种不同于准静水压实验的结构改变来自腔体内压力的不均匀分布(0.5~4.5 GPa)。高压剪切作用下,三水铝石的结构稳定性研究对查明板块冷俯冲带中含水矿物的稳定性,推演俯冲板片的物理化学性质以及板块俯冲的速率具有重要意义。     

利用声波干涉抑制旋转式压缩机的辐射噪声

压缩机是制冷设备的主要噪声源之一,其辐射噪声的抑制很有必要.理论分析了两列声波在自由场和管道中传播特性,证实了在管道中的两列声波能够产生有效干涉从而降低声压幅值.将压缩机储液器内的双管吸气改为了单吸气,数值分析表明了改进后壳体辐射噪声得到了明显抑制.声学实验验证了数值计算结果和理论分析,单吸气压缩机总声压级降低了约1.2dB(A).     

Elastic and viscoelastic solutions to rotating functionally graded hollow and solid cylinders

Analytical solutions to rotating functionally graded hollow and solid long cylinders are developed. Young＇s modulus and material density of the cylinder are assumed to vary exponentially in the radial direction, and Poisson＇s ratio is assumed to be constant. A unified governing equation is derived from the equilibrium equations, compatibility equation, deformation theory of elasticity and the stress-strain relationship. The governing second-order differential equation is solved in terms of a hypergeometric function for the elastic deformation of rotating functionally graded cylinders. Dependence of stresses in the cylinder on the inhomogeneous parameters, geometry and boundary conditions is examined and discussed. The proposed solution is validated by comparing the results for rotating functionally graded hollow and solid cylinders with the results for rotating homogeneous isotropic cylinders. In addition, a viscoelastic solution to the rotating viscoelastic cylinder is presented, and dependence of stresses in hollow and solid cylinders on the time parameter is examined.     

A note on a quadratic rational map with two Siegel disks

Suppose f（z） is a quadratic rational map with two Siegel disks. If the rotation numbers of the Siegel disks are both of bounded type, the Hausdorff dimension of the Julia set satisfies Dim （J（f））〈2.     

旋转式离散杆战斗部的杆条旋转规律试验研究

先利用多重纸靶观察旋转式离散杆战斗部的杆条飞行姿态变化,再由"直靶法"获得杆条旋转角度与飞行距离之间的关系,结合靶网测速取得了杆条旋转角速度的定量描述。相同状态试验件的静爆试验结果表明:由"直靶法"得到的旋转角度和飞行距离之间的关系式计算出的旋转特征距离与试验结果基本一致,可为旋转特征距离设计提供参考。     

Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field

A uniform strong magnetic field is considered in calculating the properties of neutron star rotating at the Kepler frequency. The results show that the effect of the magnetic field on the properties of neutron star is evident, and the properties of the neutron stars rotating at the Kepler frequency can be used as a criterion to the equations of states of the neutron star matters.     

基于Allan方差解耦自适应滤波的旋转SINS精对准方法

对旋转式SINS精对准方法进行了研究,由于转位机构转动干扰以及惯性器件误差不确定性带来的影响,旋转式SINS状态方程和量测方程噪声方差参数难以确定,进而导致初始对准精度降低,针对这个问题引入自适应Kalman滤波技术。Sage-Husa是一种常用的自适应滤波算法,但是存在噪声参数强耦合缺陷。通过研究Allan方差与量测噪声方差之间的关系,利用Allan方差滤波器具有带通滤波的特点,独立计算量测噪声协方差阵R_k,该方法能够有效克服Sage-Husa滤波耦合问题,相比其它改进方法具有简单易实现等特点。对该研究进行了仿真实验与实际系统验证实验,结果表明:对于中等精度光纤陀螺单轴旋转SINS,自适应Kalman滤波算法航向角对准精度比标准Kalman滤波算法精度要高0.6’左右,且在误差估计过程中,自适应Kalman滤波器能够更好地抑制外界干扰误差的影响,是一种较好的精对准方法。     

单轴旋转调制捷联惯导系统倾斜角误差补偿

安装在单轴转位机构上的惯性测量单元(IMU),会因IMU坐标系与载体坐标系不重合而存在一定的倾斜角,此倾斜角会使得IMU在旋转过程中引入姿态误差,在很大程度上降低了系统的姿态输出精度。为了降低安装倾斜角对旋转式捷联惯导系统的影响,文章通过对旋转过程中因安装倾斜引起的姿态角误差进行了详细分析,然后运用实验和数据拟合的方法得出了倾斜角随转位机构变化的规律,最后对倾斜角产生的误差加以补偿。经仿真和实验验证表明,对倾斜角误差补偿后,单轴旋转式捷联惯性导航系统的水平姿态精度由原先的2°提高到0.05°范围以内,航向误差由原先的0.5°提高到0.005°,大大提高了旋转式捷联惯导系统的姿态精度,具有一定的工程应用价值。     

Behaviour of Rotating Bose-Einstein Condensates Under Shrinking

When the repulsive interaction strength between atoms decreases, the size of a rotating Bose-Einstein condensate will consequently shrink. We find that the rotational frequency will increase during the shrinking of condensate, which is a quantum mechanical analogy to ballet dancing. Compared to a non-rotating condensate, the size of a rotating BEC will eventually be saturated at a finite value when the interaction strength is gradually reduced. We also calculate the vortex dynamics induced by the atomic current, and discuss the difference of vortex dynamics in this case and that observed in a recent experiment carried out by the JILA group [Phys. Rev. Lett.90 (2003) 170405].