Nonlinear electromagnetic perturbations in a degenerate electron–positron plasma

Nonlinear propagation of fast and slow magnetosonic perturbation modes in an ultra-cold, degenerate (extremely dense) electron–positron (EP) plasma (containing non-relativistic, ultra-cold, degenerate electron and positron fluids) has been investigated by the reductive perturbation method. It is shown that due to the property of being equal mass of the plasma species (_me=_mp$m_e=m_p$, where _me$m_e$ and _mp$m_p$ are electron and positron mass, respectively), the degenerate EP plasma system supports the K-dV solitons which are associated with either fast or slow magnetosonic perturbation modes. It is also found that the basic features of the electromagnetic solitary structures, which are found to exist in such a degenerate EP plasma, are significantly modified by the effects of degenerate electron and positron pressures. The applications of the results in an EP plasma medium, which occurs in compact astrophysical objects, particularly in white dwarfs, have been briefly discussed.     

Positron nonextensivity contributions on the rational solitonic,periodic, dissipative structures for MKP equation described critical plasmas

New closed forms have been exposed that rational, trigonometric, periodical, explosive, hyperbolic and shock solutions can be usable in the ionosphere plasma of earth. To explore the nonextensive impacts on the features of nonlinear waves in this plasma model, using Riccati-Bernoulli sub-ODE process, the MKP equation has been solved. This method is very important in the study of dynamics and motion in fluids. Some of the obtained new potential solutions are prefect achievements in plasma observations and applications in ionosphere.     

正电子素的络合作用

本文介绍了正电子素及其络合作用。讨论了正电子素络合反应速度常数的测量方法。比较了几种线性自由能的表达式。     

Bifurcation analysis of ion-acoustic waves for Schrödinger equation in nonextensive Solar wind plasma

Bifurcation analysis of ion-acoustic wave (IAWs) solutions of the nonlinear Schrödinger equation (NLSE) is explored for the first time in an electron-ion (e-i) magnetized solar wind plasma. The existence of ion-acoustic (IA) periodic, superperiodic, kink, antikink, compressive and rarefactive solitary wave solutions are revealed. Special values of Solar wind plasma parameters at a normalized distance from the Sun are considered for numerical simulation. The IA wave solutions are derived analytically. These solutions are analyzed numerically considering the influence of parameters, namely, wave number (k), velocity (V) of traveling wave and nonextensive parameter (q). Computational simulation reveals that only IA periodic wave grows in amplitude as waves moves from the Sun.     

基于振动模型的呼吸运动估计与伪影反卷积校正

PET／CT图像的呼吸运动伪影严重影响胸腹部肿瘤的诊断与治疗计划的制定。现有的伪影校正方法大都涉及呼吸门控设备和四维CT的使用,不仅给测试带来不便,还让患者遭受大剂量的CT照射从而对其造成额外伤害。为此,采用正弦振动来模拟呼吸运动,通过对仿真和体模图像倒谱的Radon变换来估算呼吸运动的幅度和方向,然后分别采用维纳滤波、约束最小二乘法和Richardson—Lucy迭代算法,根据估计的运动参数对伪影图像进行反卷积并比较它们的去伪影结果。仿真与体模实验结果均显示出模拟呼吸运动参数估计和伪影校正的良好结果．且方法安全、简便而经济,有望用于常规采集的静态PET图像呼吸伪影校正。     

透明导电氧化物薄膜的抗伽马辐照性能研究

利用射频磁控溅射法制备出具有良好光电性能的In₂O₃: W（IWO）薄膜,与购置的In₂O₃: Sn（ITO）薄膜一起,在伽马射线地面加速模拟试验设备中进行辐照试验。对辐照前后两种薄膜样品的微观结构、表面形貌、光电性能和元素价态进行对比分析,并用正电子湮没方法研究辐照前后的缺陷情况。结果表明,伽马射线辐照可引起ITO及IWO薄膜样品中氧空位缺陷的少量增加,且缺陷主要产生于薄膜表层及薄膜与基底界面结合处。高能伽马光子作用于透明导电氧化物薄膜,主要通过破坏其内部结合能较低的化学键,并实现薄膜系统中元素之间的选择性重组。ITO与IWO具有良好的抗伽马辐照性能,IWO相比ITO更适合于抗伽马辐照相关应用。