THE MODULATION PRINCIPLE OF VACUUM ON THE SUPERCONDUCTIVITY OF YBCO

By neutron diffraction and other experiments, we have found that oxygen ions in YBCO can diffuse out of the sample in vacuo at room and low temperature, while the T(c) decreases greatly. We have also found that if the vacuum-deoxidation process lasts for several days there will be a damping oscillation of T(c) with time (t), and higher vacuum corresponds to a greater amplitude and a shorter period. We tentatively think that T(c) should satisfy the following function: T(c0) is-proportional-to T(c)e(-betat)cos (omegat + phi); it may be due to the diffusion of oxygen and the saturation of the valence state.

由QCD求和规则计算s夸克质量

简要回顾了量子色动力学求和规则在计算s夸克质量方面的应用。结合Dominguez,Gend和Paver的工作,重新考虑渐近自由阈以下的谱函数后,计算了s夸克的质量,得到s夸克的跑动质量-ms(1 GeV)=219 MeV。讨论了影响计算结果精度的可能因素。

QCD求和规则与强子物理

量子色动力学(QCD)求和规则是强子物理研究中的一种重要的非微扰方法,已经成为强子物理与核物理研究中有力的工具。简单介绍了QCD求和规则的基本概念、方法与应用,特别讨论了QCD求和规则近年来的发展和与之相关的一些前沿问题。

Vacuum window of intermediate energy heavy-ion microbeam irradiation facility

The beam must be extracted into the air through the vacuum window to irradiate the living cell. In the window design, the material and thickness must be chosen to compromise the beam spot size broadening and the window safety. The structure-static analysis on the window of different structures and materials is done with the finite element analysis method, and the deformation and the equivalent stress axe simulated. The safety of these candidates is investigated using the intensity theory. In addition, the small angle scattering and the transverse range of ions are simulated using SRIM code, including all the effects on the beam spot size broadening, such as the incident ion energy, the material and the thickness of the window and the air composing. At last, the appropriate vacuum windows are presented, including the structure, material and thickness.

Deconfinement phase Transition including perturbative QCD corrections in (proto)neutron star matter

Deconfinement phase transition and neutrino trapping in (proto)neutron star matter are investigated in a chiral hadronic model (also referred to as the FST model) for the hadronic phase (HP) and in the color-flavor-locked (CFL) quark model for the deconfined quark phase. We include a perturbative QCD correction parameter alpha(s) in the CFL quark matter equation of states. It is shown that the CFL quark core with K-0 condensation forms in neutron star matter with the large value of alpha(s). If the small value of alpha(s) is taken, hyperons suppress the CFL quark phase and the HP is dominant in the high-density region of (proto)neutron star matter. Neutrino trapping makes the fraction of the CFL quark matter decrease compared with those without neutrino trapping. Moreover, increasing the QCD correction parameter alpha(s) or decreasing the bag constant B and the strange quark mass m(s) can make the fraction of the CFL quark matter increase, simultaneously, the fraction of neutrino in protoneutron star matter increases, too. The maximum masses and the corresponding radii of (proto)neutron stars are not sensitive to the QCD correction parameter alpha(s).

General SU(2)(L) x SU(2)(R) x U(1)(EM) sigma model with external sources, dynamical breaking and spontaneous vacuum symmetry breaking

We give a general SU(2)(L) x SU(2)(R) x U(1)(EM) sigma model with external sources, dynamical breaking and spontaneous vacuum symmetry breaking, and present the general formulation of the model. It is found that sigma and pi(0) without electric charges have electromagnetic interaction effects coming front the internal structures. A general Lorentz transformation relative to external sources J(gauge) - (J(A mu) J(A mu)(kappa)) derived, using the general Lorentz transformation and the four-dimensional current of nuclear matter of the ground si ate with J(gauge) = 0, we give the four-dimensional general relations between the different currents of nuclear matter systems with J(gauge) not equal 0 and those with J(gauge) = 0. The relation of the density's coupling with external magnetic field is derived, which conforms well to dense nuclear matter in a strong magnetic field. We show different condensed effects in strong interaction about fermions and antifermions, and give the concrete scalar and pseudoscalar condensed expressions of sigma(0) and pi(0) bosons. About different dynamical breaking and spontaneous vacuum symmetry breaking, the concrete expressions of different mass spectra are obtained in field theory. This paper acquires the running spontaneous vacuum breaking value sigma'(0), and obtains the spontaneous vacuum breaking in tenus of the running sigma'(0), which make nucleon, sigma, and pi particles gain effective masses. We achieve both the effect of external sources and nonvanishing value of the condensed scalar and pseudoscalar paticles. It is deduced that the masses of nucleons, sigma and pi generally depend on different external sources.

HIRFL大型真空系统；The vacuum system of HIRFL

HIRFL是兰州重离子加速器装置的英文首字母缩写,其真空系统是一个大型综合性系统。HIRFL由离子源、扇聚焦回旋加速器SFC、分离扇回旋加速器SSC和多用途的重离子冷却储存环(HIRFL-CSR)组成。多条束流运输线将这些加速器连接在一起,同时将各种重离子束流送往10多个实验终端。根据加速离子和束流寿命的需要,对各加速器真空度的要求是不同的:SFC已有50多年的历史,经过3次升级改造,真空度从10-4 Pa提高到10-6 Pa;建于上世纪八十年代的SSC真空度也为10-6 Pa;而两个重离子冷却储存环(CSRm和CSRe)的真空度达到10-10Pa以保证重离子有足够长的储存寿命。多条连接束运线根据不同实验终端的要求,其真空系统的设计方案也不同,文中列举了微束实验终端采取的防振措施;为充气反冲谱仪设计的清洁、大流量真空差分系统及为重离子治癌等终端设计的超薄壁扫描磁铁真空管道等。

QCD求和规则对S夸克质量的研究

QCD求和规则是强子物理中的一种非常有效的非微扰方法，它从流的算符乘积展开开始，引入算符乘积展开式的真空期望值，把微扰和非微扰效应分开处理：微扰效应包含在展开系数中，非微扰效应则由算符的真空凝聚值表示。然后利用色散关系，把算符乘积展开式的真空期望值与一个含有强子物理参数的色散积分联系起来，这样就能够计算有关强子的物理量。 本文首先系统介绍了QCD求和规则的基本原理、基本方法，然后结合Dominguez，Gend和Paver的工作[14]，展开式保留了的算符d=4凝聚值，采用新的参数化渐近自由阈以下谱函数的方法：即根据文献[25]，用实验上了解得比较清楚的两个共振态的贡献来参数化谱函数，计算了s夸克的质量，得到了在动量标度为1Gev时，s夸克的跑动质量为219MeV。在误差范围内，这是一个理论上可以接受的结果，本文计算得到的跑动质量的值能为考察动量转移为1GeV时的质量效应提供参考。 关键词：QCD求和规则 算符乘积展开 色散关系 Borel变换 夸克质

Enlarged area A-type zeolite membranes prepared by vacuum seeding method

High quality A-type zeolite membranes, with enlarged area over 70 cm(2), were successfully synthesized on a tubular alpha-Al2O3 support by applying the vacuum seeding method.