共查询到20条相似文献,搜索用时 62 毫秒
1.
2.
本文讨论了U(1)点磁荷场中零能费米子解的个数及其物理性质,特别是轴矢流部分守恒的反常源为磁荷,及电荷的有效分布集中在磁荷点的现象.本文又采用同步规范局部坐标系明显地将任意同位旋自旋(1/2)粒子在球对称 SU(2)无源场中的方程分离变量.证明了零能解仅有 J=0,|q|=(1/2);J=(1/2),|q|=1,0的情况,并且明显地求出了同位旋 I 为任意半整数及1时的解. 相似文献
3.
讨论了高能强子 -强子散射过程中的坡密子以及坡密子的 QCD内容 .认为坡密子有可能就是具有量子数 IG=0 + ,JPC=2 + +的张量胶子球 ξ( 2 2 30 ) .用雷其化胶子球模型计算了高能质子 -质子散射截面和坡密子 -核子的耦合参数 β.理论结果与实验的要求一致. The pomeron in high energy hadron hadron scattering as well as the QCD nature of the pomeron are discussed. We claimed that the pomeron may be the tenser glueball ξ(2 230) with quantum number I G =0 +, J PC =2 ++ . Under this reggeized glueball model the cross section of high energy proton proton scattering and the coupling parameter of the pomeron nucleon, β , are calculated. The theoretical results of the present model are in good agreement with experimental data. 相似文献
4.
5.
6.
7.
近年来人们对变折射率分布中的球对称分布的研究日渐重视。本文进一步深入分析了球对称折射率分布,证明球对称分布中光线的倾斜度核心值即为其积分不变量;一个令人惊异的结果是,麦克斯韦透镜中任意共轭点之间的光程都相等,并可用分布参数表为π/2n0a。 相似文献
8.
9.
10.
本文将导出重力场中粒子按高度分布的精确表达式,然后将这一分布应用于大气:估算大气的总重量;导出由大气压确定高度的近似表式. 相似文献
11.
12.
ZHANG Yuan-zhong 《理论物理通讯》1984,3(5):551-564
In this paper Newtonian limit in the Poincare gauge field theory of gravitation is investigated. In spherically symmetric and static cases interior and exterior solutions of the linearized field equations with gravitational sourtion are obtained by maens of Green's function for the five Lagrangians with out ghosts and tachyons. In cases of four Lagrangians,the space-time metrics outside gravitational source are the usual Schwarzschild one of the first-older, while in the case of the fifth hagrangian the space-time metric differs from the Schwarzschild one. Under both,Newtonian and-weak gravitational field approximations,the motion of a test particle without span should therefore be different from Newton's second law. As a result of the exchanged particles of spin o+ the deviation from Newton's second law is a Yukawa term which is attractive. A distance-dependent gravitational "constant" G(r) can be defined according to the new result. The difference between G(r) and Newton's gravitational constant G∞ is due to a nonzero component of torsion tensor, the effect of which can be tested by measuring G(r). 相似文献
13.
14.
15.
16.
17.
18.
STATIC SPHERICALLY SYMMETRIC SOLUTION OF EINSTEIN GRAVITY COUPLED TO ELECTRO-MAGNETIC AND SCALAR FIELDS 下载免费PDF全文
The static spherically symmetric solution of Einstein gravity coupled to electromagnetic and scalar fields is obtained under the consideration of the self-gravitational interaction of the electromagnetic and scalar fields, which is singularity-free and stable. 相似文献
19.