电荷密度的运动,必要的磁源和麦克斯韦方程组包括磁源的利用势解

N. Yener
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引用次数: 2

摘要

我们处理确定磁源的问题,当电荷密度突然开始任意运动时,磁源已被证明是存在的,因此,无限光速成为满足标量势和矢量势的洛伦兹条件所必需的。当施加无限光速约束时,Poynting定理方程所经历的变化是发展的基础,并且利用了所需的磁和电荷密度函数在其运动中具有相同的支撑和相同的速度这一事实。参考源区域的格林函数,得到磁源的解。磁源的计算形式为$m=Z\rho$和$\vec{M}=Z\vec{J}$,其中$Z$是可以是真空的无损简单介质的波阻抗。同时,结合磁荷和电流密度的麦克斯韦方程组的解以电荷函数发射的波具有无限传播速度的势的形式给出。磁标量势是单极矩积分形式的和。对于$t > 0$,即使得到的微分方程包含双调和算子,这些方程的特解本质上是泊松方程的解。当$t > 0$没有磁源的情况下同样的洛伦兹条件也出现在有磁源的情况下。利用亥姆霍兹定理得到了在$t=0$处洛伦兹条件失效的势的解。
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Motion of a Charge Density, Necessary Magnetic Sources and Solution of Maxwell's Equations including Magnetic Sources by Employing Potentials
We treat the problem of determining the magnetic sources that have been shown to come into existence when an electric charge density abruptly starts an arbitrary motion and hence an infinite speed of light becomes necessary for the satisfaction of the Lorenz condition for the scalar and vector potentials. The change that the Poynting theorem equation undergoes when an infinite speed of light constraint is enforced is the basis for the development and also use is made of the fact that the required magnetic and electric charge density functions share the same support and the same velocity in their motion. Reference to Green's functions in the source region is made to obtain the solution for the magnetic sources. The magnetic sources are computed to be in the form $m=Z\rho$ and $\vec{M}=Z\vec{J}$ where $Z$ is the wave impedance of the lossless, simple medium which can be vacuum. Also, the solution of Maxwell's equations incorporating the magnetic charge and current densities is given in terms of potentials with an infinite speed of propagation for the waves emitted by the charge functions. The magnetic scalar potential is a summation in the form of an integral of monopole moments. For $t > 0$ even though the resulting differential equations involve biharmonic operators, particular solutions of these equations are essentially solutions of Poisson's equations. When $t > 0$ the same Lorenz condition for the case with no magnetic sources appears also in this case with magnetic sources. The solutions for the potentials at $t=0$ where the Lorenz condition fails are obtained using the Helmholtz theorem.
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