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Exact plane gravitational waves and electromagnetic fields

机译:精确的平面重力波和电磁场

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The behaviour of a "test" electromagnetic field in the background of an exact gravitational plane wave is investigated in the framework of Einstein's general relativity. We have expressed the general solution to the de Rham equations as a Fourier-like integral. In the general case we have reduced the problem to a set of ordinary differential equations and have explicitly written the solution in the case of linear polarization of the gravitational wave. We have expressed our results by means of Fermi normal coordinates (FNC), which define the proper reference frame of the laboratory. Moreover, we have provided some Gedanken experiments, which show that an external gravitational wave induces measurable effects of a nontidal nature via electromagnetic interaction. Consequently it is not possible to eliminate gravitational effects on electromagnetic field, even in an arbitrarily small spatial region around an observer freely falling in the field of a gravitational wave. This is in contrast to the case of mechanical interaction involving measurements of geodesic deviation effects. This behaviour is not in contrast with the principle of equivalence, which applies to arbitrarily small regions of both space and time. (C) 2000 academic Press. [References: 24]
机译:在爱因斯坦广义相对论的框架下,研究了精确重力平面波背景下“测试”电磁场的行为。我们已经将de Rham方程的一般解表示为傅立叶式积分。在一般情况下,我们已将问题简化为一组常微分方程,并已明确写出了重力波线性极化情况下的解。我们已经通过费米法线(FNC)表示了我们的结果,该费米法线定义了实验室的正确参考系。此外,我们提供了一些Gedanken实验,这些实验表明外部引力波通过电磁相互作用感应出非潮汐性的可测量效果。因此,即使在自由落入重力波场的观察者周围的任意小的空间区域中,也无法消除对电磁场的重力影响。这与涉及测地线偏差效应的机械相互作用的情况相反。这种行为与等价原理相反,后者适用于时空上任意小的区域。 (C)2000学术出版社。 [参考:24]

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