论文标题
Snell的Schwarzschild Black Hole的定律
Snell's law for the Schwarzschild black hole
论文作者
论文摘要
Fizieeev发现,用于引力场中电磁干扰的Wheeler方程在事件范围上方和下方都具有精确的溶液,以向内和外部传播的波的形式。可以从光学的角度来解释和验证该观察结果,这完全是基于Schwarzschild指标的长度收缩和时间扩张,以便为Schwarzschild Black Hole提供差异版本。它揭示了有趣的物理学,包括黑洞的内部和外部Oppenheimer-Snyder锥,其声子球的特性以及结论是,灯光以长度的收缩和时间膨胀而不是偏转而保持在地平线以下,而不是偏转。
The Wheeler equation, for electromagnetic disturbances in a gravitational field, was found by Fiziev to have exact solutions both above and below the event horizon, in the form of waves propagating both inwardly and outwardly. This observation can be interpreted and verified from the optical point of view, entirely on the basis of the Schwarzschild metric for length contraction and time dilation, in order to derive a differential version of Snell's law for the Schwarzschild black hole. It reveals interesting physics, including the correct amount of light deflection by the Sun, internal and external Oppenheimer-Snyder cones of the black hole, properties of its phonon sphere and the conclusion that light-rays are kept below the horizon by length contraction and time dilation rather than deflection.