论文标题
使用Heaviside-Maxwellian（Vector）重力的重力探针B的解释
Explanation of Gravity Probe B Experimental Results using Heaviside-Maxwellian (Vector) Gravity in Flat Space-time
论文作者
论文摘要
NASA的重力探针B（GP-B）实验的目的是测试爱因斯坦1916年爱因斯坦1916年的相对论张量理论的理论预测，这是弯曲的时空（一般相对性（GR））的重力理论，这些理论是在像地球一样缓慢旋转的大质量体内的陀螺仪预防旋转轴预防的旋转轴预求。 2011年，GP-B任务报告了其对四个球形陀螺仪的旋转轴的旋转轴的测量数据，该旋转轴位于卫星轨道上的卫星旋转642 km（400英里）的卫星旋转，在极地轨道上。报告的结果与GR的预测一致。在这里，我们首次报告了使用Heaviside-Maxwellian（Vector）重力（HMG）在平坦时空中对GP-B实验结果的本科级别的解释，并于1893年首次由Heaviside提出，后来被许多作者考虑/重新发现/重新发现。我们对GP-B结果的新解释提供了对HMG的新测试，除了现有的结果外，它值得以其简单性和新的观点引起该领域的研究人员的注意。
The Gravity Probe B (GP-B) Experiment of NASA was aimed to test the theoretical predictions of Einstein's 1916 relativistic tensor theory of gravity in curved space-time (General Relativity (GR)) concerning the spin axis precession of a gyroscope moving in the field of a slowly rotating massive body, like the Earth. In 2011, GP-B mission reported its measured data on the precession (displacement) angles of the spin axes of the four spherical gyroscopes housed in a satellite orbiting 642 km (400 mi) above the Earth in polar orbit. The reported results are in agreement with the predictions of GR. For the first time, here we report an undergraduate level explanation of the GP-B experimental results using Heaviside-Maxwellian (vector) Gravity (HMG) in flat space-time, first formulated by Heaviside in 1893, and later considered/re-discovered by many authors. Our new explanation of the GP-B results provides a new test of HMG apart from the existing ones, which deserves the attention of researchers in the field for its simplicity and new perspective.
