论文标题
尝试通过特殊相对论技术获得一般相对论行星的运动
Attempt to obtain the general relativistic planet's motion by special relativity techniques
论文作者
论文摘要
它试图仅通过特殊相对论（SR）技术来得出行星运动及其解决方案的一般相对论（GR）方程。行星相对于太阳的运动和太阳向行星的运动是在天体力学中使用扰动理论独立于特殊的相对论框架解决的。该解决方案揭示了时空结构的性质，然后检查了它对行星运动的影响。当将如此检查的运动与PN近似中的一般相对论理论获得的运动进行比较时，两者在轨道的平均运动和半径上都不同，但与围骨围骨螺旋前序完全相同。
It is attempted to derive the general relativistic (GR) equation of motion for planet and its solution solely by the special relativity (SR) techniques. The motion of a planet relative to the sun and that of the sun to the planet are solved independently in special relativistic framework using the perturbation theory in the celestial mechanics. The solution reveals a nature of the structure of the spacetime under the gravitation of the sun, and then its effect on the planet's motion is examined. When the motion thus examined are compared with the one obtained by the general relativity theory in PN approximation, both are different concerning the mean motion and the radius of the orbit but exactly the same as for the perihelion precession.
