Newtonian Gravitational Waves from a Continuum

Peter Vadasz
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Abstract

Gravitational waves are being shown to derive directly from Newtonian dynamics for a continuous mass distribution, e g compressible fluids or equivalent. It is shown that the equations governing a continuous mass distribution, i e the inviscid Navier Stokes equations for a general variable gravitational field g(t,x), are equivalent to a form identical to Maxwell equations from electromagnetism, subject to a specified condition. The consequence of this equivalence is the creation of gravity waves that propagate at finite speed. The latter implies that Newtonian gravitation as presented in this paper is not spooky action at a distance but rather is similar to electromagnetic waves propagating at finite speed, despite the apparent form appearing in the integrated field formula. In addition, this proves that in analogy to Maxwell equations the Newtonian gravitation equations are Lorentz invariant for waves propagating at the speed of light.
来自连续体的牛顿引力波
引力波是直接从连续质量分布的牛顿和动力学(例如可压缩流体或等价物)中推导出来的。研究表明,管理连续质量分布的方程,即针对一般可变引力场 g(t,x) 的不粘性纳维-斯托克斯方程,与电磁学中的马克斯韦勒方程等价,但须满足一个特定条件。这一等价关系的结果是产生了以有限速度传播的引力波。后者意味着本文提出的牛顿万有引力不是距离上的幽灵作用,而是类似于以有限速度传播的电磁波,尽管在积分场公式中出现了明显的形式。此外,这还证明,与麦克斯韦方程相比,牛顿万有引力方程对于以光速传播的波是洛伦兹不变的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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