非线性共形引力

J.-F. Pommaret
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引用次数: 0

摘要

1909年,e·科塞拉特和f·科塞拉特兄弟发现了一种新的非线性群理论方法来研究弹性(EL),唯一的实验需要是测量EL常数。在现代框架中,他们使用非线性Spencer序列代替非线性Janet序列来定义空间刚性运动群的李群。继H. Weyl之后,我们的目的是首次计算定义时空共形群的李群的线性和非线性Spencer序列,以便为电磁学(EM)和引力(GR)提供数学基础,唯一的实验需要是测量EM和GR常数。对于维数n≥3的流形,困难在于处理E. Cartan在1922年称为“关系”的n个非线性变换。利用维数n = 4对于Spencer上同调的计算具有非常特殊的性质,我们也证明了(非线性)coserat电磁场或感应方程与(线性)Maxwell电磁场或感应方程之间没有概念上的区别。至于万有引力,维度n = 4也允许在除中心吸引质量外的任何地方都有一个共形因子,因为由二阶射流形成的各向同性亚群的反转定律将吸引力转化为排斥力。电磁学和万有引力的数学基础因此只依赖于时空共形伪群的结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Nonlinear Conformal Gravitation
In 1909 the brothers E. and F. Cosserat discovered a new nonlinear group theoretical approach to elasticity (EL), with the only experimental need to measure the EL constants. In a modern framework, they used the nonlinear Spencer sequence instead of the nonlinear Janet sequence for the Lie groupoid defining the group of rigid motions of space. Following H. Weyl, our purpose is to compute for the first time the linear and nonlinear Spencer sequences for the Lie groupoid defining the conformal group of space-time in order to provide the mathematical foundations of both electromagnetism (EM) and gravitation (GR), with the only experimental need to measure the EM and GR constants. With a manifold of dimension n ≥ 3, the difficulty is to deal with the n nonlinear transformations that have been called “elations” by E. Cartan in 1922. Using the fact that dimension n = 4 has very specific properties for the computation of the Spencer cohomology, we also prove that there is no conceptual difference between the (nonlinear) Cosserat EL field or induction equations and the (linear) Maxwell EM field or induction equations. As for gravitation, the dimension n = 4 also allows to have a conformal factor defined everywhere but at the central attractive mass because the inversion law of the isotropy subgroupoid made by second order jets transforms attraction into repulsion. The mathematical foundations of both electromagnetism and gravitation are thus only depending on the structure of the conformal pseudogroup of space-time.
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