克利福德空间中的广义相对论变换及其物理意义

C. Perelman
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引用次数: 0

摘要

对克利福德空间(C 空间)中的广义相对论的简要介绍,为明确构建 C 空间中克利福德多矢量值坐标的广义相对论变换铺平了道路。最一般的变换提供了多矢量值坐标等级的全面混合。多矢量值矩的变换会导致 C 空间中的不变广义质量 M,它与 m 不同。在广义相对论变换下,相对论色散关系 E 2 - ⃗p - ⃗p = m 2 中出现的适当质量不再保持不变。我们论证了这一发现如何可能给宇宙常数问题、暗能量和暗物质带来一些启示。最后,我们对将这些变换扩展到相空间和玻恩互易相对论作了一些总结性评论。附录中包含了克利福德代数多向量生成器的最一般(反)换元。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Generalized Relativistic Transformations in Clifford Spaces and their Physical Implications
A brief introduction of the Extended Relativity Theory in Clifford Spaces ( C - space) paves the way to the explicit construction of the generalized relativistic transformations of the Clifford multivector-valued coordinates in C -spaces. The most general transformations furnish a full mixing of the grades of the multivector-valued coordinates. The transformations of the multivector-valued momenta follow leading to an invariant generalized mass M in C -spaces which differs from m . No longer the proper mass appearing in the relativistic dispersion relation E 2 − ⃗p · ⃗p = m 2 remains invariant under the generalized relativistic transformations. It is argued how this finding might shed some light into the cosmological constant problem, dark energy, and dark matter. We finalize with some concluding remarks about extending these transformations to phase spaces and about Born reciprocal relativity. An appendix is included with the most general (anti) commutators of the Clifford algebra multivector generators.
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