de Sitter-Fantappié-Arcidiacono射影相对论中惯性起源的一种可能机制
A possible mechanism for the origin of inertia in de Sitter-fantappié-arcidiacono projective relativity
摘要：
Fantappié-Arcidiacono投影相对论，也被称为“德西特相对论”，提供了一个力学公式，根据这个公式，可以通过运动学方法来识别惯性参考系。本文提出了惯性参考系起源于所谓的宇宙“古老时代”的假设。一个简单的机制，提出了这个过程。这样一个过程可能会留下宇宙流体颗粒，这可能会在目前的宇宙中表现为星系中的暗物质集群。
英文摘要：
Fantappié-Arcidiacono projective relativity, also known as "de Sitter relativity", provides a formulation of mechanics according to which it is possible to identify an inertial frame of reference by means of kinematic methods. This article presents the hypothesis that inertial frames of reference originated during the so-called "archaic era" of the Universe. A simple mechanism is proposed for this process. Such a process could leave behind cosmic fluid granulation, which could manifest itself in the present Universe as a clustering of dark matter in galaxies.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
