INERTIAL ABSOLUTE AND RELATIVE REFERENCE SYSTEMS

V. Pavlov
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Abstract

It is noted that the problem of choosing a frame of reference for the relative motion of inertial objects of comparable mass is especially relevant for interplanetary flights at a considerable distance from the planets. There is a point of view that all inertial frames of reference are equal and the choice between them is determined solely by the convenience of calculations. The aim of the work is to determine the absolute inertial frame of reference for the relative unaccelerated motion of an arbitrary number of inert objects in three-dimensional Euclidean space and to establish its difference from relative frames of reference. For the same inert objects moving relative to each other, different coordinate systems give completely different total kinetic energies of objects. In this sense, it is not possible to recognize them as equal in rights. Obviously, none of these coordinate systems can be considered as absolute. An absolute coordinate system should be considered such a system, the choice of which completely excludes arbitrariness. This requirement is satisfied by a system in which the total kinetic energy of inert objects is minimal. The absolute coordinate system coincides with the center of mass of inert objects and with the epicenter of their hypothetical repulsion from the state (also hypothetical) of mutual immobility. After a hypothetical repulsion, the velocities of inert objects relative to the center of mass acquire the same values as in the absolute coordinate system. Along with a wide variety of reference systems in the mutual motion of unaccelerated inertial objects, including those associated with these objects (these reference systems can be considered relative), there is one absolute reference system associated with the center of mass of the considered inertial objects. The considered repulsions of inert objects are calculated and may have nothing to do with reality. The number of inert objects in determining the absolute coordinate system is not limited by anything. It can be either two objects or a star system.
惯性绝对参考系和相对参考系
应当指出,为质量相当的惯性物体的相对运动选择一个参照系的问题,对于距离行星相当远的行星际飞行尤其重要。有一种观点认为,所有的惯性参照系都是相等的,它们之间的选择完全取决于计算的便利性。本工作的目的是确定三维欧几里德空间中任意数量的惰性物体相对非加速运动的绝对惯性参考系,并确定其与相对参考系的区别。对于彼此相对运动的同一惰性物体,不同的坐标系给出的物体总动能完全不同。从这个意义上说,不可能承认他们在权利上是平等的。显然,这些坐标系都不能被认为是绝对的。绝对坐标系应该被认为是这样一个系统,它的选择完全排除了随意性。这个要求可以通过一个系统来满足,在这个系统中,惰性物体的总动能是最小的。绝对坐标系与惰性物体的质心和它们在相互不动状态(也是假设的)的假设斥力的中心一致。经过假设的斥力后,惰性物体相对于质心的速度得到与绝对坐标系中相同的值。在非加速惯性物体的相互运动中,除了各种各样的参照系,包括与这些物体相关的参照系(这些参照系可以被认为是相对的)之外,还有一个与所考虑的惯性物体的质心相关的绝对参照系。考虑惰性物体的斥力是计算出来的,可能与现实无关。在确定绝对坐标系时,不动物体的数量不受任何限制。它可以是两个物体,也可以是一个恒星系统。
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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