Dynamics of double galactic system on the background of dark substance

L. Chechin, А. Yelibaeva
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Abstract

In this article we searched the dynamics of double galactic system (the Local Group of galaxies, as example) on the background of dark substance, including both dark energy and dark matter. For modern cosmology the study influence on the dynamics of the Local Group not only the dark energy, but also the second most important component of dark substance dark matter is rather actually today. The study of dark energy in nearby Universe becomes significant and perspective for the observations at large space scales where it was discovered for the first time. That is why we constructed the Lagrangian of such dynamical system for more correctly searching the dynamics of Local Group. Such approach allowed, instead of the initially forwarded rectilinear trajectory found its more realistic one. Talk about the real elliptical trajectory, more accurate resulting expression for the revolving time and the relaxation time due to accounting the contribution of the dark substance. The results show that the contribution of the dark substance in the total amount of revolving time of galaxies is about 10%. All these results are astronomically observable quantities and testify the strict accounting of the dark substance properties within the Local Group of galaxies.
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暗物质背景下的双星系动力学
本文在暗物质背景下对双星系系统(以本星系群为例)的动力学进行了研究,包括暗能量和暗物质。对于现代宇宙学来说,对本星系群动力学影响的研究不仅包括暗能量,还有暗物质的第二重要组成部分。对近地宇宙暗能量的研究对于在大空间尺度上首次发现暗能量具有重要意义和前景。因此,我们构造了这种动力系统的拉格朗日量,以便更准确地搜索局部群的动力学。这种方法允许,而不是最初转发的直线轨迹找到了更现实的轨迹。讨论真实的椭圆轨道,由于考虑了暗物质的贡献,得到了更准确的旋转时间和弛豫时间的表达式。结果表明,暗物质对星系总旋转时间的贡献约为10%。所有这些结果都是天文学上可观测到的数量,并证明了对本星系群中暗物质性质的严格计算。
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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