角动量和动力摩擦对结构形成的影响:III.暗能量的影响

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Reports Pub Date : 2024-05-08 DOI:10.1134/S1063772924700021
Antonino Del Popolo
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引用次数: 0

摘要

摘要我们研究了修改暗能量状态方程参数(\(w\))对先前研究[1](以下简称论文II)结果的影响,在先前的研究中,暗能量被假定为宇宙学常数。第一步,通过求解运动方程,我们找到了质量(\(M\))和回转半径(\({{R}_{0}}}\)之间的关系。然后,我们得到了速度({v})和半径(R)之间的关系。将这一关系拟合到论文 II 中使用的星团数据中,得到了星团的哈勃参数和质量(\(M\))。与论文二的结果(\(w = - 1\) )和\(w = - 1{\text{/}3\)的情况相比,我们观察到质量(M\)明显减小,而哈勃常数从\(w = - 1\) 增加到\(w = - 1{\text{/}3\)。
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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On the Influence of Angular Momentum and Dynamical Friction on Structure Formation: III. The Effect of Dark Energy

We study the effect of modifying the equation of state parameter (\(w\)) of dark energy on the results of the previous study [1] (hereafter Paper II), in which dark energy was assumed to be a cosmological constant. As a first step, solving the equation of motion, we found a relation between mass, \(M\), and the turn-around radius, \({{R}_{0}}\). Then, we obtained a relationship between the velocity, \({v}\), and radius, \(R\). The relation was fitted to data of the groups used in Paper II to obtain the Hubble parameter, and the mass, \(M\) of the groups. We observe a significant reduction of the mass, \(M\), comparing Paper II results (for which \(w = - 1\)) and the case \(w = - 1{\text{/}}3\), while the Hubble constant increases going from \(w = - 1\) to \(w = - 1{\text{/}}3\).

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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