相对论像差对宇宙学距离的影响
宇宙学与河外天体物理
2024-04-05 v2
摘要
目标：我们提出，我们与所观测的宇宙天体之间的相对运动条件应对这些天体发射的光子产生相对论像差，类似于耀变体和中子星的情况改变观测到的通量，但表现为辐射通量的降低。方法：我们遵循现代宇宙学中的一些重要论文和教科书，在宇宙的理论描述中加入相对论像差效应。结果：出现了光度距离和角距离的新定义，其结果是改变了近年来测量到的宇宙学参数。对宇宙微波背景辐射的多极分析也进行了所有这些的定性描述。
引用
@article{arxiv.2403.18567,
title = {The effect of Relativistic Aberration on Cosmological Distances},
author = {Nicolò Cedola},
journal= {arXiv preprint arXiv:2403.18567},
year = {2024}
}
备注
It was rejected by the journal, which means that this paper is wrong; the paper is based on the false assumption that galaxies are in a different reference frame in which we are, and this error is present in the "computations" section of the paper. Following this, all the results presented are wrong