基于GN-Z11星系模型频率的慢光红移

Luciano Rota
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引用次数: 0

摘要

根据波长对红移的计算,得出了某些具有偏移bbbb1的物体的回归速度可以大大超过光的回归速度的结论。本研究以2016年发现的离我们最远的星系GN-z11为模型,表明基于光速减慢导致频率降低的结果可以具体解决离我们很远的天体红移的复杂问题。与此模型相关的结果可以通过进行此处简要描述的实验进一步得到证实。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Redshift As Slow-Light on Base of Frequency on Model of Galaxy GN-Z11
The calculation of the redshift on base of wavelength leads to the conclusion that the regression speed of some body showing a shift >1 can greatly exceed that of light. This research, taking as model the most far from us galaxy GN-z11, discovered in 2016, shows that results given on base of decreasing of frequency as consequence of slowed light-speed, could concretely solve the complex question of the redshift of bodies very distant from us. The results related to this model could be further substantially confirmed by performing an experiment briefly described here.
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