Interstellar Hydrogen and Cosmic Background Radiation
综合物理
2015-06-26 v1
摘要
It is shown that a collection of photons with nearly the same frequency exhibits a "condensation" type of phenomenon corresponding to a peak intensity. The observed cosmic background radiation can be explained from this standpoint in terms of the radiation due to fluctuations in interstellar Hydrogen.
引用
@article{arxiv.physics/0004036,
title = {Interstellar Hydrogen and Cosmic Background Radiation},
author = {B. G. Sidharth},
journal= {arXiv preprint arXiv:physics/0004036},
year = {2015}
}
备注
3 pages, TeX