pith. sign in

arxiv: physics/0004036 · v1 · pith:LZXNJSFMnew · submitted 2000-04-18 · ⚛️ physics.gen-ph

Interstellar Hydrogen and Cosmic Background Radiation

classification ⚛️ physics.gen-ph
keywords radiationbackgroundcosmichydrogeninterstellarcollectioncondensationcorresponding
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.