Monday, April 28, 2014

The background radiation

Imagine if this chart was the density of free protons, going right to left,  from the atom to the edge of the universe.  At the edge of the universe, there is no vacuum density to support the proton, it dissipates. What would the light wave numbers look like on that way back. Light will not readily form, right way, but  as soon as the protons are near instability, we get light emission returning. The returning radiation matching the free proton density on the way down.



Why would free protons be migrating outward? They help stabilize far field gravity?  How would a bunch of, not quite so stupid, protons figure that out? The didn't, they just happened to match their returning light and phase locked in one of those usual equilibriums the vacuum does.

No comments: