Cosmic Microwave Background Radiation (CMB). (question  edit  March 29, 2016)

Assume very dense proto-stellar formation prior to a cosmic inflation event as hypothesized in The Pearlman SPIRAL cosmological redshift hypothesis and no ongoing cosmic expansion subsequent to that cosmic inflation event.

Could the cause of the CMB be from:

Prior to the stellar formation?

During stellar formation?

Post stellar formation?

Prior to that cosmic inflation event?

during that event?

at the very end of that event?

Under The Standard Cosmology Model (SCM) the current distance to the most distant visible galaxies is 46.5 B LY. Is that understanding correct?

CMB-LEAK:

A sub-hypothesize in SPIRAL is the CMB should 'leak' have dissipated 1 LY per year radius beyond the most distant galaxy.

If valid under SCM the CMB is spread out over an area of a sphere with a radius of at least 59.99 B LY = 46.5B + 13.4B is this already established or a published hypothesis?

If CMB does not 'leak' / spread beyond the most distant stars at 1 LY per year why not?

.

Thank you in advance for any and all proposed solutions you can think of. r

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