It used to be really hot around here, but everything blew away from us in the explosion, and has continued to cool and expand over time, leaving it relatively cool around here after 14 billion years. We can see remnants of the explosion 14 billion light years away, as the CMB emitter. We can see closer remnants that have cooled and coalesced into galaxies. We cannot yet see the hotter portions of the explosion that are beyond the CMB-emitter [on the other side of the brehmstrahlung opacity wall]. As time passes, we will continue to see further and further away. One billion years from now, we will see a CMB-emitter that is 15 billion light-years away, matter which we can't yet see because it's beyond the CMB-emitter, in our reference frame. In its own reference frame, it too has cooled extensively and formed galaxies - we just can't see it yet due to the finite speed of light.
Repeating yourself over and over doesn't make your pet theory correct.
CMB-emitter?
:roflmao: