vizart said:
I see your point and apologize for misjudgment. But the question is still open to me: assuming a compact universe with no boundary, what will happen to the observed CMB in later times?
Vizart, are you OK with the idea of a compact U with no boundary which expands forever due to positive cosmological constant Lambda?
That is one version of the widely used "standard" or "consensus" universe model, the LambdaCDM. The other version of the standard cosmo model is spatially infinite.
No wise person would claim to know the right model, but one has to have some model to fit the data to and the LCDM gives a remarkably good fit (either spatial finite or spatial infinite) and has become the preferred one to use.
So if you are talking about LCDM, then it is easy to answer your question. The observed CMB just slowly fades. Wavelengths lengthen and the temperature declines forever---as the U expands forever.
A prominent cosmologist, Larry Krauss, wrote a paper describing this and other aspects of the indefinite future (according to LCDM). He pointed out that in the far future the cosmologists if there are any would not be able to detect the Background because it will be too redshifted. He pointed out that although the U keeps expanding the imagined future scientists will not have all the clues that we have, and may not realize it is expanding. If you are curious in such far-distant matters, the Krauss paper is called "return of a static universe and the end of cosmology"
If you google "Krauss static" you will get the free online preprint:
http://arxiv.org/abs/0704.0221
Or google "Krauss end cosmology".
Working cosmologists normally assume no boundary. I wouldn't speculate about the case where there was a boundary. What would it be like?
Keeping within the no-boundary assumption, there is the spatial compact and spatial infinite distinction. It doesn't seem to make any difference---the CMB just keeps on redshifting as the U expands. I'm probably repeating what others have already replied in this thread.