OK, here's what I know (probably with many inaccuracies, but feel free to correct me):
The "oldest" picture of the universe we have is the Cosmic Microwave Background Radiation image.
It shows a constant background radiation that exists throughout the universe at a constant 3 Kevin (K).
We initially believed that there were no fluctuations in that radiation level, until we took the picture I linked to above, which shows variances of micro kelvins. Those differences are evidence showing slight differences that could account for hydrogen coming together to form stars, and eventually, other galaxies.
But what theories do we have to explain the initial differences in these radiation levels?
The "oldest" picture of the universe we have is the Cosmic Microwave Background Radiation image.
It shows a constant background radiation that exists throughout the universe at a constant 3 Kevin (K).
We initially believed that there were no fluctuations in that radiation level, until we took the picture I linked to above, which shows variances of micro kelvins. Those differences are evidence showing slight differences that could account for hydrogen coming together to form stars, and eventually, other galaxies.
But what theories do we have to explain the initial differences in these radiation levels?