Early galaxies contribute to the 'afterglow' of the universe #319
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Stars are not perfect black body so how does that works? |
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Actually this foreground could be responsible for 100% of the CMB?
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I know a lot is made out of the black body spectrum, but maybe it's importance is over-stated? If you look at the image in this comment, you can see from the top it's a pretty good black body, but at the bottom, it's also not perfect. https://github.com/orgs/a-cosmology-group/discussions/237#discussioncomment-9834211 Also, any one point on the sky will appear to be a black body. If you move to another nearby point you'll get a different, (though still pretty close), black body spectrum. If you take a star's spectrum, it's kind of like a black body, close enough to use as an approximation. If you zoom out far enough, doesn't it the approximation get closer and closer? It seems like if the spectrum peaks orders of magnitudes lower than a stars, that the deviations from a perfect black body would decrease too. Though I'm sure there are mathematically more rigorous ways to show that the CMB's spectrum is indeed the nearest to perfect we've found. I don't really have a solid point here. Just kind of musing on the latest development. |
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Good explanation of the paper here https://youtu.be/Xb69yPNgX-Q |
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The CMB is not what you think. Eda Gjergo and Pavel Kroupa show that some of the background radiation comes from early galaxies. This contribution is larger, by a factor of a hundred, than the fluctuations on the CMB used to derive cosmological parameters in the Big Bang model.
Another falsification of the hypothesis that the CMB is the afterglow of a Big Bang.
Published paper: https://linkinghub.elsevier.com/retrieve/pii/S0550321325001403
arXiv preprint: https://arxiv.org/abs/2505.04687
Press release: https://phys.org/news/2025-05-early-galaxies-contribute-afterglow-universe.html
<<However, the variations in the background radiation that form the basis of this theory [Big Bang] are only a few thousandths of a percentage point. The question now is how reliable these measurements can actually be if elliptical galaxies (which are also not uniformly distributed) account for at least 1.4% of the total measured radiation.>>
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