New findings from the University of Bonn challenge the assumptions of the standard cosmological model.
The faint “afterglow” that fills the universe has long been one of the most important clues supporting the Big Bang theory. Known as cosmic microwave background radiation, this ancient light not only serves as a snapshot of the early universe, but also helps scientists understand how the very first galaxies came to be.
Now, a team of researchers from the Universities of Bonn, Prague, and Nanjing is challenging what we thought we knew. Their new calculations suggest that the strength of this background radiation may have been significantly overestimated. If their findings are confirmed, it could force scientists to rethink some of the most fundamental ideas in modern cosmology.
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