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I saw this question (in a far removed forum), and I thought it was interesting. Do we have any theoretical reason (or observations) that would suggest that inflation change the fine structure constant.
I understood pervect's question to be, not has alpha varied over cosmological time, but during the period of inflation.there is no credible evidence 'alpha' has varied over time.
Cosmic inflation is a theory that explains the rapid expansion of the universe in the first fraction of a second after the Big Bang. It is important because it helps to explain the large-scale structure and uniformity of the universe, as well as the origin of galaxies and other cosmic structures.
The fine structure constant is a fundamental constant of nature that describes the strength of the electromagnetic force. Cosmic inflation is thought to have caused small variations in the density of matter in the early universe, which in turn affected the value of the fine structure constant. This has implications for the evolution of the universe and the formation of galaxies.
One of the strongest pieces of evidence for cosmic inflation is the cosmic microwave background (CMB) radiation. This is a faint glow of radiation that permeates the entire universe and is thought to be leftover radiation from the Big Bang. The CMB shows patterns that are consistent with the predictions of cosmic inflation.
The fine structure constant can be measured in a number of ways, including through laboratory experiments and astronomical observations. For example, scientists can study the spectral lines of atoms to determine the value of the constant. They can also observe the effects of the constant on the behavior of particles and fields in the universe.
Understanding cosmic inflation and the fine structure constant can help us to better understand the origins and evolution of the universe. It also has implications for our understanding of the fundamental laws of nature and the potential for new discoveries in physics. Additionally, this knowledge can inform future research and technological advancements.