Inflationary Cosmology proposes a brief period of extremely rapid expansion in the early universe. This theory explains why the universe appears homogeneous, isotropic, and spatially flat on large scales. Inflation stretches tiny quantum fluctuations to cosmic sizes, seeding galaxy formation. It resolves conceptual problems of the standard Big Bang model, such as the horizon and flatness problems. Inflationary cosmology introduces scalar fields that drive accelerated expansion. Predictions of inflation are tested through cosmic microwave background observations. Although details remain uncertain, inflation provides a compelling framework for early-universe evolution. It represents one of the most influential ideas in modern cosmology.
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