Inflationary Theory

Inflationary Theory is a scientific concept about the early universe. It suggests that just after the Big Bang, the universe underwent a rapid expansion, growing exponentially in a tiny fraction of a second. This inflation smoothed out irregularities, leading to the uniform and structured cosmos we observe today. It also explains the distribution of galaxies and cosmic background radiation. Essentially, this theory helps us understand how the universe transformed from a hot, dense state into the vast, cool cosmos we see, providing answers to fundamental questions about the origin and development of everything.