Inflation Theory is a cosmological model that suggests a rapid expansion of the universe occurred just after the Big Bang, driven by a form of energy that caused the universe to grow exponentially in size within a fraction of a second. This theory helps explain several observations about the universe, such as its large-scale uniformity and the distribution of cosmic microwave background radiation. By proposing that this brief period of extreme inflation smoothed out any irregularities, it provides a crucial framework for understanding the early moments of the universe's existence.
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