How does cosmic inflation address the Flatness Predicament?

Answer

The exponential expansion drives the spatial geometry toward flatness (\Omega \to 1).

The intense, superluminal stretching characteristic of inflation acts to dilute any initial spatial curvature, pushing the density parameter relentlessly toward unity, thereby achieving near-perfect flatness naturally.

How does cosmic inflation address the Flatness Predicament?

#Videos

Cosmic Inflation Explained | Cosmology 101 Episode 6 - YouTube

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