How does cosmic inflation help explain the cosmic microwave backgroundās uniform temperature?
The high degree of isotropy in the cosmic microwave background presents a challenge known as the "light-horizon" problem. Because opposite sides of the observable universe are beyond each other's light horizons, they should not have had time to exchange information or reach a uniform temperature since the beginning of the universe.1
Cosmic inflation provides a solution to this dilemma. The theory posits that before this rapid expansion occurred, the matter and radiation that now make up the entire observable universe were in close thermal contact within a small cosmic event horizon. During this period, these regions were able to interact and acquire the same thermodynamic characteristics and temperature.12
When the universe underwent exponential inflation, these regions were stretched far apart, moving outside their individual event horizons. As the universe later resumed normal expansion, these distant portions reappeared on our horizon. Because they were in thermal equilibrium before the inflationary period, they are observed today to maintain the same uniform temperature.12