Inflation leads to the isotropy of the Cosmic Microwave Background (CMB) by rapidly expanding quantum fluctuations, which become the initial seeds for temperature variations observed in the CMB. These quantum fluctuations are stretched beyond the event horizon during inflation, freezing them in place. Once inflation ends, distant regions of the universe can interact again, allowing these fluctuations to manifest as irregularities in the CMB. The discussion also touches on the estimated values of primordial fluctuations and their impact on the CMB, with inquiries about relevant research papers. Understanding these processes is crucial for comprehending the early universe's structure and evolution.