MSc Thesis: From Quantum Fields to Cosmic Structures: Tracing the Early Universe through Correlation Functions
Under the kind guidance of Dr. Debaprashad Maity
Our current understanding of gravity is limited by observational constraints. While building a particle accelerator the size of the solar system isn't feasible, the universe has provided an alternative. Inflation, the highest-energy process in the early universe, acts as a natural laboratory. My thesis explored how particle production and quantum field dynamics during this era imprint on cosmological correlation functions, with a focus on non-Gaussianity and observable signatures in the CMB. This work introduces reheating into collider physics to study its distinct imprint on the CMB, aiming to make a distinction between signals of particle production and particle interactions.