Cosmology

 From the Quantum to the Cosmic

We investigate the full chronological sweep of cosmic history — tracing the evolution of the cosmos from its primordial birth to its current accelerated expansion. Work begins at the earliest epochs, exploring how microscopic quantum fluctuations in the infant universe laid the seeds for the massive galaxies and galaxy clusters we observe today. We focus heavily on:


Cosmic Inflation: Understanding the mechanism that drove the rapid expansion of the early universe.

Large-Scale Structure: Studying how matter clustered over billions of years to form the "cosmic web."

Gravity & Geometry: Investigating Modified Gravity theories and the nature of spacetime itself to address open puzzles like
                                      Matter-Antimatter Asymmetry, Dark Energy, the Hubble Tension and other cosmological tensions or anomalies.

 We believe that rigorous mathematics must be grounded in physical evidence. By confronting our theoretical models with the latest data of Cosmic Microwave Background (CMB), Large-scale galaxy distributions, Gravitational wave observations, etc., we aim to refine our understanding of the fundamental laws governing the universe.