Pressure-Regulated Feedback-Modulated Star Formation Model: A Plausible Explanation for High-z Galaxies

Explore a 20-minute conference talk on the Pressure-Regulated Feedback-Modulated Star Formation Model presented by Sultan Hassan from NYU at the Kavli Institute for Theoretical Physics. Delve into a plausible explanation for the abundance of high-redshift galaxies observed by the James Webb Space Telescope (JWST) and its implications for cosmic reionization. Gain insights into the exciting exploration of cosmic dawn and how JWST observations provide a unique "stress test" for new theoretical models of galaxy formation. Discover key questions addressed in the talk, including the nature of first stars and black hole seeds, stellar populations in early galaxies, and the physical processes shaping the evolution of these galaxies and their black holes. Learn how this research connects near-field and deep field observations, contributing to our understanding of the universe's early stages.