Transition of IMF in the Early Universe
Offered By: Kavli Institute for Theoretical Physics via YouTube
Course Description
Overview
Explore the transition of the Initial Mass Function (IMF) in the early universe through this 19-minute conference talk by Sunmyon Chon from the Max Planck Institute for Astrophysics. Delve into cutting-edge research presented at the "Cosmic Dawn Revealed by JWST: The Physics of the First Stars, Galaxies, and Black Holes" conference held at the Kavli Institute for Theoretical Physics. Gain insights into the nature of first stars, black hole seeds, and early galaxy formation as observed by the James Webb Space Telescope. Examine the connection between near-field and deep field observations, and understand the key physical processes shaping the evolution of early galaxies and their black holes. Discover how this talk contributes to the broader discussion on star formation, chemical enrichment, and stellar populations in the first galaxies, providing a unique perspective on the cosmic dawn era.
Syllabus
Transition of IMF in the Early universe (H) ▸ Sunmyon Chon (MPA)
Taught by
Kavli Institute for Theoretical Physics
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