Probing the physics of the early universe with pulsating stars
Earl Patrick Bellinger· Yale University
Thu, Oct 15 · 18:00 UTC · Online
Pulsating ancient stars preserve information about distance, chemical composition and age that can constrain the early history of galaxies. Earl Patrick Bellinger describes advances in stellar-evolution and pulsation simulations, together with machine-learning acceleration, that allow these stellar records to test models of galaxy formation. The talk develops two applications. RR Lyrae stars trace the Galactic halo and Milky Way dwarf galaxies; a new physics-informed approach to their observations enables distance precision of about one percent almost to the Milky Way’s virial radius, supporting galactic archaeology and nearby-universe cosmology. For the distant universe, the presentation examines JWST’s Little Red Dots and evidence for an interpretation as pulsating quasi-stars: black holes surrounded by supermassive, Cepheid-like stellar envelopes. If confirmed, this interpretation could explain both the Little Red Dots and the early formation of supermassive black holes.