Chao-Lin Kuo

Chao-Lin Kuo is Professor of Physics and Particle Physics and Astrophysics at Stanford University, specializing in cosmology and cosmic microwave background (CMB) research. His work focuses on inflationary gravitational waves, CMB polarization, and dark matter detection using millimeter-wave observations.

Key contributions include leading measurements of CMB lensing and delensed power spectra with SPT-3G data, constraining inflationary models through B-mode polarization studies with BICEP/Keck telescopes, and developing axion detection technology. Research utilizes ground-based telescopes including the South Pole Telescope and balloon-borne instruments like SPIDER.