معرفی
Maximiliano Silva-Feaver is a Mossman Postdoctoral Fellow at Yale University's Wright Laboratory specializing in experimental cosmology and dark matter detection, with active roles in the Simons Observatory, HAYSTAC, and ALPHA collaborations.
His academic qualifications include:
- Ph.D. in Physics, University of California, San Diego (2023)
- Bachelor's in Physics, Santa Clara University (2015)
Dr. Silva-Feaver's research bridges cosmological observation and particle-scale dark matter detection. As an experimentalist, he pioneers instrumentation for cosmic microwave background measurements through the Simons Observatory's Small Aperture Telescope and develops axion haloscopes (HAYSTAC/ALPHA) targeting micro-electronvolt mass ranges. His technical expertise spans microwave multiplexing electronics, cryogenic sensor systems, and novel plasma-resonance coupling techniques for next-generation detectors.
His recognition includes:
- Mossman Fellow (2023)
He actively advocates for early-career researcher representation in large collaborations, implementing structural changes within Simons Observatory and ALPHA governance. While specific grant funding isn't detailed, his work involves cross-institutional coordination with SLAC National Laboratory and the Flatiron Institute. Current technical leadership focuses on ALPHA's microwave receiver integration and HAYSTAC sensitivity upgrades at Yale's Wright Laboratory facilities.
