Overview
I am a professor in the physics department studying particle physics and cosmology. I try to understand both the nature of the ghostly particles called neutrinos in giant detectors deep underground, and why the expansion of the universe is accelerating using telescopes on top of mountains. My background and training is originally in particle physics and I was part of the team that showed the sub-atomic particles called neutrinos have mass. The leader of our team, T. Kajita was co-awarded the 2015 Nobel Prize in Physics for this discovery which cited the work of our collaboration. I also began the effort in observational cosmology at Duke, joining the Vera C. Rubin Observatory, a giant telescope under construction in Chile designed to make a 10 year, three dimensional survey of the entire visible sky. Using the Rubin Observatory, we will focus on examining billions of galaxies, along with supernovae and other astronomical probes to try to determine the nature of the mysterious “Dark Energy” which is unaccountably causing the universe to pushed apart at a faster and faster rate.
Current Duke Appointments & Affiliations
Professor of Physics
·
2017 - Present
Physics,
Trinity College of Arts & Sciences
Chair of Physics
·
2025 - Present
Physics,
Trinity College of Arts & Sciences
Recent Scholarly Works
Photometric redshift estimation for Rubin Observatory Data Preview 1 with Redshift Assessment Infrastructure Layers
Journal article Monthly Notices of the Royal Astronomical Society · August 1, 2026 We present the first systematic analysis of photometric redshifts (photo-z) estimated from the Rubin Observatory Data Preview 1 (DP1) data taken with the Legacy Survey of Space and Time (LSST) Commissioning Camera. Employing the Redshift Assessment Infrast ... Full text CiteSearch for Diffuse Supernova Neutrino Background with 956.2 Days of Super-Kamiokande Gadolinium Dataset
Journal article Astrophysical Journal · July 1, 2026 We report the search result for the Diffuse Supernova Neutrino Background (DSNB) in neutrino energies beyond 9.3 MeV in the gadolinium-loaded Super-Kamiokande (SK) detector with a 22,500 × 956.2 m3 day exposure. Starting in the summer of 2020, S ... Full text CiteThe Vera C. Rubin Observatory Data Preview 1
Journal article Astronomical Journal · June 1, 2026 We present Rubin Data Preview 1 (DP1), the first data from the National Science Foundation–Department of Energy Vera C. Rubin Observatory, comprising raw and calibrated single-epoch images, coadds, difference images, detection catalogs, and ancillary data ... Full text CiteRecent Grants
Research in High Energy Physics at Duke University
ResearchPrincipal Investigator · Awarded by Department of Energy · 2013 - 2029Support During Dean's Leave for Christopher Walter
ResearchPrincipal Investigator · Awarded by SLAC National Accelerator Laboratory · 2024 - 2024SLAC Sabbatical
ResearchPrincipal Investigator · Awarded by Stanford University · 2022 - 2022View All Grants
Education
California Institute of Technology ·
1997
Ph.D.
California Institute of Technology ·
1991
M.S.
University of California, Santa Cruz ·
1989
B.A.