School of Natural Sciences

Scholars from the School of Natural Sciences are leading investigations into the sources of gravitational wave signals, the unexpectedly high frequency of detections, and—extending beyond these direct questions—establishing innovative and unexpected connections between gravitational wave research and particle collider physics. These contributions are redefining our understanding of the field.

The work of plasma fusion physicists may seem completely divorced from the realm of theoretical astrophysics, but, as Chris Hamilton, John N. Bahcall Fellow in the School of Natural Sciences, explains, the mathematical methods developed to exploit the power of the electrons, ions, and magnetic fields in fusion plasmas are precisely the same as those needed to describe the dynamics of stars, spiral arms, and dark matter in galaxies like the Milky Way.