معرفی
Hannah Poole is a Researcher in the Department of Physics and Astronomy at the University of Rochester, School of Arts & Sciences. Her research focuses on high-energy density physics, plasma diagnostics, and the study of materials under extreme conditions. She employs advanced techniques such as X-ray and optical Thomson scattering to investigate plasma turbulence, magnetic field dynamics, and heat transport in astrophysical and laboratory settings.
Her work addresses fundamental questions in astrophysical plasma behavior, including dynamo mechanisms in turbulent environments and the thermal properties of planetary interiors. She collaborates on laser-driven experiments and computational simulations using platforms like the OMEGA Laser Facility and FLASH code.
Key contributions include studies on shock-compressed silicon, methane under planetary conditions, and the suppression of heat conduction in magnetized turbulent plasmas. Her research bridges laboratory experiments with astrophysical phenomena, advancing our understanding of extreme matter states and plasma dynamics.
