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Gordon Ogilvie is a Professor of Mathematical Astrophysics at the Department of Applied Mathematics and Theoretical Physics, University of Cambridge. His research primarily focuses on the dynamics of astrophysical disks, which includes materials orbiting a central mass. He investigates a variety of topics such as planetary rings of Saturn, dusty gas disks from which planets form around young stars, and plasma accretion disks surrounding compact stars like black holes. His work delves into the fundamental dynamical processes that lead to sustained nonlinear behavior in angular momentum transport, highlighting hydrodynamic and magnetohydrodynamic instabilities. He explores dynamics in warped and eccentric disks, and the interaction of tidal forces in planetary systems, especially those involving extrasolar planets. Ogilvie has authored numerous influential papers in his field and continues to contribute to our understanding of celestial mechanics and astrophysical fluid dynamics.
Department of Applied Mathematics and Theoretical Physics, University of Cambridge • Cambridge, England
Leading research in mathematical astrophysics, focusing on the dynamics of astrophysical discs.
Department of Applied Mathematics and Theoretical Physics, University of Cambridge • Cambridge, England
Conducted advanced research and taught courses in mathematical astrophysics.
Department of Applied Mathematics and Theoretical Physics, University of Cambridge • Cambridge, England
Delivered lectures and supervised research in applied mathematics.
Institute of Astronomy, University of Cambridge • Cambridge, England
Conducted independent research while mentoring students in astrophysics.
Max-Planck-Institut für Astrophysik • Garching, Germany
Engaged in postdoctoral research in astrophysics.
Space Telescope Science Institute • Baltimore, USA
Worked on projects involving space observations and astrophysical theories.
Standard postgraduate requirements for Department of Politics and International Studies (POLIS) and related humanities departments.