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Loren E Held is a theoretical astrophysicist at the University of Cambridge, affiliated with the Department of Applied Mathematics and Theoretical Physics. His research primarily revolves around astrophysical fluid dynamics, focusing on applied accretion disks. Presently, he is investigating the dynamics of distorted disks, including warped, eccentric, and tidally distorted configurations. Previously, he held a postdoctoral position at the Max Planck Institute for Gravitational Physics, which focused on the computational aspects of relativistic astrophysics and explored how disks form during binary neutron star mergers. His PhD research delved into the interaction of convection disks and magnetorotational instability (MRI), with applications to phenomena such as Dwarf Novae. He has a long-standing interest in turbulence, including homogeneous isotropic turbulence and its implications in astrophysical contexts. Throughout his career, he has contributed to several publications, addressing various aspects of astrophysical fluid dynamics and magnetohydrodynamics.
Department of Applied Mathematics and Theoretical Physics, University of Cambridge • Cambridge, UK
Conducting research in astrophysical fluid dynamics and applied accretion disks.
Max Planck Institute for Gravitational Physics •
Focused on computational relativistic astrophysics and dynamics of disks formed in binary neutron star mergers.
Standard postgraduate requirements for Department of Politics and International Studies (POLIS) and related humanities departments.