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Fred Rasio's research spans a wide range of topics in theoretical astrophysics, including exoplanets and planet formation, dynamics of dense stellar systems such as globular clusters and galactic nuclei, and hydrodynamic stellar interactions, which encompass stellar collisions, mergers, binary coalescence, and common envelope evolution. He has made significant contributions to the field of relativistic astrophysics, studying neutron stars, black holes, gravitational waves, and radio pulsars. His recent work has focused on the dynamics of tightly packed planetary systems and the identification of gravitational wave sources for laser-interferometer detectors like LIGO and LISA, as well as the formation of massive black holes through stellar dynamical processes.
Standard PhD requirements for TGS departments including Chemistry, Physics, and Sociology.