Research in gravitational physics on extreme-mass-ratio inspirals and sources of gravitational radiation relevant to the LISA space mission. Research effort involves use of black hole perturbation and self-force theory, and post-Newtonian theory, to construct gravitational waveforms from binary inspiral calculations. Some work will be done in cooperation with the international FEW waveform-development collaboration. Position is nominally for two years, but renewal for a second year is subject to the availability of adequate funding and sufficient progress.
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Education Level
No Education Listed
Number of Employees
11-50 employees