Third-generation ground-based gravitational-wave detectors such as the Einstein Telescope and the space mission LISA will observe compact binary systems with unprecedented sensitivity. In order to extract information on fundamental physics and on the nature of the sources with these instrument, it is necessary to improve current models of the gravitational-wave emission from compact binaries.
This will be done through the use of analytic approximations, including post-Newtonian theory, black-hole perturbation theory, and effective field theory.
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This is NTNU At NTNU, creating knowledge for a better world is the vision that unites our 7 400 employees and 42 000 students. We are looking for dedicated employees to join us. ... (Video unable ...
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