We’re accepting applications from prospective PhD students. The deadline is Dec 31, 2019 for positions starting in the Fall of 2020.
Here below is my project description:
Astrophysics and phenomenology of gravitational-wave sources with LIGO and LISA
This project concentrates on developing theoretical and astrophysical prediction s of gravitational-wave sources. The first observations of gravitational waves by LIGO have ushered us into the golden age of gravitational-wave discoveries. Thousands of new events are expected to be observed in the next few years as detectors reach their design sensitivities. Such large catalogs of gravitational-wave observations will open new, unprecedented opportunities in terms of both fundamental physics and astrophysics. Crucially, they will need to be faced with increasingly accurate predictions. First, among large catalogs, there will be “golden” events. We expect systems that, because of their properties, are particularly interesting to carry out some specific measurements (perhaps because of their favorable orientations, or because they are very massive, or very rapidly rotating, etc). Second, large catalogs need to be exploited with powerful statistical techniques. In the long run, future facilities like LISA will deliver new kinds of sources providing access to a whole new set of phenomena in both astrophysics and fundamental physics. New theoretical tools and techniques need to be developed (and immediately applied!) to maximize the scientific payoff of current and future gravitational-wave observatories.