Angular emission patterns of remnant black holes -- Towards a more complete temporal-spatial fitting with high precision
Xiang Li California Institute of Technology (Caltech)
Strong Gravity research at Perimeter Institute is devoted to understanding both the theoretical and observational aspects of systems in which gravity is very strong (i.e., spacetime is highly curved or dynamical],. On one hand, this means studying extreme astrophysical systems, like black holes and neutron stars, as well as making and testing predictions for existing and forthcoming gravitational wave detectors, electromagnetic telescopes, and particle astrophysics experiments. On the other hand, it also includes a range of non-astrophysical topics, such as the instabilities of higher-dimensional black holes or the dynamics of strongly-coupled quantum field theories (via holography). The goal of strong gravity researcher is to test the validity of Einstein's theory of gravity, constrain proposed alternatives, understand the most extreme astrophysical systems, and investigate the ways in which highly curved or dynamical spacetimes are linked with a range of other problems in fundamental physics.
Xiang Li California Institute of Technology (Caltech)
Sebastian Volkel SISSA International School for Advanced Studies
Anna Ijjas Max Planck Institute for Gravitational Physics - Albert Einstein Institute (AEI)
Kyriakos Destounis University of Tübingen
Bruce Edelman University of Oregon
Beatriz Elizaga Waseda University
Aaron Held Friedrich Schiller University Jena
Sarah Gossan Canadian Institute for Theoretical Astrophysics (CITA)
Mohammed Khalil Perimeter Institute for Theoretical Physics
Luciano Combi Perimeter Institute for Theoretical Physics
Andrea Biscoveanu Massachusetts Institute of Technology (MIT)