
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.
Format results
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Production of Solar Scalars
University of Cambridge -
Probing quantum gravity at all scales
Universität Heidelberg -
Simulating a Quantised Black Hole
King's College London -
Town Hall - Fundamental aspects of Modified gravity
Adam Solomon, Andrew Tolley, Astrid Eichhorn, Sergey Sibiryakov -
Against Horndeski
McMaster University -
Extending EFT of inflation/dark energy to arbitrary background with timelike scalar profile
Yukawa Institute for Theoretical Physics -
Galileon Duality and its Generalizations
Imperial College London -
Post-Newtonian limit of Lorentz-violating scalar-tensor theories
Rikkyo University -
Town Hall - New generation of LSS surveys and modified gravity/dark energy
Hanyu Zhang, Jessie Muir, Kazuya Koyama, Martin Kunz -
Testing screened modified gravity models
University of Portsmouth -
Non-linear dark energy simulations
University of Geneva (UNIGE)