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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University of Tokyo
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David Defeats Goliath: How Ultralight Fields Affect The Dynamics of Massive Black Holes
Instituto Superior Tecnico - Departamento de Física -
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Spinning black-hole binaries as gravitational and cosmological probes
SISSA International School for Advanced Studies -
Fundamental Physics with Optically Levitated Dielectric Objects
Perimeter Institute for Theoretical Physics -
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Canonical gravity using unconstrained null initial data
Universidad de la Republica Uruguay -
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Exploiting the Strong Gravitational Fields of Neutron Stars to Measure their Properties
University of Arizona -
Gamma Rays at 130 GeV and How They Might Come from Dark Matter
University of Winnipeg -
12/13 PSI - Gravitational Physics Review Lecture 15
King's College London