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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Force-Free Electrodynamics around Extreme Kerr Black Holes
Maria J. Rodriguez Utah State University
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A mechanism for vortex annihilation in two dimensional superfluid turbulence
Andrew Lucas University of Colorado Boulder
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Gravity waves from Kerr/CFT
Achilleas Porfyriadis Harvard University
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Black holes without Lorentz symmetry
Thomas Sotiriou University of Nottingham
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Geometric inequalities for black holes
Sergio Dain Universidad Nacional de Córdoba
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The characteristic structure of the Weyl curvature tensor and its utilization
Fan Zhang Beijing Normal University
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Compact objects as dark-matter probes
Paolo Pani Instituto Superior Tecnico - Departamento de Física
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Sequestering Lorentz violation in the Lifshitz sector
Maxim Pospelov University of Minnesota
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