
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
-
Fudan University
-
The Pioneer Anomaly: Known and Unknown Unknowns
Carleton University -
Modeling the evaporation of mini black holes
University of Sheffield -
Cross-Correlation Methods in Continuous Gravitational-Wave Searches
Rochester Institute of Technology -
Cauchy horizon (in)stability in spherically symmetric self-similar gravitational collapse.
Dublin City University -
Gravitational wave phenomenology for LIGO, LISA and co from effective field theories
Carnegie Mellon University -
Local and Global Properties of Green Functions in Black Hole Space-times
University College Dublin -
High-accuracy modeling of extreme mass ratio inspirals with effective field theory
California Institute of Technology -
On the instability of general relativistic wormholes
Universidad Michoacana de San Nicolas de Hidalgo -
The Double Pulsar: testing GR in strong regime
Purdue University -
Strong Gravity
317 talksCollection NumberS020