Cosmologists at Perimeter Institute seek to help pin down the constituents and history of our universe, and the rules governing its origin and evolution. Many of the most interesting clues about physics beyond the standard model (e.g., dark matter, dark energy, the matter/anti-matter asymmetry, and the spectrum of primordial density perturbations], come from cosmological observations, and cosmological observations are often the best way to test or constrain a proposed modification of the laws of nature, since such observations can probe length scales, time scales, and energy scales that are beyond the reach of terrestrial laboratories.
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Format results
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Hanyu Zhang, Jessie Muir, Kazuya Koyama, Martin Kunz
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Testing screened modified gravity models
University of Portsmouth -
Non-linear dark energy simulations
University of Geneva -
Beyond Horndeski theories
Université Paris Cité -
Gravitational wave generation in effective field theories of dark energy
SISSA International School for Advanced Studies -
Town Hall - Modified gravity strong field regime
Enrico Barausse, Laura Bernard, Maxence Corman, Suvendu Giri -
Black hole binaries in Einstein-scalar-Gauss-Bonnet gravity and their effective-one-body description
Max Planck Institute for Gravitational Physics -
Nonlinear dynamics of compact object mergers in Einstein-scalar-Gauss-Bonnet gravity
Max Planck Institute for Gravitational Physics (Albert Einstein Institute) -
Scalarized black holes - from equilibrium models to nonlinear dynamics
University of Tübingen -
Do Neutron stars k-mouflage?
Max Planck Institute for Gravitational Physics -
Hi-COLA: Horndeski Goes Non-linear
University of Portsmouth -
Black holes in Horndeski theories
IJCLAB CNRS