Description
New observational programs and techniques are opening a window to the first galaxies in the universe and bringing surprises along the way. In this workshop, we'll explore how dark matter phenomenology may have impacted the first stars and galaxies, focusing on how improved modeling and simulations can allow us to use new and upcoming high-redshift data to gain insight into dark matter's fundamental nature.
Sponsored in part by:
Displaying 1 - 12 of 26
Format results
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Opening Remarks
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Perimeter Institute for Theoretical Physics
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Queen's University
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Dark and visible structures with dissipative dark matter
Pennsylvania State University -
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Formation of Dark Compact Objects in an Early Matter Dominated Era
Queen's University -
The First Stars in the Universe as Dark Matter Laboratories
Colgate University -
Probing Atomic Dark Matter using Simulated Galactic Subhalo Populations
University of Toronto -
Dark matter at high redshifts with JWST
The University of Texas at Austin -
(Dark) Baryogenesis through Asymmetric Reheating in the Mirror Twin Higgs.
University of Toronto -
Panel Discussion: Theory motivations - why are we here?
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York University
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Massachusetts Institute of Technology
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University of Toronto
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Supermassive black hole seeds from sub-keV dark matter
Queen's University -
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Forming the first stars amidst decaying and annihilating dark matter
Massachusetts Institute of Technology (MIT)