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Flip Tanedo (UC Riverside)2024-10-18, 9:00 a.m.
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Bryce Cyr (Massachusetts Institute of Technology)2024-10-18, 9:30 a.m.
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Yikun Wang (Caltech)2024-10-18, 10:00 a.m.
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Nassim Bozorgnia (U Alberta)2024-10-18, 11:00 a.m.
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Leo Kim (Queen's University)2024-10-18, 11:30 a.m.Contributed Talks
Dark compact objects can arise naturally in a variety of dark sectors. Clouds of dark matter between a source star and an observer could effectively act as a "lampshade" and dim starlight if the dark sector couples to the Standard Model photon. These dimming effects can be searched for in microlensing surveys, which measure the brightness of stars as a function of time. By considering the...
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Michael A. Fedderke (Perimeter Institute)2024-10-18, 11:50 a.m.Contributed Talks
Primordial black hole (PBH) dark matter (DM) can be probed by "picolensing". Widely spatially separated gamma-ray detectors near Earth would observe parallax of an intervening PBH lens with respect to a cosmologically distant gamma-ray burst (GRB). This parallax can be of order the Einstein angle of the lens, resulting in differential magnification of the source as viewed from the two...
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Michael Shamma (TRIUMF)2024-10-18, 12:10 p.m.
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Simona Murgia (UC Irvine)
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