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Colloquium- Matthew Szydagis (University at Albany)- Shining High- *and* Low-Energy Light on Dark Matter: A Multi-Pronged Approach

Photo of Matthew Szydagis with trees in the background
February 22, 2024
2:30PM - 3:30PM
1080 Physics Research Building

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Add to Calendar 2024-02-22 14:30:00 2024-02-22 15:30:00 Colloquium- Matthew Szydagis (University at Albany)- Shining High- *and* Low-Energy Light on Dark Matter: A Multi-Pronged Approach Professor Matthew SzydagisUniversity at AlbanyShining High- *and* Low-Energy Light on Dark Matter: A Multi-Pronged ApproachLocation: 1080 Physics Research BuildingFaculty Host: Chris Hill 1080 Physics Research Building Department of Physics physics@osu.edu America/New_York public

Professor Matthew Szydagis

University at Albany

Shining High- *and* Low-Energy Light on Dark Matter: A Multi-Pronged Approach

Location: 1080 Physics Research Building

Faculty Host: Chris Hill

Photo of Matthew Szydagis with trees in the background

Abstract: The mystery of dark matter is one of the greatest puzzles in modern science. What is 85% of the matter, or 25% of the mass/energy, of the universe made up of? No human knows for certain. Despite mountains of evidence from astrophysics and cosmology, direct laboratory detection eludes physicists. A leading candidate to explain dark matter is the WIMP or Weakly Interacting Massive Particle, a thermal relic left over after the Big Bang. I will be presenting the first search results as well as subsequent analyses from the LZ experiment deployed in South Dakota, one of the flagship US DOE dark matter projects, and currently world leading above 10 GeV in mass-energy in terms of setting limits on the WIMP interaction strength following non-discovery. I will also describe the Noble Element Simulation Technique (NEST) software I created to model signal and background interactions in a detector like LZ. However, dark matter may be lighter than we’ve thought for decades: perhaps 1 GeV in mass or even less. I will thus also present on a different technology unrelated to the liquid xenon used by LZ. The snowball chamber uses the phase transition of supercooled water to detect incoming radiation, and do so on a tabletop, bringing HEP back to its pre-large-accelerator roots. Lastly, tangential accidental discoveries made during the quest for dark matter will be discussed, especially a new type of nuclear reactor inspired by xenon detector calibrations.

Bio: Dr. Matthew Szydagis received his B.A., M.S., and Ph.D. from the University of Chicago in 2005, 2006, and 2010, respectively, then worked as a postdoc at UC Davis. Since 2014, he has been a faculty member at the physics department at the University at Albany. He is an experimental astroparticle physicist, looking for dark matter, and building new types of particle detectors for rare event searches. Matthew has served in numerous leadership positions on the LZ / LUX collaborations and in the APS DPF, and is a former member of LBNE / DUNE and COUPP. He co-invented the snowball chamber with his colleague Prof. Cecilia Levy, a device that detects incoming particles through the phase transition of supercooled water. He was inspired by Star Trek to become a scientist. He has collaboratively published nearly 100 scientific papers, and delivered close to 200 talks both at conferences and for the public.