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25–28 Mar 2020
UCLA
US/Pacific timezone

In Search of Cosmic-Ray Antinuclei from Dark Matter with the GAPS Experiment

27 Mar 2020, 08:00
15m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095
Talk Indirect dark matter detection Session 11

Speaker

Kerstin Perez (MIT)

Description

The GAPS Antarctic balloon payload, scheduled for its initial flight in late 2021, is the first experiment optimized specifically for low-energy cosmic antinuclei signatures of dark matter. Low-energy antideuterons provide a “smoking gun" signature of dark matter annihilation or decay, essentially free of astrophysical background. Studies in recent years have emphasized that models for cosmic-ray antideuterons must be considered together with the abundant cosmic antiprotons and any potential observation of antihelium. Together, these signatures offer a potential breakthrough in unexplored dark matter parameter space, providing complementary coverage with direct detection, collider, and other indirect searches. In this contribution, I will detail the novel GAPS detection technique, based on exotic atom capture and decay; the status of the GAPS instrument construction; and the potential of upcoming measurements to clarify ongoing open issues.

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