The GAPS Experiment to Search for Dark Matter using Low-energy Antimatter
R.A. Ong, T. Aramaki, R. Bird, M. Boezio, S.E. Boggs, R. Carr, W.W., Craig, P. von Doetinchem, L. Fabris, F. Gahbauer, C. Gerrity, H. Fuke, C.J., Hailey, C. Kato, A. Kawachi, M. Kozai, S.I. Mognet, K. Munakata, S. Okazaki,, G. Osteria, K. Perez, V. Re, F. Rogers, N. Saffold

TL;DR
The GAPS experiment aims to detect low-energy cosmic ray antimatter, especially antideuterons, using an exotic atom technique to search for dark matter signals with high sensitivity and low background.
Contribution
This paper introduces the GAPS experiment's novel detection method and its potential to explore dark matter models through low-energy antimatter measurements.
Findings
Prototype flown successfully in 2012
GAPS will provide new constraints on dark matter below 10 GeV
Designed for long-duration balloon flights in Antarctica
Abstract
The GAPS experiment is designed to carry out a sensitive dark matter search by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will provide a new avenue to access a wide range of dark matter models and masses that is complementary to direct detection techniques, collider experiments and other indirect detection techniques. Well-motivated theories beyond the Standard Model contain viable dark matter candidates which could lead to a detectable signal of antideuterons resulting from the annihilation or decay of dark matter particles. The dark matter contribution to the antideuteron flux is believed to be especially large at low energies (E < 1 GeV), where the predicted flux from conventional astrophysical sources (i.e. from secondary interactions of cosmic rays) is very low. The GAPS low-energy antiproton search will provide stringent constraints on less than 10 GeV…
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