# An Indirect Dark Matter Search Using Cosmic-Ray Antiparticles with GAPS

**Authors:** Alexander Lowell, Tsuguo Aramaki, Ralph Bird, Mirko Boezio, Steven, Boggs, Rachel Carr, William Craig, Philip von Doetinchem, Lorenzo Fabris,, Hideyuki Fuke, Florian Gahbauer, Cory Gerrity, Charles Hailey, Chihiro Kato,, Akiko Kawachi, Masayoshi Kozai, Isaac Mognet, Kazuoki Munakata, Shun Okazaki,, Rene Ong, Guiseppe Osteria, Kerstin Perez, Sean Quinn, Valerio Re, Field, Rogers, Jamie Ryan, Nathan Saffold, Yuki Shimizu, Achim Stoessl, Atsumasa, Yoshida, Tetsuya Yoshida, Gianluigi Zampa, Jeffrey Zweerink

arXiv: 1812.04800 · 2018-12-13

## TL;DR

GAPS is a balloon-borne experiment designed to detect cosmic-ray antiparticles like antideuterons and antiprotons at low energies, aiming to identify signals of dark matter interactions beyond current methods.

## Contribution

This paper introduces the GAPS detector's design, its innovative detection technique using exotic atom formation, and its potential to constrain dark matter models through cosmic-ray antiparticle measurements.

## Key findings

- GAPS will measure the cosmic antideuteron flux below 0.25 GeV/n.
- GAPS will detect around 1000 antiprotons in a new energy range.
- The experiment will validate a novel antiparticle detection method.

## Abstract

Experiments aiming to directly detect dark matter (DM) particles have yet to make robust detections, thus underscoring the need for complementary approaches such as searches for new particles at colliders, and indirect DM searches in cosmic-ray spectra. Low energy (< 0.25 GeV/n) cosmic-ray antiparticles such as antideuterons are strong candidates for probing DM models, as the yield of these particles from DM processes can exceed the astrophysical background by more than two orders of magnitude. The General Antiparticle Spectrometer (GAPS), a balloon borne cosmic-ray detector, will perform an ultra-low background measurement of the cosmic antideuteron flux in the regime < 0.25 GeV/n, which will constrain a wide range of DM models. GAPS will also detect approximately 1000 antiprotons in an unexplored energy range throughout one long duration balloon (LDB) flight, which will constrain < 10 GeV DM models and validate the GAPS detection technique. Unlike magnetic spectrometers, GAPS relies on the formation of an exotic atom within the tracker in order to identify antiparticles. The GAPS tracker consists of ten layers of lithium-drifted silicon detectors which record dE/dx deposits from primary and nuclear annihilation product tracks, as well as measure the energy of the exotic atom deexcitation X-rays. A two-layer, plastic scintillator time of flight (TOF) system surrounds the tracker and measures the particle velocity, dE/dx deposits, and provides a fast trigger to the tracker. The nuclear annihilation product multiplicity, deexcitation X-ray energies, TOF, and stopping depth are all used together to discern between antiparticle species. This presentation provided an overview of the GAPS experiment, an update on the construction of the tracker and TOF systems, and a summary of the expected performance of GAPS in light of the upcoming LDB flight from McMurdo Station, Antarctica in 2020.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1812.04800/full.md

## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1812.04800/full.md

## References

6 references — full list in the complete paper: https://tomesphere.com/paper/1812.04800/full.md

---
Source: https://tomesphere.com/paper/1812.04800