Cosmic antihelium-3 nuclei sensitivity of the GAPS experiment
arXiv:2012.05834 · doi:10.1016/j.astropartphys.2021.102580
Abstract
The General Antiparticle Spectrometer (GAPS) is an Antarctic balloon experiment designed for low-energy (0.10.3 GeV/) cosmic antinuclei as signatures of dark matter annihilation or decay. GAPS is optimized to detect low-energy antideuterons, as well as to provide unprecedented sensitivity to low-energy antiprotons and antihelium nuclei. The novel GAPS antiparticle detection technique, based on the formation, decay, and annihilation of exotic atoms, provides greater identification power for these low-energy antinuclei than previous magnetic spectrometer experiments. This work reports the sensitivity of GAPS to detect antihelium-3 nuclei, based on full instrument simulation, event reconstruction, and realistic atmospheric influence simulations. The report of antihelium nuclei candidate events by AMS-02 has generated considerable interest in antihelium nuclei as probes of dark matter and other beyond the Standard Model theories. GAPS is in a unique position to detect or set upper limits on the cosmic antihelium nuclei flux in an energy range that is essentially free of astrophysical background. In three 35-day long-duration balloon flights, GAPS will be sensitive to an antihelium flux on the level of (95% confidence level) in the energy range of 0.110.3 GeV/, opening a new window on rare cosmic physics.
Accepted for publication at Astroparticle Physics, 13 pages, 5 figures
References in corpus (4)
- Antideuteron fluxes from dark matter annihilation in diffusion models
- Scrutinizing the evidence for dark matter in cosmic-ray antiprotons
- Large-scale Simulations of Antihelium Production in Cosmic-ray Interactions
- Passivation of Si(Li) detectors operated above cryogenic temperatures for space-based applications
Cited by in corpus (6)
- The ALICE experiment: a journey through QCD
- Reevaluation of the cosmic antideuteron flux from cosmic-ray interactions and from exotic sources
- Sensitivity of the GAPS Experiment to Low-energy Cosmic-ray Antiprotons
- The antinucleus annihilation reconstruction algorithm of the GAPS experiment
- Large-scale detector testing for the GAPS Si(Li) Tracker
- Antihelium-3 Sensitivity for the GRAMS Experiment