Abstract
The Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation balloon/satellite mission utilizing a Liquid Argon Time Projection Chamber (LArTPC) detector to measure both MeV gamma rays and antinuclei produced by dark matter annihilation or decay. The GRAMS can identify antihelium-3 events based on the measurements of X-rays and charged pions from the decay of the exotic atoms, Time of Flight (TOF), energy deposition, and stopping range. This paper shows the antihelium-3 sensitivity estimation using a GEANT4 Monte Carlo simulation. For the proposed long-duration balloon (LDB) flight program (35 days x 3 flights) and future satellite mission (2-year observation/10-year observation), the sensitivities become 1.47 × 10−7 [m2 s sr GeV/n]−1 and 1.55 × 10−9 [m2 s sr GeV/n]−1/3.10 x 10-10 [m2 s sr GeV/n]−1, respectively. The results indicate that GRAMS can extensively investigate various dark matter models through the antihelium-3 measurements.
