Gamma-Ray and AntiMatter Survey(GRAMS) experiment
J. Zeng, T. Aramaki, D. Ames, K. Aoyama, S. Arai, S. Arai, J. Asaadi, A. Bamba, N. Cannady, P. Coppi, G. De Nolfo, M. Errando, L. Fabris, T. Fujiwara, Y. Fukazawa, P. Ghosh, K. Hagino, T. Hakamata, N. Hiroshima, M. Ichihashi, Y. Ichinohe, Y. Inoue, K. Ishikawa, K. Ishiwata

TL;DR
GRAMS is a cutting-edge experiment employing a Liquid Argon TPC to measure MeV gamma rays and antiparticles, aiming to fill the MeV gap and enhance multi-messenger astronomy capabilities.
Contribution
It introduces a novel LArTPC-based approach for simultaneous gamma-ray and antiparticle detection, advancing sensitivity in the MeV range.
Findings
Progress towards prototype balloon flight in 2026.
Initial sensitivity calculations for antihelium-3.
Potential to improve MeV gamma-ray measurement accuracy.
Abstract
The Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation experiment using a Liquid Argon Time Projection Chamber (LArTPC) detector to measure MeV gamma rays and antiparticles. MeV gamma-ray observations are important for understanding multi-messenger and time-domain astronomy, enabling exploration of the universe's most potent events, such as supernovae and neutron star mergers. Despite the significance of MeV gamma-rays, GRAMS could also explore the so-called 'MeV gap' region to improve MeV gamma-ray measurement sensitivity that was restricted by the challenge of accurately reconstructing Compton events. Aside from gamma-ray detection, the GRAMS proposed method also serves as an antiparticle spectrometer, targeting the low-energy range of cosmic antinuclei measurements. This work will provide updates on the current status and progress towards the prototype balloon flight with a…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae
