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Proton Rejection in the Measurements of High Energy Electrons and Positrons Detected from Lateral Aperture of the GAMMA-400 Gamma-Ray Telescope

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The space observatory GAMMA-400 is processed currently in accordance with the Federal Space Program of the Russian Federation for 2016–2025. The observatory includes a gamma-ray telescope for experimental studies of gamma rays in the energy range from ~20 MeV to ~1 TeV with high angular and energy resolution, as well as for research of electrons + positrons at energies above 100 GeV in both the main (top-down), and lateral apertures. At present time, there are experimental indications concerning the possibility of existing of spectrum break in electrons + positrons intensities about TeV energies. This point stimulates several speculations to explain such phenomena. In this paper we examined capabilities of GAMMA-400 telescope to explore this problem. The methods for electron detection in the energy range from 100 GeV up to 10 TeV from the lateral aperture of a gamma-ray telescope are presented. Also, the results of calculation for proton rejection factor and for electron acceptance are revealed.

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Funding

The work was supported by the RF Ministry of Science and Higher Education, project “Fundamental and Applied Research of Cosmic Rays” no. FSWU-2023-0068.

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Correspondence to A. A. Leonov.

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Leonov, A.A., Galper, A.M., Topchiev, N.P. et al. Proton Rejection in the Measurements of High Energy Electrons and Positrons Detected from Lateral Aperture of the GAMMA-400 Gamma-Ray Telescope. Bull. Russ. Acad. Sci. Phys. 87, 1027–1031 (2023). https://doi.org/10.3103/S1062873823702325

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  • DOI: https://doi.org/10.3103/S1062873823702325

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