Detection response of the active components of the SciBar Cosmic Ray Telescope at Sierra Negra

Abstract The Scibar Cosmic-Ray Telescope (SciCRT) is the most promising detector of the Sierra Negra Cosmic Rays Observatory (SN-CRO). At this location, being a target and a tracker of secondary cosmic rays, the SciCRT offers a high probability of observing solar energetic particles and lower energy galactic cosmic rays (LEGCR); also, it allows the identification of incoming particles by measuring their energy deposition. In this work we present a Geant4-based simulation of the energy deposited by neutrons, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> -rays, protons, electrons and muons in the optimally running SciCRT components. We also calculated the detection efficiency of the SciCRT at its current state. Our simulation results provide new information about the SciCRT detection response that may be used as a basis to estimate and analyze the energy spectra of primary particles.

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Publication Details

Journal
The European Physical Journal C
Published
2024-09-27
DOI
https://doi.org/10.1140/epjc/s10052-024-13325-0
Primary Topic
Particle Detector Development and Performance
Type
article
Field-Weighted Citation Impact
0.00

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article

Detection response of the active components of the SciBar Cosmic Ray Telescope at Sierra Negra

Takeshi Kawabata, L. X. González, Y. Itow, T. Sako et al.
The European Physical Journal C
Particle Detector Development and Performance
article

Detection response of the active components of the SciBar Cosmic Ray Telescope at Sierra Negra

Takeshi Kawabata, L. X. González, Y. Itow, T. Sako, Jania Newton-Bosch, Y. Hayashi, Kyoko Watanabe, Oscar G. Morales-Olivares, E. Ortiz, Jose F. Valdés Galicia, H. Tsuchiya, R. Taylor, F. Monterde-Andrade, Y. Matsubara, Hiroyuki Takamaru, Maria A. Sergeeva, K. Munakata, M. Kozai, Yuya Nakamura, T. Koi, C. Kato, Y. Masuda, S. Shibata, ANDRES FELIPE CALDERON HURTADO, H. Kojima, A. Oshima, M. Matsumoto
article en

Abstract

Abstract The Scibar Cosmic-Ray Telescope (SciCRT) is the most promising detector of the Sierra Negra Cosmic Rays Observatory (SN-CRO). At this location, being a target and a tracker of secondary cosmic rays, the SciCRT offers a high probability of observing solar energetic particles and lower energy galactic cosmic rays (LEGCR); also, it allows the identification of incoming particles by measuring their energy deposition. In this work we present a Geant4-based simulation of the energy deposited by neutrons, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> -rays, protons, electrons and muons in the optimally running SciCRT components. We also calculated the detection efficiency of the SciCRT at its current state. Our simulation results provide new information about the SciCRT detection response that may be used as a basis to estimate and analyze the energy spectra of primary particles.

The European Physical Journal CVol. 84(9)
Japan Atomic Energy Agency (JP), Shinshu University (JP), Chubu University (JP), Chinese Academy of Sciences (CN), Shinshu University Hospital (JP), Universidad Autónoma de Chiapas (MX), Institute of High Energy Physics (CN), Research Organization of Information and Systems (JP), Universidad Latina de América (MX), National Defense Academy of Japan (JP), Nagoya University (JP), The University of Tokyo (JP), Universidad Nacional Autónoma de México (MX)
Consejo Nacional de Ciencia y Tecnología, Universidad Nacional Autónoma de México
Affordable and clean energy
Openalex Percentile: Top 95%
Particle Detector Development and Performance
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