The High Energy cosmic-Radiation Detector (HERD) Trigger System | |
Velasco, M. A.60; Bao, T.59; Berti, E.58; Bonvicini, V.57; Casaus, J.60; Giovacchini, F.60; Liu, X.59; Marco, R.60; Marín, J.60; Martínez, G.60 | |
2022-03-18 | |
会议日期 | 2021-07-12 |
会议地点 | Virtual, Berlin, Germany |
卷号 | 395 |
英文摘要 | The High Energy cosmic-Radiation Detection (HERD) facility is a next generation spaceborne detector to be installed onboard the Chinese Space Station for about 10 years. HERD will address major problems in fundamental physics and astrophysics, providing precise measurements of charged-cosmic rays up to PeV energies, performing indirect searches for dark matter in the electron spectrum up to few tens of TeV and monitoring the gamma-ray skymap for surveys and transient searches. HERD is composed of a 3D imaging calorimeter (CALO) surrounded by a scintillating fiber tracker (FIT), a plastic scintillator detector (PSD) and a silicon charge detector (SCD). In addition, a transition radiation detector (TRD) is placed on a lateral side to provide accurate energy calibration. Based on this innovative design, the effective geometric factor of HERD will be one order of magnitud larger than that of current space-based detectors. The HERD trigger strategy is designed to accomplish the scientific goals of the mission, and is based on trigger definitions that rely on the energy deposited in CALO and the PSD. The trigger performances are evaluated using a detailed Monte Carlo simulation that includes the latest HERD geometry. In addition, alternative trigger definitions based on the event topology can be established thanks to the photodiode readout of CALO crystals. The feasibility of these topological triggers is also investigated and presented. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0) |
产权排序 | 第19完成单位 |
会议录 | Proceedings of Science |
资助机构 | N/A |
会议录出版者 | Sissa Medialab Srl |
文献子类 | Conference article (CA) |
学科主题 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 核科学技术 |
语种 | 英语 |
内容类型 | 会议论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25687] |
专题 | 中国科学院云南天文台 |
作者单位 | 1.INFN sez. Catania, Catania, Italy 2.Dipartimento di Fisica e Chimica "E. Segrè", Universitá degli Studi di Palermo, Palermo, Italy; 3.Universitá di Bologna, Bologna, 40126, Italy; 4.INFN Sezione di Bologna, Bologna, 40126, Italy; 5.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy; 6.Universitá degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 7.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 8.Universitá degli Studi di Trieste, Italy; 9.Universitá degli Studi di Napoli Federico II, Napoli, Italy; 10.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy; |
推荐引用方式 GB/T 7714 | Velasco, M. A.,Bao, T.,Berti, E.,et al. The High Energy cosmic-Radiation Detector (HERD) Trigger System[C]. 见:. Virtual, Berlin, Germany. 2021-07-12. |
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