YNAO OpenIR
Design and expected performances of the large acceptance calorimeter for the HERD space mission
Pacini, Lorenzo1; Adriani, Oscar1,2; Bai, Yong-Lin2; Bao, Tian-Wei2; Berti, Eugenio1,2; Bottai, Sergio1; Cao, Wei-Wei2; Casaus, Jorge6; Cui, Xing-Zhu2; D’Alessandro, Raffaello1,2; Formato, Valerio7; Gao, Jia-Rui2; Li, Ran2; Liu, Xin2; Lorusso, Leonarda3; Lyu, Lin-Wei2; Marin, Jesus6; Martinez, Gustavo6; Pizzolotto, Cecilia8; Qin, Jun-Jun2; Quan, Zheng2; Shi, Da-Lian2; Starodubtsev, Oleksandr1; Tang, Zhi-Cheng2; Tiberio, Alessio1,2; Vagelli, Valerio4,5; Velasco, Miguel Angel6; Wang, Bo2; Wang, Rui-Jie2; Wang, Zhi-Gang2; Xu, Ming2; Yang, Yang2; Zhang, Li2; Zheng, Jin-Kun2; Adriani, O.34; Alemanno, F.35,36; Aloisio, R.35,36; Altomare, C.31; Ambrosi, G.43; An, Q.18; Antonelli, M.53; Azzarello, P.46; Bai, L.16; Bai, Y. L.11; Bao, T. W.9; Barbanera, M.43; Barbato, F. C.35,36; Bernardini, P.39; Berti, E.34; Bertucci, B.44; Bi, X. J.9; Bigongiari, G.45; Bongi, M.34; Bonvicini, V.53; Bordas, P.48; Bosch-Ramon, V.48; Bottai, S.33; Brogi, P.45; Cadoux, F.46; Campana, D.40; Cao, W. W.11; Cao, Z.9; Casaus, J.47; Catanzani, E.44; Cattaneo, P. W.42; Chang, J.17,21; Chang, Y. H.29; Chen, G. M.9; Chen, Y.23; Cianetti, F.44; Comerma, A.48,49; Cortis, D.37; Cui, X. H.21; Cui, X. Z.9; Dai, C.13; Dai, Z. G.23; D’Alessandro, R.34; De Gaetanoe, S.32; De Mitri, I.35,36; de Palma, F.39; Di Felice, V.58; Di Giovanni, A.35,36; Di Santo, M.35,36; Di Venere, L.32; Dong, J. N.14,15; Dong, Y. W.9; Donvito, G.31; Duranti, M.43; D’Urso, D.57; Evoli, C.35,36; Fang, K.9; Fariña, L.50; Favre, Y.46; Feng, C. Q.18; Feng, H.24; Feng, H. B.13; Feng, Z. K.13; Finetti, N.30; Formato, V.58; Frieden, J. M.52; Fusco, P.32; Gao, J. R.11; Gargano, F.31; Gascon-Fora, D.48; Gasparrini, D.58; Giglietto, N.32; Giovacchini, F.47; Gomez, S.48; Gong, K.9; Gou, Q. B.9; Guida, R.54; Guo, D. Y.9; Guo, J. H.17; Guo, Y. Q.9; He, H. H.9; Hu, H. B.9; Hu, J. Y.9,10; Hu, P.9,10; Hu, Y. M.17; Huang, G. S.18; Huang, J.9; Huang, W. H.14,15; Huang, X. T.14,15; Huang, Y. B.13; Huang, Y. F.23; Ionica, M.43; Jouvin, L.50; Kotenko, A.46; La Marra, D.46; Li, M. J.14,15; Li, Q. Y.14,15; Li, R.11; Li, S. L.9,10; Li, T.14,15; Li, X.17; Li, Z.25; Li, Z. H.9,10; Liang, E. W.13; Liang, M. J.9,10; Liao, C. L.16; Licciulli, F.31; Lin, S. J.9; Liu, D.14,15; Liu, H. B.13; Liu, H.16; Liu, J. B.18; Liu, S. B.18; Liu, X.9,10; Liu, X. W.13; Liu, Y. Q.9; Loparco, F.32; Loporchio, S.31; Lu, X.13; Lyu, J. G.12; Lyu, L. W.11; Maestro, P.45; Mancini, E.43; Manera, R.48; Marin, J.47
Source PublicationProceedings of Science
2022-03-18
Volume395
DOI10.22323/1.395.0066
Contribution Rank第22完成单位
Indexed ByEI
Conference Name37th International Cosmic Ray Conference, ICRC 2021
Conference Date2021-07-12
Conference PlaceVirtual, Berlin, Germany
Abstract

The High Energy cosmic-Radiation Detection (HERD) is a future space experiment which will be installed on the China’s Space Station around 2027. The main goal of the experiment is the measurement of cosmic rays up to energies which are not explored by the instruments currently operating in space, in particular protons with energies up to PeV, nuclei up to hundreds of TeV per nucleon and electrons up to tens of TeV. HERD will consist of silicon charge detectors, anti-coincidence scintillators, scintillating fiber trackers, a transition radiation detector and a calorimeter. The latter is a homogeneous, deep, 3D segmented calorimeter made of about 7500 LYSO cubic crystals: thanks to this innovative design, it will achieve large acceptance, good energy resolution and excellent electron/proton discrimination. In order to increase both energy calibration capabilities and redundancy of the instrument, the LYSO scintillation light will be read-out by two independent systems: the first is made of wave-length shifting fibers coupled with imaged intensified CMOS cameras, and the second one consists of photodiodes with different active areas connected to a custom front-end electronics. Both read-out systems are designed to have a large dynamic range, up to 107, and a low power consumption. The design of the calorimeter is validated by several Monte Carlo simulations and beam test results obtained with detector prototypes. In this paper we describe the anticipated performances of the calorimeter and the current status of the double read-out system, and we discuss the recent developments of both the HERD prototype and the flight model design. © Copyright owned by the author(s).

Funding ProjectN/A
Funding OrganizationN/A
Language英语
Subject Area天文学 ; 天体物理学 ; 高能天体物理学 ; 核科学技术
MOST Discipline Catalogue理学 ; 理学::天文学 ; 工学 ; 工学::核科学与技术
SubtypeConference article (CA)
PublisherSissa Medialab Srl
URL查看原文
EI Accession Number20225113275650
EI KeywordsCalorimeters
EI Classification Number656.1 Space Flight - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 723.4 Artificial Intelligence - 922.2 Mathematical Statistics - 944.5 Temperature Measuring Instruments - 944.7 Radiation Measuring Instruments
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/25684
Collection中国科学院云南天文台
Affiliation1.INFN sezione di Firenze, Sesto Fiorentino, Florence, I-50019, Italy;
2.Department of Physics and Astronomy, University of Florence, Sesto Fiorentino, Florence, I-50019, Italy;
3.Dipartimento di Matematica, Università degli Studi di Roma
4.Agenzia Spaziale Italiana (ASI), Roma, I-00133, Italy;
5.Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Perugia, Perugia, I-06123, Italy;
6.Centro de Investigaciones Energéticas, Medioambientales y Tecnoló gicas (CIEMAT), Madrid, E-28040, Spain;
7.INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy;
8.INFN Sezione di Trieste, Trieste, I-34149, Italy;
9.Key Laboratory of Particle and Astrophysics, Chinese Academy of Sciences, Beijing, China;
10.University of Chinese Academy of Sciences, Beijing, China;
11.Xi’an Institute of Optics and Precision Mechanics of CAS, Xi’an, China;
12.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China;
13.School of Physical Science and Technology, Guangxi University, Nanning, China;
14.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, China;
15.Key Laboratory of Particle Physics and Particle Irradiation, Ministry of Education, China;
16.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, China;
17.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;
18.Department of Modern Physics, University of Science and Technology of China, Hefei, China;
19.Department of Astronomy, Yunan University, Kunming, China;
20.North Night Vision Technology co. ltd., Kunming, China;
21.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
22.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, China;
23.School of Astronomy and Space Science, Nanjing University, Nanjing, China;
24.Department of Astronomy, Tsinghua University, Beijing, China;
25.Department of Astronomy, Peking University, Beijing, China;
26.Institute of Astrophysics, Central China Normal University, Wuhan, China;
27.Department of Physics, China University of Geosciences, Wuhan, China;
28.The University of Hong Kong, Hong Kong;
29.Institute of Physics, Academia Sinica, Taipei, Taiwan;
30.Universitá dell’Aquila, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
31.Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy;
32.Dipartimento di Fisica
33.Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
34.Universitá di Firenze, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
35.Gran Sasso Science Institute, L’Aquila, Italy;
36.INFN Laboratori Nazionali del Gran Sasso, Assergi, L’Aquila, Italy;
37.INFN Laboratori Nazionali del Gran Sasso, L’Aquila, Italy;
38.Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
39.Universitá del Salento, Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
40.Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy;
41.Universitá di Napoli
42.Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, Pavia, Italy;
43.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
44.Universitá degli Studi di Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
45.Universitá di Siena, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy;
46.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève, Switzerland;
47.Department of Astronomy, University of Geneva, Geneva, Switzerland;
48.Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain;
49.Universitat Pompeu Fabra (UPF), Barcelona, Spain;
50.Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona, E-08193, Spain;
51.KTH Royal Institute of Technology, Stockholm, Sweden;
52.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland;
53.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy;
54.Universitá degli Studi di Napoli Federico II, Napoli, Italy;
55.Universitá degli Studi di Trieste, Italy;
56.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
57.Universitá degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
58.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy;
59.INFN Sezione di Bologna, Bologna, 40126, Italy;
60.Universitá di Bologna, Bologna, 40126, Italy;
61.Dipartimento di Fisica e Chimica
62.INFN sez. Catania, Catania, Italy
Recommended Citation
GB/T 7714
Pacini, Lorenzo,Adriani, Oscar,Bai, Yong-Lin,et al. Design and expected performances of the large acceptance calorimeter for the HERD space mission[C]:Sissa Medialab Srl,2022.
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