Institutional Repository System Of Yunnan Observatories, CAS
| The Plastic Scintillator Detector of the HERD space mission | |
| Kyratzis, D.1,2; Alemanno, F.1,2; Altomare, C.3,4; Barbato, F. C.1,2; Bernardini, P.5,6; Cattaneo, P. W.7; De Mitri, I.1,2; de Palma, F.5,6; Di Venere, L.3,4; Di Santo, M.1,2; Fusco, P.3,4; Gargano, F.4; Loparco, F.3,4; Loporchio, S.4; Marsella, G.8; Mazziotta, M. N.4; Pantaleo, F. R.3,4; Parenti, A.1,2; Pillera, R.3,4; Rappoldi, A.7; Raselli, G.7; Rossella, M.7; Serini, D.4; Silveri, L.1,2; Surdo, A.6; Wu, L.1,2; Adriani, O.34; Aloisio, R.35,36; Ambrosi, G.40; An, Q.18; Antonelli, M.51; Azzarello, P.43; Bai, L.16; Bai, Y. L.11; Bao, T. W.9; Barbanera, M.40; Berti, E.34; Bertucci, B.41; Bi, X. J.9; Bigongiari, G.42; Bongi, M.34; Bonvicini, V.51; Bordas, P.46; Bosch-Ramon, V.46; Bottai, S.33; Brogi, P.42; Cadoux, F.43; Campana, D.38; Cao, W. W.11; Cao, Z.9; Casaus, J.45; Catanzani, E.41; Chang, J.17,21; Chang, Y. H.29; Chen, G. M.9; Chen, Y.23; Cianetti, F.41; Comerma, A.46,47; Cortis, D.37; Cui, X. H.21; Cui, X. Z.9; Dai, C.13; Dai, Z. G.23; D'Alessandro, R.34; De Gaetano, S.32; Di Felice, V.56; Di Giovanni, A.35,36; Dong, J. N.14,15; Dong, Y. W.9; Donvito, G.31; Duranti, M.40; D'Urso, D.55; Evoli, C.35,36; Fang, K.9; Fariña, L.48; Favre, Y.43; Feng, C. Q.18; Feng, H.24; Feng, H. B.13; Feng, Z. K.13; Finetti, N.30; Formato, V.56; Frieden, J. M.50; Gao, J. R.11; Gascon-Fora, D.46; Gasparrini, D.56; Giglietto, N.32; Giovacchini, F.45; Gomez, S.46; Gong, K.9; Gou, Q. B.9; Guida, R.52; 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.40; Jouvin, L.48; Kotenko, A.43; La Marra, D.43; 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; Lu, X.13; Lyu, J. G.12; Lyu, L. W.11; Maestro, P.42; Mancini, E.40; Manera, R.46; Marin, J.45; Marrocchesi, P. S.42; Martinez, G.45; Martinez, M.48; Marzullo, D.53; Mauricio, J.46; Mocchiutti, E.51; Morettini, G.41; Mori, N.33; Mussolin, L.41; Oliva, A.57; Orlandi, D.37; Osteria, G.38; Pacini, L.33; Panico, B.38; Papa, S.52; Papini, P.33; Paredes, J. M.46; Pauluzzi, M.41; Pearce, M.49; Peng, W. X.9; Perfetto, F.38; Perrina, C.50; Perrotta, G.52; Pizzolotto, C.51; Qiao, R.9; Qin, J. J.11 | |
| 会议录名称 | Proceedings of Science |
| 2022-03-18 | |
| 卷号 | 395 |
| DOI | 10.22323/1.395.0054 |
| 产权排序 | 第22完成单位 |
| 收录类别 | EI |
| 会议名称 | 37th International Cosmic Ray Conference, ICRC 2021 |
| 会议日期 | 2021-07-12 |
| 会议地点 | Virtual, Berlin, Germany |
| 摘要 | The High Energy cosmic-Radiation (HERD) detector is one of the prominent space-borne instruments to be installed on-board the Chinese Space Station (CSS), around 2027. Primary scientific goals regarding this initiative include: precise measurements of cosmic ray (CR) energy spectra and mass composition, at energies up to the PeV range; contributions to high energy gamma-ray astronomy and transient studies; as well as indirect searches for Dark Matter (DM) particles via their possible annihilation/decay to detectable products. HERD is configured to accept incident particles from both its top and four lateral sides. Owing to its pioneering design, an order of magnitude increase in acceptance is foreseen, with respect to previous and ongoing experiments. The Plastic Scintillator Detector (PSD) constitutes an important sub-detector of HERD, particularly aimed towards anti-coincidence (discriminating incident photons from charged particles), while providing precise charge measurement of incoming cosmic-ray nuclei in a range of Z = 1-26. Main requirements concerning its design, include: high detection efficiency, broad dynamic range and good energy resolution. In order to select the optimal layout, two geometries are currently under investigation: one based on long scintillator bars and the other on square tiles, with both layouts being readout by Silicon Photomultipliers (SiPMs). Ongoing activities and future plans regarding the HERD PSD will be presented in this work. © 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) |
| 资助项目 | N/A |
| 项目资助者 | N/A |
| 语种 | 英语 |
| 学科领域 | 机械工程 ; 仪器仪表技术 ; 天文仪器 |
| 文章类型 | Conference article (CA) |
| 出版者 | Sissa Medialab Srl |
| URL | 查看原文 |
| EI入藏号 | 20225113256982 |
| EI主题词 | Cosmic rays |
| EI分类号 | 656.1 Space Flight - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics - 944.7 Radiation Measuring Instruments |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25677 |
| 专题 | 中国科学院云南天文台 |
| 作者单位 | 1.Gran Sasso Science Institute (GSSI), Via Iacobucci 2, L'Aquila, 67100, Italy; 2.INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, L'Aquila, 67100, Italy; 3.Dipartimento di Fisica 4.INFN, Sezione di Bari, Bari, 70126, Italy; 5.Dipartimento di Matematica e Fisica 6.INFN, Sezione di Lecce, Lecce, 73100, Italy; 7.INFN, Sezione di Pavia, Pavia, 27100, Italy; 8.Dipartimento di Fisica e Chimica 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, 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 Napoli, Napoli, Italy; 39.Universitá di Napoli 40.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 41.Universitá degli Studi di Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 42.Universitá di Siena, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy; 43.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève, Switzerland; 44.Department of Astronomy, University of Geneva, Geneva, Switzerland; 45.Centro de Investigaciones Energéticas Medioambientales y Tecnoló Gicas (CIEMAT), Madrid, E-28040, Spain; 46.Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain; 47.Universitat Pompeu Fabra (UPF), Barcelona, Spain; 48.Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona, E-08193, Spain; 49.KTH Royal Institute of Technology, Stockholm, Sweden; 50.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland; 51.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy; 52.Universitá degli Studi di Napoli Federico II, Napoli, Italy; 53.Universitá degli Studi di Trieste, Italy; 54.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 55.Universitá degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 56.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy; 57.INFN Sezione di Bologna, Bologna, 40126, Italy; 58.Universitá di Bologna, Bologna, 40126, Italy |
| 推荐引用方式 GB/T 7714 | Kyratzis, D.,Alemanno, F.,Altomare, C.,et al. The Plastic Scintillator Detector of the HERD space mission[C]:Sissa Medialab Srl,2022. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| The Plastic Scintill（3339KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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