Double Photodiode Readout System for the Calorimeter of the HERD Experiment: Challenges and New Horizons in Technology for the Direct Detection of High-Energy Cosmic Rays

Author:

Betti Pietro1ORCID,Adriani Oscar1ORCID,Antonelli Matias2ORCID,Bai Yonglin3ORCID,Bai Xiaohong3,Bao Tianwei4,Berti Eugenio5,Bonechi Lorenzo5,Bongi Massimo1ORCID,Bonvicini Valter2,Bottai Sergio5,Cao Weiwei3ORCID,Casaus Jorge6ORCID,Chen Zhen3,Cui Xingzhu4,D’Alessandro Raffaello1ORCID,Detti Sebastiano5,Diaz Carlos6,Dong Yongwei4,Finetti Noemi57ORCID,Formato Valerio8ORCID,Frutos Miguel Angel Velasco6ORCID,Gao Jiarui3,Giovacchini Francesca6,Liang Xiaozhen3,Li Ran3,Liu Xin49ORCID,Lyu Linwei3,Martinez Gustavo6ORCID,Mori Nicola5ORCID,Munoz Jesus Marin6,Pacini Lorenzo5ORCID,Papini Paolo5ORCID,Pizzolotto Cecilia2ORCID,Quan Zheng4,Qin Junjun3,Shi Dalian3,Starodubtsev Oleksandr5,Tang Zhicheng4,Tiberio Alessio1,Vagelli Valerio1011ORCID,Vannuccini Elena5,Wang Bo3,Wang Junjing4,Wang Le12,Wang Ruijie4,Zampa Gianluigi2ORCID,Zampa Nicola2ORCID,Wang Zhigang4,Xu Ming4,Zhang Li4,Zheng Jinkun3

Affiliation:

1. Dipartimento di Fisica e Astronomia, Università degli Studi di Firenze and INFN Firenze, Via Sansone 1, 50019 Sesto Fiorentino, Italy

2. INFN Trieste, via Valerio 2, 34127 Trieste, Italy

3. Xi’an Institute of Optics and Precision Mechanics of CAS, Xi’an 710019, China

4. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

5. INFN Firenze, Via Sansone 1, 50019 Sesto Fiorentino, Italy

6. Ciemat, E-28040 Madrid, Spain

7. Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi dell’Aquila, Via Vetoio, Coppito, I-67100 L’Aquila, Italy

8. INFN—Sezione di Roma Tor Vergata, via della Ricerca Scientifica 1, I-00133 Roma, Italy

9. University of Chinese Academy of Sciences, Beijing 101408, China

10. Agenzia Spaziale Italiana, via del Politecnico s.n.c., I-00133 Roma, Italy

11. INFN Perugia, Via Alessandro Pascoli 23c, I-06123 Perugia, Italy

12. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

Abstract

The HERD experiment is a future experiment for the direct detection of high-energy cosmic rays and is to be installed on the Chinese space station in 2027. The main objectives of HERD are the first direct measurement of the knee of the cosmic ray spectrum, the extension of electron+positron flux measurement up to tens of TeV, gamma ray astronomy, and the search for indirect signals of dark matter. The main component of the HERD detector is an innovative calorimeter composed of about 7500 LYSO scintillating crystals assembled in a spherical shape. Two independent readout systems of the LYSO scintillation light will be installed on each crystal: the wavelength-shifting fibers system developed by IHEP and the double photodiode readout system developed by INFN and CIEMAT. In order to measure protons in the cosmic ray knee region, we must be able to measure energy release of about 250 TeV in a single crystal. In addition, in order to calibrate the system, we need to measure typical releases of minimum ionizing particles that are about 30 MeV. Thus, the readout systems should have a dynamic range of about 107. In this article, we analyze the development and the performance of the double photodiode readout system. In particular, we show the performance of a prototype readout by the double photodiode system for electromagnetic showers as measured during a beam test carried out at the CERN SPS in October 2021 with high-energy electron beams.

Funder

National Natural Science Foundation of China

Publisher

MDPI AG

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