15–20 May 2022
University of Sussex
Europe/London timezone

Photodiode read-out system for the calorimeter of the HERD experiment

Not scheduled
20m
University of Sussex

University of Sussex

Falmer Campus, Brighton, Sussex, BN1 9QH, United Kingdom

Speaker

Pietro Betti (Universita e INFN, Firenze (IT))

Description

The HERD experiment is a future space experiment which will be installed on the Chinese Space Station in 2027. The detector is based on a 3D, homogeneous, isotropic, deep and finely segmented calorimeter, and it will be capable to detect particles from every direction. Thanks to its large acceptance and energy resolution, it will expand the measurements of proton and nuclei fluxes up to the cosmic ray knee region (about 1 PeV), and electron+positron flux up to tens of TeV.
The calorimeter will be composed by about 7500 LYSO cubic crystals. Every crystal is coupled with two independent read-out systems: the first is based on wavelength shifting fibers coupled to Intensified scientific CMOS, the second one is based on a system of two photodiodes coupled to a specifically designed front-end electronics. The two photodiodes have different responses with respect to scintillation light, in order to increase the dynamic range of the read-out system. This is also expanded by the use of the front-end electronics chip HiDRA2, which features a very high dynamic range, low noise and small power consumption. The latter is a necessary requirement for a space experiment due to the limited power budget. All these characteristics are necessary to obtain a dynamic range higher than 107, in order to measure signals ranging from the small MIP energy deposit for calibration purposes to typical releases caused by hadronic showers induced by PeV protons.
In this poster we will describe the main characteristics of the photodiode read-out system and we will discuss the performances of the first prototypes that were tested so far.

Primary author

Pietro Betti (Universita e INFN, Firenze (IT))

Co-authors

Alessio Tiberio (Universita e INFN, Firenze (IT)) Bo Wang (Chinese Academy of Sciences (CN)) Cecilia Pizzolotto (INFN - National Institute for Nuclear Physics) Dalian Shi (Chinese Academy of Sciences (CN)) Eugenio Berti (Universita e INFN, Firenze (IT)) Gustavo Martinez (Ciemat) Jesus Marin Munoz (Centro de Investigaciones Energéti cas Medioambientales y Tecno) Jiarui Gao (Chinese Academy of Sciences (CN)) Jinkun Zheng (Chinese Academy of Sciences (CN)) Jorge Casaus (Centro de Investigaciones Energéticas Medioambientales y Tec. (ES)) Junjing Wang (Chinese Academy of Sciences (CN)) Junjun Qin (Chinese Academy of Sciences (CN)) Leonarda Lorusso (INFN Bari) Li Zhang (Chinese Academy of Sciences (CN)) Linwei Lyu (Chinese Academy of Sciences (CN)) Lorenzo Pacini (Universita e INFN, Firenze (IT)) Miguel Angel Velasco Frutos (Centro de Investigaciones Energéticas Medioambientales y Tec. (ES)) Ming Xu (Chinese Academy of Sciences (CN)) Nicola Mori (INFN Florence) Oleksandr Starodubtsev (Universita e INFN, Firenze (IT)) Oscar Adriani (Universita e INFN, Firenze (IT)) Raffaello D’Alessandro (INFN) Ran Li (Chinese Academy of Sciences (CN)) Ruijie Wang (Chinese Academy of Sciences (CN)) Sebastiano Detti (Universita e INFN, Firenze (IT)) Sergio Bottai (Universita e INFN, Firenze (IT)) Tianwei Bao (Chinese Academy of Sciences (CN)) Valerio Formato (INFN - Sezione di Roma Tor Vergata) Valerio Vagelli (Universita e INFN, Perugia (IT)) Weiwei Cao (Chinese Academy of Sciences (CN)) Xin Liu (Chinese Academy of Sciences (CN)) Xingzhu Cui (Chinese Academy of Sciences (CN)) Yonglin Bai (Chinese Academy of Sciences (CN)) Yongwei Dong (Chinese Academy of Sciences (CN)) Zheng Quan (Chinese Academy of Sciences (CN)) Zhicheng Tang (Chinese Academy of Sciences (CN)) Zhigang Wang (Chinese Academy of Sciences (CN))

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