22–28 May 2022
La Biodola - Isola d'Elba (Italy)
Europe/Rome timezone
submission of the proceedings for the PM2021 has been postponed to July 31, 2022

The Silicon Charge Detector of the High Energy Cosmic Radiation Detection facility

Speaker

Matteo Duranti (Istituto Nazionale di Fisica Nucleare)

Description

The High Energy Cosmic Radiation Detection (HERD) facility is a large field-of-view and high-energy cosmic ray detector planned to be installed on the Chinese Space Station in 2027. The Silicon Charge Detector (SCD) is a specialized HERD sub-detector measuring with accuracy the cosmic ray absolute charge magnitude $Z$, separating chemical species in cosmic rays from hydrogen ($Z=1$) to iron ($Z=26$) and beyond. The SCD concept is based on layers of single-sided micro-strip sensors able to measure energy loss and coordinates of the traversing particle. The status of the SCD design, the expected performances, and its prototyping will be discussed.

Collaboration HERD SCD Collaboration

Primary author

Alberto Oliva (Istituto Nazionale di Fisica Nucleare)

Co-authors

Andrii Tykhonov (University of Geneva) Corrado Altomare (Istituto Nazionale di Fisica Nucleare) Edoardo Mancini (Istituto Nazionale di Fisica Nucleare) Fabio Gargano (INFN-Bari) Francesco De Palma (LE) Giovanni Ambrosi (Istituto Nazionale di Fisica Nucleare) Giulia Morettini (University of Perugia) Jia-Ju Wei (Purple Mountain Observatory) Jian-Hua Guo (Purple Mountain Observatory) Ke Gong (IHEP) Lorenzo Mussolin (Istituto Nazionale di Fisica Nucleare) Lorenzo Pacini (Istituto Nazionale di Fisica Nucleare) Lucio Quadrani (BO) Massimiliano Palmieri (University of Perugia) Matteo Duranti (Istituto Nazionale di Fisica Nucleare) Mattia Barbanera (Istituto Nazionale di Fisica Nucleare) Nicola Mori (INFN Firenze) Noemi Finetti (FI) Oscar Adriani (Istituto Nazionale di Fisica Nucleare) Philipp Azzarello (DPNC, University of Geneva) Raffaello D'Alessandro (Istituto Nazionale di Fisica Nucleare) Rui Qiao (IHEP) Valerio Formato (RM2) Wang Shen (Purple Mountain Observatory) Wen-Xi Peng (IHEP) Xiang Li (Purple Mountain Observatory) Yi-Ming Hu (Purple Mountain Observatory) Yongwei Dong (Institute of High Energy Physics, Chinese Academy of Sciences) Yu-Xing Cui (Purple Mountain Observatory) Zheng Quan (IHEP)

Presentation materials