15–19 Apr 2024
Edinburgh
Europe/London timezone

A Beam Monitor For The AMS-02 Layer0 Tracker Upgrade

17 Apr 2024, 14:50
20m
Nucleus Building, Yew Lecture Theatre (Edinburgh)

Nucleus Building, Yew Lecture Theatre

Edinburgh

Scotland, United Kingdom

Speaker

Dexing Miao (The Institute of High Energy Physics of the Chinese Academy of Sciences (CN))

Description

The Alpha Magnetic Spectrometer (AMS-02) detector operates on the International Space Station. It performs high precision measurements of cosmic ray composition and fluxes, searches for antimatter and dark matter. To increase the detection acceptance and improve its heavy ion identification power, the AMS collaboration plan to add a new layer (L0) of silicon tracker on top of AMS-02. The detector consists of 2 planes, 72 silicon strip detector ladders. Each ladder has 8, 10, or 12 silicon strip detector sensors (SSDs) connected in serial, producing an effective strip length of about 1 meter. The total sensitive area is about $8m^2$.

In order to study the detector ladder in cosmic rays and particle beams, and calibrate the L0 tracker with particle beams before launching to the space, a beam monitor has been produced. The monitor consists of 10 single-SSD modules with a readout electronics system similar to that of the L0 detector. The beam monitor alone had been used in testbeams using electron beam at IHEP to characterize the SSD, which was custom designed for the AMS L0 upgrade. The beam monitor has also been used to test prototype ladders using proton, muon and heavy ion beams at CERN.

In this talk details of the beam monitor and its performance will be described. The tracking and alignment methods based on GBL and Millepede-II packages will also be introduced. Results from the SSD characterization from the testbeam at IHEP will also be presented.

Authors

Alessio Ubaldi (Universita e INFN, Perugia (IT)) Dexing Miao (The Institute of High Energy Physics of the Chinese Academy of Sciences (CN)) Gianluigi Silvestre (Universita e INFN, Perugia (IT)) Ms Hongyu Zhang (FDU) Hsinyi Chou Jianchun Wang (Chinese Academy of Sciences (CN)) Mr Liu Cong (SDIAT) Lorenzo Mussolin (Universita e INFN, Perugia (IT)) Mrs Maria Ionica (INFN Perugia, via A. Pascoli 23c, Perugia, I-06100, Italy) Matteo Duranti (Universita e INFN, Perugia (IT)) Mattia Barbanera (Universita e INFN, Perugia (IT)) Maura Graziani (Universita e INFN, Perugia (IT)) Mingjie Feng (Chinese Academy of Sciences (CN)) Pingcheng Liu (Shandong Institute of Advanced Technology (SDIAT) (CN)) Qinze Li (Chinese Academy of Sciences (CN)) Shuqi Sheng (Chinese Academy of Sciences (CN)) Tiange Li (Chinese Academy of Sciences (CN)) Valerio Formato (INFN - Sezione di Roma Tor Vergata) Xiaojie Jiang (Chinese Academy of Sciences (CN)) Xudong Cai (Massachusetts Inst. of Technology (US)) Yaozu Jiang (Universita e INFN, Perugia (IT)) Zhiyu Xiang (Chinese Academy of Sciences (CN)) Zijun Xu (Chinese Academy of Sciences (CN))

Presentation materials