z-logo
open-access-imgOpen Access
Construction and operation of large scale Micromegas detectors for the ATLAS Muon upgrade
Author(s) -
I. M. Maniatis,
D. Sampsonidis,
C. Lampoudis,
I. Manthos,
C. Petridou,
S. Tzamarias,
K. Kordas,
Katerina Dima,
A. Kallitsopoulou,
I. Kalaitzidou,
I. Karkanias,
S. Kompogiannis,
I. Maznas,
E. Maragkou,
M. Tsopoulou,
P. Paschalias,
T. Koutsosimos,
I. Tsiafis
Publication year - 2021
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/2105/1/012021
Subject(s) - micromegas detector , upgrade , large hadron collider , detector , physics , atlas (anatomy) , muon , nuclear physics , atlas experiment , cosmic ray , atlas detector , optics , computer science , geology , operating system , paleontology
After the forthcoming upgrade of the LHC accelerator at CERN, its luminosity will increase up to 7.5 × 10 34 cm −2 s −1 . That will raise the readout rates and the background data to unmanageable levels for the existing ATLAS muon spectrometer. The ATLAS collaboration has proposed to replace the present small wheel muon detector with the New Small Wheel (NSW) to surpass those limitations. The new wheels consist of Micromegas (MM) and small-strip Thin Gap Chambers (sTGC). The first technology aims for precision tracking, and the last one for trigger purposes. Each wheel will be equipped with eight small and eight large sectors, while each sector will have a double MM wedge surrounded by sTGC wedges. The MM detectors for the NSW will be the largest developed Micro Pattern Gaseous Detector (MPGD) as they will cover an area up to 1280 m 2 . During detectors’ manufacture have been used various custom materials (PCBs, mesh) and innovative construction techniques. This paper describes the MM drift panels production at Aristotle University of Thessaloniki laboratory. Then will be presented resolution results of the MM detectors with cosmic-ray tests at CERN facilities.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here