Bulletin of the American Physical Society
Fall 2022 Meeting of the APS Division of Nuclear Physics
Thursday–Sunday, October 27–30, 2022; Time Zone: Central Daylight Time, USA; New Orleans, Louisiana
Session LM: Undergraduate Research II
2:00 PM–3:36 PM,
Saturday, October 29, 2022
Hyatt Regency Hotel
Room: Imperial 9
Chair: Riccardo Longo, University of Illinois at Urbana-Champai
Abstract: LM.00006 : A New LED Pulser Board For The ATLAS Reaction Plane Detector in LHC Run 4*
3:00 PM–3:12 PM
Presenter:
Kristopher D Young
(University of Illinois at Urbana-Champaign)
Authors:
Kristopher D Young
(University of Illinois at Urbana-Champaign)
Riccardo Longo
(University of Illinois at Urbana-Champaign)
Matthias Grosse Perdekamp
(University of Illinois at Urbana-Champaign)
Daniel R MacLean
(University of Illinois at Urbana Champaign (Now at FNAL))
Yi Liu
(University of Illinois at Urbana-Champaign)
Mandela Phillips
(Parkland College (REU student at University of Illinois at Urbana Champaign)))
Christian Hornhuber
(University of Kansas)
Michael Murray
(University of Kansas)
Collaboration:
JZCaP
The HL-ZDC will be installed inside the TAXN absorber, 126 meters downstream of the interaction point, for heavy ion related data taking. The extreme radiation environment that the detector will be exposed to requires a LED calibration system, that allows for monitoring the HL-ZDC Photo-Multiplier Tubes (PMTs) performance during data taking.
The University of Illinois at Urbana Champaign (UIUC), in collaboration with Kansas University (KU), is developing a new LED pulser board to be deployed in the HL-ZDC. When provided external triggers, this board will drive LEDs of different colors to pulse the HL-ZDC PMTs, monitoring their response at different wavelengths. This contribution will present the design of the new board and the evaluation of its performance. Next steps towards the final design of the pulser will be discussed, together with plans for radiation hardness tests at irradiation facilities at CERN.
*This work is supported by the National Science Foundation, Grants no. NSF PHY-2111046 and NSF PHY-2110772.
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