Bulletin of the American Physical Society
2025 Annual Meeting of the APS Mid-Atlantic Section
Friday–Sunday, November 14–16, 2025; Penn State Harrisburg, Middletown, Pennsylvania
Session F01: Poster Session (4:00pm - 6:00pm)
4:00 PM,
Saturday, November 15, 2025
Penn State Harrisburg
Room: Capital Union Building (CUB) Room 210
Abstract: F01.00046 : Pitt-CoRTExCosmic Ray Tracker Experiment for Education and Outreach*
Presenter:
Sean Maloney
(Department of Physics and Astronomy, Pitt)
Author:
Sean Maloney
(Department of Physics and Astronomy, Pitt)
designed to be easily transportable for education and outreach purposes. The grid-
like detector is able to record spatial information about the path of the muon and
displays its path in real time on an LED cube. The detector makes use of multiple
solid-state scintillating panels which can be interlocked to form a 3D grid. As muons
pass though this grid, they deposit energy which is then emitted as scintillation light.
The light is ultimately transmitted to a silicon photomultiplier via a optical fiber,
enabling reconstruction of muon tracks. Due to the modular nature of our detector,
it can easily be transported to new locations both for education and data capturing
purposes. In initial simulations of the detector, we have shown that we can reconstruct
the path of a muon and display its trajectory in real time using low-power, portable
hardware such as a Raspberry Pi 4. We also implement a live monitoring web server
to be able to track the health of the detector and individual panels; as well as a LED
visualization cube, to be able to show the path of the muon in real time. Future version
of the detector will feature built-in LEDs to eliminate the need for the visualization
cube. This presentation will highlight the ongoing work of the construction of 3x3x3
prototype detector and the R&D for an 8x8x8 in the near future for improved data
acuracy and spatial resolution.
*We would like to thank the Emil Sanielevici Scholarship, NASA Pennsylvania Space Grant ConsortiumResearch Scholarship, Dietrich Innovation Initiative, and Pitt’s Department of Physics and Astronomy for support for this project
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