Transforming DIY Geiger Counter Kits into Muon Detectors for Education and Scientific Exploration

Author:

Arcani Marco1ORCID,Liguori Domenico2ORCID,Frassà Andrea3,Nemolato Altea Renata Maria4,Del Monte Omar5,Guaita Cesare6

Affiliation:

1. Astroparticle Detectors Array Laboratory, GAT Astronomical Center, 21049 Tradate, Italy

2. INFN, National Laboratories of Frascati, Associated Group of Cosenza, IIS Liceo Scientifico “Patrizi”, 87062 Cariati, Italy

3. Dipartimento di Fisica, Università di Torino, 10124 Torino, Italy

4. Dipartimento di Scienze e Tecnologie Ambientali, Biologiche e Farmaceutiche, Università Degli Studi Della Campania “Luigi Vanvitelli”, 81100 Caserta, Italy

5. VVF, Corpo Nazionale dei Vigili del Fuoco, 15121 Alessandria, Italy

6. GAT Tradate–Planetarium “Ulrico Hoepli”, 20121 Milano, Italy

Abstract

Any Geiger counter can be used as an effective cosmic ray detector on its own. In fact, it is known that even in the absence of a radioactive source, the instrument detects what is known as background radiation, which consists of various types of ionizing particles present in the environment. Remarkably, it is estimated that up to 15% of this background radiation is attributable to cosmic rays, high-energy particles originating from outer space. The remaining radiation detected by the Geiger counter originates from terrestrial sources, such as natural radioactivity in the ground and in the air. The main goal of this project is to build a muon detector for scientific and educational purposes using two commercial DIY Geiger counter kits and just a few additional components. To identify cosmic radiation from terrestrial radiation and improve the accuracy of cosmic ray measurements, the use of a coincident circuit is essential. This coincident circuit was introduced in cosmic ray physics by Walther Bothe and Bruno Rossi in the early 1930s and allows for the detection of a subatomic particle passing through two or more sensors, thereby reducing false positives and enhancing the reliability of cosmic ray detection. The following idea is an alternative replica of our AMD5 detectors, instruments that we have been using for years to teach and perform scientific experiments in the cosmic ray field under the umbrella of the ADA project (2023 Particles, Arcani et al.). The resulting device, named AMD5ALI, offers a reliable and inexpensive solution for the same goal, making it a valuable tool for both educational purposes and scientific surveys. Practical applications range from cosmic ray physics to radioactivity, including the relationship between cosmic ray flux and meteorology, the zenithal effect, the Regener–Pfotzer curve in the atmosphere, and the anti-correlation of cosmic particle intensity with solar activity.

Publisher

MDPI AG

Reference29 articles.

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2. Walther Bothe and Bruno Rossi: The birth and development of coincidence methods in cosmic-ray physics;Bonolis;Am. J. Phys.,2011

3. Korff, S.A. (1946). Electron and Nuclear Counters Theory and Use, D. Van Nostrand Company, Inc.

4. The CosmicWatch Desktop Muon Detector: A self-contained, pocket sized particle detector;Axani;J. Instrum.,2018

5. (2024, June 07). Available online: http://cosmicpi.org/.

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