Cosmic ray muons are produced when high energy particles interact with nuclei in Earth's atmosphere. Muons make up the majority of charged particles that reach sea level and are the only particles (apart from neutrinos) that can penetrate to significant depths underground. The muon flux underground decreases approximately exponentially as a function of depth. We use a cosmic ray detector developed by the QuarkNet Program at Fermi National Laboratory to map the topography of the mountain above an abandoned Pennsylvania Turnpike tunnel by analyzing muon flux at different rock overburdens. Cosmic ray muons have been used in this capacity before to search for hidden chambers in pyramids and for mapping volcanoes. This study provides a unique field experience to learn about particle physics and particle detectors, which could be of interest to students and teachers in physics.
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November 2017
PAPERS|
November 01 2017
Cosmic ray topography
Matthew Bressler;
Matthew Bressler
Department of Math, Physics, and Statistics, Messiah College
, Mechanicsburg, Pennsylvania 17055
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Lydia Goodwin;
Lydia Goodwin
Department of Math, Physics, and Statistics, Messiah College
, Mechanicsburg, Pennsylvania 17055
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Abaz Kryemadhi
Abaz Kryemadhi
a)
Department of Math, Physics, and Statistics, Messiah College
, Mechanicsburg, Pennsylvania 17055
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a)
Electronic mail: [email protected]
Am. J. Phys. 85, 840–843 (2017)
Article history
Received:
July 21 2016
Accepted:
July 13 2017
Citation
Matthew Bressler, Lydia Goodwin, Abaz Kryemadhi; Cosmic ray topography. Am. J. Phys. 1 November 2017; 85 (11): 840–843. https://doi.org/10.1119/1.4996874
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