The Advanced Physics course at Oral Roberts University is designed to prepare students for careers in engineering and research by integrating hands-on, adaptable laboratory projects relevant to applied physics and engineering disciplines. A central component of this curriculum involves a student-led investigation into cosmic ray cascades, emphasizing the detection and characterization of muons—massive elementary particles analogous to electrons, generated through high-energy interactions between cosmic rays and atmospheric molecules.
This research represents the latest phase of an ongoing experimental series exploring cosmic ray cascade phenomena. Previous phases optimized detection methodologies by calibrating steel plate thickness to enhance cascade visualization and by mapping the angular distribution of muons under varying geometrical configurations. The current phase focuses on quantifying the effects of environmental parameters on cascade formation and muon detection. Students conducted systematic measurements correlating cascade frequency and intensity with atmospheric temperature, pressure, and meteorological conditions using an optimized detector array (11 plates inclined at 70° toward the northern horizon).
Preliminary results suggest that environmental variations play a significant role in muon flux at ground level. Elevated atmospheric temperatures correspond to reduced muon counts due to increased meson decay altitudes, while lower pressure conditions appear to enhance muon transmission to the surface. Additional influences, including humidity, solar activity, geomagnetic effects, and altitude, further modulate detection rates.
These findings advance the pedagogical integration of experimental particle physics into undergraduate education, while contributing meaningful data to the broader study of cosmic ray interactions and environmental modulation of high-energy particle cascades.
The full paper will be available to logged in and registered conference attendees once the conference starts on June 21, 2026, and to all visitors after the conference ends on June 24, 2026