Students will learn about the difference between the methods of neutrino detection – optical versus radio. This will then allow them to understand why the relative size of the detectors is so different. Students will also engage in a hands-on activity to understand scale through creating models of the two detectors.
Kate Miller & Katey Shirey co-presented at the National Science Teachers Association (NSTA) Regional Conference in Milwaukee, WI. Our presentation was entitled "Living & Working at the South Pole" and was part of the "Physics Day" set of IceCube-related presentations. About 100 people attended with several questions at the end.
Kate Miller is joined by IceCube undergraduate researcher, Samantha Pedek, in presenting at the Arlington Public Schools' Superintendent's Seminar.
Superintendent’s Seminar is a summer enrichment program for rising 11th and 12th graders who have demonstrated a desire for an academic experience. Approximately 30 students from across the district spend a week participating in activities focusing on this year's theme of
Oftentimes called “ghost particles,” neutrinos can travel through nearly everything (the sun, the earth, you!) undetected. Because they are nearly massless, gravitational fields do not affect neutrinos; Similarly, because they are chargeless, electric and magnetic fields do not con affect neutrinos. This lack of interaction is advantageous for IceCube researchers – when they detect a neutrino, it is a
In this lesson, students will be introduced to the Standard Model, learning key vocabulary such as Fermions, Hadrons, Mesons, Baryons, Quarks, Leptons, particles, and anti-particles. In particular, students will come to understand what a neutrino is and why it is such a unique particle. This understanding connects to the IceCube Neutrino Observatory’s search for neutrinos in an effort to