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
How Physical Processes Form Physical Features. PolarTREC researcher Samantha Hansen shares this resource as a background to her work and information on geologic processes.
Class notes and detailed information on mountain building. PolarTREC researcher Samantha Hansen shares this resource as a background to her work and information on geologic processes. Created by John C. Butler, July 29, 1995. Credit to: John Butler jbutler [at] uh.edu