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Skip to Search Results- 4IceCube
- 1Atmospheric Neutrinos
- 1Calibration
- 1Cosmic Rays
- 1DOM Efficiency
- 1Deep Inelastic Scattering
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Fall 2018
Neutrinos, one of nature's fundamental particles, have been demonstrated to oscillate (change flavour) from their point of production to detection; implying neutrinos must have mass and hence providing the first evidence for physics beyond the Standard Model of Particle Physics. Atmospheric...
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In Situ Measurement of the IceCube DOM Efficiency Factor Using Atmospheric Minimum Ionizing Muons
DownloadFall 2019
The IceCube Neutrino Observatory is a large scale neutrino detector embedded deep within the Antarctic ice located at the geographical South Pole. It instruments over one cubic kilometre of ice with 5,160 Digital Optical Modules (DOM), each of which houses a 10 inch diameter photomultiplier tube...
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Spring 2023
The dominant neutrino-nucleon interaction above 100 GeV is Deep Inelastic Scattering (DIS) in which an incoming neutrino scatters off a quark in the nucleon by exchanging a weak boson, producing an outgoing lepton accompanied by a hadron shower. Two sub-dominant processes are expected to produce...
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Fall 2023
The IceCube neutrino observatory is a gigaton Cherenkov detector located at the geographic south pole. The experiment is designed to detect neutrinos originating from the atmosphere and astrophysical objects over a huge energy range from 10 GeV to 10 PeV. Information about the interacting...