HIGH-ENERGY NEUTRINO ASTROPHYSICS
By J. Learned, K. Mannheim. 2003
243 citations recorded by the source corpus.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/8dc24b52e7b77e37e3a5630c558a90fb672abd73
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In Nuclear and High Energy Physics
- Todor Stanev
- W. Rhode
- S. Boser
- T. Kintscher
- Thomas K. Gaisser
- D. Soldin
- Anna Franckowiak
- The IceCube Collaboration
Citations in the corpus
- OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA (2016, background): “Their observation will help to elucidate the unknown sources of high-energy cosmic rays (Gaisser et al. 1995; Learned & Mannheim 2000; Becker 2008).”
- Muon Track Reconstruction and Data Selection Techniques in AMANDA (2004, background): “electron- or tau-neutrinos. A high-energy νµ charged current interaction creates a muon, which is nearly collinear with the neutrino direction; having a mean deviation angle of ψ= 0.7◦ ×(E ν/TeV)−0.7 [2], which implies an accuracy requirement of .1◦ for reconstructing the muon direction. The high-en”