IceCube Science
arXiv:0901.4722 · doi:10.1088/1742-6596/171/1/012014 10.1088/1742-6596/173/1/012021
Abstract
We discuss the status of the kilometer-scale neutrino detector IceCube and its low energy upgrade Deep Core and review its scientific potential for particle physics. We subsequently appraise IceCube's potential for revealing the enigmatic sources of cosmic rays. After all, this aspiration set the scale of the instrument. While only a smoking gun is missing for the case that the Galactic component of the cosmic ray spectrum originates in supernova remnants, the origin of the extragalactic component remains as inscrutable as ever. We speculate on the role of the nearby active galaxies Centaurus A and M87.
19 pages, 8 figures; Talk at Discrete 08, Valencia, Spain
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Cited by in corpus (7)
- Prospects for constraining quantum gravity dispersion with near term observations
- The Glashow resonance at IceCube: signatures, event rates and vs. interactions
- Ultra-high neutrino fluxes as a probe for non-standard physics
- Diffuse Ultra-High Energy Neutrino Fluxes and Physics Beyond the Standard Model
- Measurements of the Time-Dependent Cosmic-Ray Sun Shadow with Seven Years of IceCube Data -- Comparison with the Solar Cycle and Magnetic Field Models
- Can the new Neutrino Telescopes reveal the Gravitational Properties of Antimatter?
- IceCube expectations for two high-energy neutrino production models at active galactic nuclei