English

IceCube: physics, status, and future

High Energy Astrophysical Phenomena 2019-08-13 v1

Abstract

The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detectors in the IceTop surface array. The range of physics topics includes neutrino signals from astrophysical sources, dark matter, exotic particle physics, cosmic rays, and atmospheric neutrinos. The current IceCube status and selected results are described. Anticipated future developments are also discussed, in particular the Deep Core low energy subarray which was recently deployed.

Keywords

Cite

@article{arxiv.1003.2300,
  title  = {IceCube: physics, status, and future},
  author = {Klas Hultqvist},
  journal= {arXiv preprint arXiv:1003.2300},
  year   = {2019}
}

Comments

Presentation at the 4th International Workshop on Very Large Volume Neutrino Telescopes

R2 v1 2026-06-21T14:56:37.444Z