Neutrino Astronomy in the Ice
arXiv:0901.2664 · doi:10.1016/j.nuclphysbps.2009.02.056
Abstract
The South Pole is an optimal location for hosting astrophysical observatories. The status of the construction of the IceCube Observatory and some selected physics results will be discussed. Moreover prospects for detection of Ultra-High Energy cosmogenic neutrinos and techniques that can address this energy region will be considered.
Proc. of NOW 2008 Conference, Conca Specchiulla, Lecce, Italy, Sept. 2008 (6 pages, 8 figures)
References in corpus (4)
- Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory
- Predictions for the Cosmogenic Neutrino Flux in Light of New Data from the Pierre Auger Observatory
- An upper limit on the electron-neutrino flux from the HiRes detector
- High energy neutrino astronomy using upward-going muons in Super-Kamiokande-I