High-energy neutrino telescopes

被引：0
|
作者：
Riccobene, G. [1 ]
机构：
[1] INFN, Lab Nazionali Sud, Via S Sofia 62, I-95123 Catania, Italy
来源：
NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS | 2010年 / 33卷 / 06期
关键词：
D O I：
10.1393/ncc/i2011-10762-8
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Recent results from high-energy cosmic ray and gamma detectors indicate the occurrence of hadron acceleration in cosmic sources and possible production of very-high-energy gamma-rays and neutrinos through h-. or h-h interactions. Underwater and under-ice neutrino telescopes are discovery apparatuses aiming at the detection of high-energy (> TeV) astrophysical neutrinos. The operation of the Baikal, AMANDA, ANTARES and NEMO demonstrators, validated the. Cerenkov technique as preferred solution for the construction of larger HE neutrino telescopes: IceCube, operational at the South Pole, and KM3NeT, that will be built in the Mediterranean Sea. Several R&D activities are also conducted to develop complementary experimental techniques, based on the detection of coherent acoustic (tens of kHz) or e.m. (GHz) radiation, induced by ultra-high-energy neutrino interaction in deep sea or ice.
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