Ice Cube: Physics, status, and future

被引：6
|
作者：
Hultqvist, Klas [1 ]
机构：
[1] Stockholm Univ, Dept Phys, Oskar Klein Ctr, S-10691 Stockholm, Sweden
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2011年 / 626卷
关键词：
IceCube; Neutrino astronomy; Cosmic rays; South pole; Dark matter; HIGH-ENERGY NEUTRINOS; PAIR PRODUCTION; DARK-MATTER; ANISOTROPY; ICECUBE; BREMSSTRAHLUNG; SIMULATION; EXTENSION;
D O I：
10.1016/j.nima.2010.05.014
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
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. (c) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码：S6 / S12
页数：7
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