scholarly journals IceCube — the next generation neutrino telescope at the South Pole

2003 ◽  
Vol 118 ◽  
pp. 388-395 ◽  
Author(s):  
A. Karle ◽  
J. Ahrens ◽  
J.N. Bahcall ◽  
X. Bai ◽  
T. Becka ◽  
...  
Keyword(s):  
Neutrino Telescope ◽  
South Pole ◽  
Next Generation ◽  
The South

STATUS OF THE ICECUBE NEUTRINO TELESCOPE

2005 ◽  
Vol 20 (14) ◽  
pp. 3160-3162 ◽  
Author(s):  
◽  
T. DEYOUNG
Keyword(s):  
Present Status ◽  
Neutrino Telescope ◽  
South Pole ◽  
The South ◽  
Expected Performance

IceCube is a kilometer-scale deep-ice neutrino telescope, to be constructed at the South Pole beginning in January 2005. The concept and design of IceCube, its science goals, present status, and expected performance will be discussed.

scholarly journals Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole

2020 ◽  
Author(s):  
Lorenzo Moncelsi ◽  
Peter A. Ade ◽  
Zeeshan Ahmed ◽  
Mandana Amiri ◽  
Denis Barkats ◽  
...  
Keyword(s):  
South Pole ◽  
Next Generation ◽  
The South

scholarly journals Hybrid detection of high-energy cosmic neutrinos with the next generation neutrino detectors at the South Pole

2019 ◽  
Author(s):  
Simona Toscano ◽  
Paul Coppin ◽  
Krijn de Vries ◽  
Nick van Eijndhoven ◽  
Juan Antonio Aguilar
Keyword(s):  
High Energy ◽  
South Pole ◽  
Next Generation ◽  
The South ◽  
Neutrino Detectors ◽  
Hybrid Detection

scholarly journals Observation of radio emissions from electron beams using an ice target

2019 ◽  
Vol 216 ◽  
pp. 02010
Author(s):  
Keiichi Mase ◽  
Daisuke Ikeda ◽  
Aya Ishihara ◽  
Hiroyuki Sagawa ◽  
Tatsunobu Shibata ◽  
...  
Keyword(s):  
Light Source ◽  
Electron Beams ◽  
High Energy ◽  
Neutrino Telescope ◽  
South Pole ◽  
The South ◽  
Telescope Array ◽  
Radio Emissions ◽  
Systematic Uncertainties ◽  
Radio Signals

To observe high energy cosmogenic neutrinos above 50 PeV, the large neutrino telescope ARA is being built at the South Pole. The ARA telescope detects neutrinos by observing radio signals by the Askaryan effect. We performed an experiment using 40 MeV electron beams of the Telescope Array Electron Light Source to verify the understanding of the Askaryan emission as well as the detector responses used in the ARA experiment. Clear coherent polarized radio signals were observed with and without an ice target. We found that the observed radio signals are consistent with simulation, showing that our understanding of the radio emissions and the detector responses are within the systematic uncertainties of the ARAcalTA experiment which is at the level of 30%.

scholarly journals IceCube: A Kilometer-Scale Neutrino Observatory at the South Pole

2005 ◽  
Vol 13 ◽  
pp. 949-950
Author(s):  
Francis Halzen
Keyword(s):  
Cosmic Rays ◽  
Particle Physics ◽  
High Energy ◽  
Neutrino Telescope ◽  
South Pole ◽  
Neutrino Detector ◽  
The South ◽  
High Energy Neutrino ◽  
Neutrino Telescopes ◽  
Diversity Of Science

AbstractSolving the century-old puzzle of how and where cosmic rays are accelerated mostly drives the design of high-energy neutrino telescopes. It calls, along with a diversity of science goals reaching particle physics, astrophysics and cosmology, for the construction of a kilometer-scale neutrino detector. This led to the IceCube concept to transform a kilometer cube of transparent Antarctic Ice, one mile below the South Pole, into a neutrino telescope.

ICECUBE-DEEPCORE-PINGU: FUNDAMENTAL NEUTRINO AND DARK MATTER PHYSICS AT THE SOUTH POLE

2011 ◽  
Vol 26 (39) ◽  
pp. 2899-2915 ◽  
Author(s):  
D. JASON KOSKINEN
Keyword(s):  
Dark Matter ◽  
Atmospheric Neutrino ◽  
Neutrino Flux ◽  
Neutrino Telescope ◽  
Low Energy ◽  
Atmospheric Neutrinos ◽  
South Pole ◽  
The South ◽  
Original Design ◽  
Successful Observation

The IceCube neutrino observatory at the South Pole uses 1 km3 of instrumented ice to detect both astrophysical and atmospheric neutrinos. Expanding the capabilities of the original design, the DeepCore sub-array is a low-energy extension to IceCube which will collect [Formula: see text] atmospheric neutrinos a year. The high statistics sample will allow DeepCore to make neutrino oscillation measurements at higher energies and longer baselines than current experiments. The first successful observation of neutrino induced cascades in a neutrino telescope has recently been observed in DeepCore, which upon further cultivation should help refine atmospheric neutrino flux models. Besides the fundamental neutrino physics, the low-energy reach of DeepCore, down to as low as 10 GeV, and multi-megaton effective volume will enhance indirect searches for WIMP-like dark matter. A new proposal seeking to lower the energy reach down to [Formula: see text] GeV known as the Phased IceCube Next Generation Upgrade (or PINGU) will also be described.

scholarly journals Next generation neutrino detectors at the South Pole

2019 ◽  
Vol 207 ◽  
pp. 01005
Author(s):  
Marek Kowalski
Keyword(s):  
Neutrino Physics ◽  
South Pole ◽  
Energy Window ◽  
Next Generation ◽  
The South ◽  
Neutrino Detectors ◽  
Scientific Questions

Since the construction of IceCube was completed in 2010/11, the observatory has delivered several outstanding measurements in neutrino physics and multimessenger astronomy. Additionally, a series of new scientific questions and opportunities appeared. To address these, plans have been developed to expand on the IceCube concept, targeting both lower and higher energies, as well as the central PeV-energy window at significantly improved sensitivity. In this contribution I will outline these plans.

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