Elsevier B.V.Nuclear Physics B (Proceedings Supplements)H. Landsman and The AURA Collaboration. AURA next generation neutrino detector in the South Pole. NuPhB Proceedings Supplements, 168:268-270, June 2007.Nucl. Phys. B (Proc. Suppl.) 168: pp. 268AURA Collab. (H. Landsman et al.), ...
In this contribution, recent results from the Antarctic Muon And Neutrino Detector Array (AMANDA-II) on searches for high-energy neutrinos of extraterrestrial origin are presented. In particular, different methods to investigate the diffuse neutrino flux, the single and stacked search for neutrino ...
“With the completion ofIceCube, the 1970s dream of building a kilometer-scale neutrino detector has finally become a reality,” says Francis Halzen, a professor of physics at the University of Wisconsin-Madison and the IceCube Collaboration’s principal investigator. “Finally science can start wit...
“With the completion ofIceCube, the 1970s dream of building a kilometer-scale neutrino detector has finally become a reality,” says Francis Halzen, a professor of physics at the University of Wisconsin-Madison and the IceCube Collaboration’s principal investigator. “Finally science can start wit...
A similar foreign neutrino detector is the IceCube Neutrino Observatory deployed near the South Pole. Compared with this glacier facility, the TRIDENT in the deep sea will perform much better as clean water with fewer impurities is better for observation. ...
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near theSouth Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmospheric and extra-terrestrial. A complete simulation ...
On Mar. 30, the National Science Foundation announced a five-year, $35 million grant for the continued operation and management of IceCube, the neutrino detector located over a mile deep in the ice at NSF’s Amundsen-Scott South Pole Station. Get training in Effectively Advocating for the ...
The first stage of the AMANDA High Energy Neutrino Detector at the south Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection, seasonal muon flux variation, relativistic monopole flux limits, a search for...
The AMANDA neutrino detector - Status reportdoi:10.1016/S0920-5632(00)00497-7The first stage of the AMANDA High Energy Neutrino Detector at the south Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection...
In the present paper we evaluate the effect of neutrino flavor mixing and possible CPT violation (MINOS like) for up-going atmospheric muon neutrinos measured with the Deep Core detector of the IceCube Neutrino Observatory at South Pole. Our evaluation of rate and spectrum is based on the known...