Results from the AMANDA Detector

Details Results from the AMANDA Detector Results from the AMANDA Detector

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004acppb..35.1919o&link_type=abstract

Acta Physica Polonica B, vol. 35, Issue 6, p.1919

Astronomy and Astrophysics

Astronomy

Scientific paper

The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial ν μ s with energies between 1011 eV and 1018 eV, ν μ s emitted from point sources and ν μ s from dark matter annihilation in the Earth and the Sun.

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