Results from the Antarctic Muon and Neutrino Detector Array (AMANDA)

Details Results from the Antarctic Muon and Neutrino Detector Array (AMANDA) Results from the Antarctic Muon and Neutrino Detector Array (AMANDA)

2002-11-12

arxiv.org/abs/astro-ph/0211264v1

Nucl.Phys.Proc.Suppl.118:371-379,2003

Astronomy and Astrophysics

Astrophysics

Invited talk at the XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 2

Scientific paper

10.1016/S0920-5632(03)01335-5

We show new results from both the older and newer incarnations of AMANDA (AMANDA-B10 and AMANDA-II, respectively). These results demonstrate that AMANDA is a functioning, multipurpose detector with significant physics and astrophysics reach. They include a new higher-statistics measurement of the atmospheric muon neutrino flux and preliminary results from searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, gamma-ray bursters and diffuse sources producing muons in the detector, and diffuse sources producing electromagnetic or hadronic showers in or near the detector.

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