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

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

AMANDA

Collaboration

Nov, 2002

9 pages

Part of Neutrino physics and astrophysics. Proceedings, 20th International Conference, Neutrino 2002, Munich, Germany, May 25-30, 2002, 371-379

Published in:

Nucl.Phys.B Proc.Suppl. 118 (2003) 371-379

Contribution to:

- Neutrino 2002
, 371-379

e-Print:

astro-ph/0211264 [astro-ph]

DOI:

10.1016/S0920-5632(03)01335-5

Experiments:

AMANDA

View in:

ADS Abstract Service

reference search17 citations

Citations per year

Abstract: (arXiv)

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.

Note:

Invited talk at the XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 25-30, 2002

talk: Munich 2002/05/25
neutrino: cosmic radiation
neutrino/mu
cosmic radiation: flux
cosmic radiation: particle source
gamma ray: burst
muon: production
showers: hadronic
showers: electromagnetic
Cherenkov counter

References(18)

Figures(0)

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