Results from the Antarctic muon and nuetrino detector array

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 at...

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Bibliographic Details
Main Authors: Ahrens, Jürgen, Bertrand, Daniel, Binon, Freddy, Bouhali, Othmane, Dewulf, Jean-Paul
Format: Article in Journal/Newspaper
Language:English
Published: 2003
Subjects:
Physique atomique et nucléaire
Antarctic
The Antarctic
Antarc*
Online Access:http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/206055
https://dipot.ulb.ac.be/dspace/bitstream/2013/206055/1/Elsevier_189682.pdf
Description
Summary: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. 0 SCOPUS: ar.j SCOPUS: ar.j info:eu-repo/semantics/published

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