Published June 2005
| Version v1
Journal article
The Auger Observatory: Status and Potential for Neutrino Detection
Creators
- 1. Departamento de Fisica de Particulas, Universidad, E-15706 Santiago de Compostela (Spain) and Kavli Institute for Cosmological Physics, 5640 South Ellis Av., Chicago, IL 60637 (US)
Description
The southern Auger observatory which is being constructed in Malarguee, Mendoza, Argentina, is the largest cosmic ray detector in operation. Its concept and design, progress in its construction and its excellent performance are summarized paying special attention to inclined showers. Data are being collected at an ever increasing rate and some representative examples of reconstructed events are shown. The connection between Ultra High Energy Cosmic Rays and neutrinos is discussed. Progress in understanding the differences between inclined showers produced by protons and nuclei and those expected from neutrinos and calculations of the neutrino acceptance are reviewed
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2005.01.133;
- PII
- S0920-5632(05)00134-9;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 143
- Journal Page Range
- p. 373-380
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 21. international conference on neutrino physics and astrophysics
- Acronym
- NEUTRINO 2004
- Dates
- 14-19 Jun 2004
- Place
- Paris (France)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37108968
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CONSTRUCTION; DESIGN; NEUTRINO DETECTION; NEUTRINOS; NUCLEI; OPERATION; PROTONS; RADIATION DETECTORS; SHOWERS
- Descriptors DEC
- BARYONS; DETECTION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; LEPTONS; MASSLESS PARTICLES; MEASURING INSTRUMENTS; NUCLEONS; RADIATION DETECTION
Optional Information
- Copyright
- Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.