'Amanda ii' diaporamas de présentation

first-generation neutrino telescopes

first-generation neutrino telescopes. Infrequently, a cosmic neutrino is captured in the ice, i.e. the neutrino interacts with an ice nucleus. In the crash a muon (or electron, or tau) is produced. Cerenkov light cone. muon or tau. interaction. Detector.

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Baikal-Amanda-IceCube

Baikal-Amanda-IceCube. Neutrino-Astronmie in DESY Zeuthen. Christian Spiering, Technisches Seminar, Mai2004. Entdeckung der Kosmischen Strahlen 1912. Viktor Hess (Nobelpreis 1936). 1 TeV (HERA). Kosmische Strahlen. ?. ?. ?. Neutrino-Teleskope in Wasser und Eis. Super-K. Baikal.

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High Energy Neutrino Astronomy from infancy to maturity

?. A. High Energy Neutrino Astronomy from infancy to maturity. LAUNCH Meeting Heidelberg Christian Spiering DESY. ?. A. High Energy Neutrino Astronomy from infancy to maturity. technological. ?. A. The idea. Bruno Pontecorvo. Moisej Markov. M.Markov, 1960 :

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UHE Neutrino Astronomy

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Particle Astronomy from Antarctica Per Olof Hulth Stockholm University

Particle Astronomy from Antarctica Per Olof Hulth Stockholm University. Why Particle Astronomy from Antarctica?. Difficult logistics No continues access during the year Cold and expensive Long time to build up large experiment. Antarctic platform.

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IceCube

IceCube. Christian Spiering, VLVNT Workshop Amsterdam, October 2003. IceCube Collaboration. Institutions: 11 US, 11 European, 1 Japanese and 1 Venezuelan Bartol Research Institute, University of Delaware BUGH Wuppertal, Germany Universite Libre de Bruxelles, Brussels, Belgium

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The AMANDA-II Telescope - Status and First Results -

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Searching for Quantum Gravity with AMANDA-II and IceCube

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

Results from the Antarctic Muon and Neutrino Detector Array (AMANDA). Allan Hallgren** Uppsala University Allan.Hallgren@tsl.uu.se. For the most excellent marriage of particle physics and astronomy : Something old Recap of recent results Something new New analyses of older data

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Tests of Quantum Gravity with Neutrino Telescopes

Tests of Quantum Gravity with Neutrino Telescopes. John Kelley University of Wisconsin, Madison From Quantum to Emergent Gravity: Theory and Phenomenology Trieste, Italy June 15, 2007. Overview. Detection principles of large-scale neutrino telescopes Capabilities (and limitations)

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Neutrino Astronomy with AMANDA

Neutrino Astronomy with AMANDA. Steven W. Barwick University of California-Irvine. SPIE Conference -Hawaii, 2002. Outline of Talk. Science of HE Neutrino Telescopes Point Sources Diffuse Sources (up and down) GRBs WIMP annihilations in earth and sun

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Neutrino Astronomy at the South Pole

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Neutrino Astronomy at the South Pole

Neutrino Astronomy at the South Pole. David Boersma UW Madison Lake Louise Winter Institute Chicago, 23 February 2006. IceCube Collaboration. Alabama University, USA University of Alaska, Anchorage, USA Bartol Research Institute, Delaware, USA Pennsylvania State University, USA

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Searching for Quantum Gravity with AMANDA-II and IceCube

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Probing for Leptonic Signatures from Gamma-Ray Bursts with Antarctic Neutrino Telescopes

Probing for Leptonic Signatures from Gamma-Ray Bursts with Antarctic Neutrino Telescopes. M ICHAEL S TAMATIKOS U NIVERSITY OF W ISCONSIN, M ADISON D EPARTMENT OF P HYSICS michael.stamatikos@icecube.wisc.edu

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Neutrino Point Source Searches with AMANDA-II m -DAQ

Neutrino Point Source Searches with AMANDA-II m -DAQ. Jim Braun. AMANDA-II complete. 2000. D. Steele: Phys.Rev.Lett.92:071102 2004. 2001. Y.-R. Wang: Phys.Rev.D71:077102 2005. 2002. M. Ackermann: Phys.Rev.D75:102001 2007. 2003. 2004. 2005. Unblinded in 2007 by J. Braun. 2006.

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CORSIKA/MMC for the IceCube simulation production

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IceCube

single neutrinos average of two neutrinos. 2 o x 2 o. 250 n m a day for IceCube. GRB/SN time -window:100 sec. Detecting high energy neutrinos from Supernovae. While core-collapse SNe are guaranteed sources of low-energy neutrinos,

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Performance of the AMANDA-II Detector

Performance of the AMANDA-II Detector. R.Wischnewski for the AMANDA Collaboration; DESY-Zeuthen, Germany. AMANDA-II Detector. ? Largest High Energy Neutrino-Detector ever built:An open Under-Ice Cerenkov Detector for high energy muons and showers.

154 views • 1 slides