'Neutrino telescope' diaporamas de présentation

Neutrino Telescopes and the Neutrino Mass Hierarchy

University of Manchester, School of Physics and Astronomy Seminar, 27 February 2013. Neutrino Telescopes and the Neutrino Mass Hierarchy. Uli Katz ECAP / Univ. Erlangen. The plan for the next 50 minutes:. Introduction Present and future neutrino telescopes: ANTARES, IceCube, KM3NeT

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Request for CERN recognized experiment status for the IceCube neutrino telescope

Request for CERN recognized experiment status for the IceCube neutrino telescope. Per Olof Hulth Stockholm university hulth@physto. se. IceCube. Neutrino telescope to be built in the ice sheet at the South Pole, Antarctica

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Neutrino Astronomy with KM3NeT

Vulcano Workshop 2008: Frontier Objects in Astrophysics and Particle Physics Vulcano, Eolian Islands, Italy, May 25-31, 2008. Neutrino Astronomy with KM3NeT. The KM3NeT physics case What happened so far The KM3NeT Conceptual Design Report The Preparatory Phase: Towards implementation.

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Neutrino Telescopes and Neutrinos from LHC

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Moscow, 18.10.2005

The Baikal neutrino telescope: Physics results and future plans. V. Aynutdinov, INR RAS for Baikal collaboration. Moscow, 18.10.2005. Collaboration. Institute for Nuclear Research, Moscow, Russia. Irkutsk State University, Russia.

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KM 3 Ne utrino T elescope European deep-sea research infrastructure

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Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. Calibration, filtering and reconstruction strategies for KM3NeT. G. Bourlis , N. A. B. Gizani , A. Leisos , A. G. Tsirigotis , S.E. Tzamarias.

458 views • 27 slides

Deep-sea neutrino telescopes

Deep-sea neutrino telescopes. Prof. dr. Maarten de Jong Nikhef / Leiden University. contents. Neutrino astronomy Antares prototype KM3NeT next generation neutrino telescope issues, ideas. Neutrino astronomy. p. n. g. neutrinos. Why neutrinos? no absorption no bending.

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CP-even neutrino beam

CP-even neutrino beam. N. Sasao Kyoto University The talk is based on hep-ex/0612047 done in collaboration with A. F ukumi, I. Nakano, H. Nanjo, S. Sato, M. Yoshimura. Introduction. If finite value of q 13 is NOT found in the next round neutrino experiments, we need

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ANTARES: a system of underwater sensors looking for neutrinos

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Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. Use of fl oating surface detector stations for the calibration of a deep-sea neutrino telescope. G. Bourlis , N. A. B. Gizani , A. Leisos , A. G. Tsirigotis , S.E. Tzamarias.

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Time Calibration of the ANTARES Neutrino Telescope

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Probing Neutrino Mixing and Unitarity Violation at Neutrino Telescopes

TeV Particle Astrophysics, 24-28 September, 2008, Beijing, China. Shun Zhou. IHEP, CAS, Beijing. Based on our recent works: Z.Z. Xing and S. Zhou, PLB (2008); PRD (2006). Outline. UHE Neutrinos: Challenges and Opportunities Determination of the Initial Flavor Composition

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Rezo Shanidze

MC Studies in Erlangen & Neutrinos from SN in KM3NeT ?. Rezo Shanidze. KM3NeT Meeting, Catania, 11-13 March, 2008. MC Optimization Studies. S. Kuch, PhD thesis, www.slac.stanford.edu/spires/find/hep/www?r=FAU-PI1-DISS-07-001.

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Development of a compact acoustic calibrator for ultra-high energy neutrino detection

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Search for diffuse cosmic neutrino fluxes with the ANTARES detector

Search for diffuse cosmic neutrino fluxes with the ANTARES detector. Vladimir Kulikovskiy. The ANTARES Collaboration. Overview. ANTARES description Full sky searches Special region searches Fermi bubbles Milky Way Future plans. The ANTARES detector. Visibility. LED beacon.

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The KM3Net Consortium

The KM3Net Consortium. Towards a km3-scale neutrino telescope in the Mediterranean Sea. C. Distefano on behalf of the KM3NeT Consortium. Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Sud. What is KM3NeT ?. An acronym for KM3 Ne utrino T elescope

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George W.S. Hou & M.A. Huang Center for Cosmology and Particle Astrophysics

Expected Performance of a Neutrino Telescope for Seeing AGN/GC Behind a Mountain. Abstract We study the expected performance of building a neutrino telescope, which targets at energy greater than

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? track

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KM3NeT Neutrino telescope in the Mediterranean Sea

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