Results 211 to 220 of about 77,742 (251)

Underwater Neutrino Detectors

2001
Due to their weak interaction with matter and to the absence of their interaction with the electro-magnetic radiations, neutrinos can travel in the Universe without being absorbed. This is not the case for photons which interact with matter, with the infra-red (IR) radiation and with the cosmic microwave background (CMB).
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Fluorine scintillator neutrino detector

Nuclear Physics B - Proceedings Supplements, 1994
8B solar neutrino detection is proposed via charge current reaction ve + 19F with hexafluorobenzene scintillator detector. Main advantage of the detector is possibility to identify neutrino interaction by means of observation of coincidence with delayed β+-decay of 19Ne (T12 = 17s).
I.R. Barabanov, V.I. Cherehovsky, G.V. Domogatsky, V.I. Gurentsov, A.B. Gurski, A.V. Kopylov, S.P. Mikheyev, I.V. Orekhov, V.G. Ryasny, G.T. Zatsepin   +9 more
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The AMANDA Neutrino Detector

Nuclear Physics B - Proceedings Supplements, 1999
The first stage of the AMANDA High Energy Neutrino Detectorat the South Pole, the 302 PMT array AMANDA-B with an expected effectivearea for TeV neutrinos of similar to 10(4) m(2), has been taking datasince 1997. Progress with calibration, investigation of ice properties,as well as muon and neutrino data analysis are described.
R. Wischnewski, E. Andrés, P. Askebjer, S. Barwick, R. Bay, L. Bergström, A. Biron, J. Booth, O. Botner, A. Bouchta, S. Carius, M. Carlson, W. Chinowsky, D. Chirkin, D. Cowen, C. Costa, E. Dalberg, T. Deyoung, J. Edsjo, P. Ekström, A. Goobar, L. Gray, A. Hallgren, F. Halzen, R. Hardtke, Y. He, G. Hill, P. Hulth, S. Hundertmark, J. Jacobsen, V. Kandhadai, A. Karle, J. Kim, H. Leich, M. Leuthold, P. Lindahl, T. Liss, I. Liubarsky, P. Loaiza, D. Lowder, P. Marciniewski, T. Miller, P. Miocinovic, P. Mock, R. Morse, M. Newcomer, P. Niessen, D. Nygren, C. Pérez de los Heros, R. Porrata, P. Price, G. Przybylski, W. Rhode, S. Richter, J. Rodriguez, P. Romenesko, D. Ross, H. Rubinstein, T. Schmidt, E. Schneider, R. Schwarz, U. Schwendicke, G. Smoot, M. Solarz, V. Sorin, C. Spiering, P. Steffen, R. Stokstad, O. Streicher, L. Thollander, T. Thon, S. Tilav, C. Walck, C. Wiebusch, K. Woschnagg, W. Wu, G. Yodh, S. Young   +77 more
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Liquid argon neutrino detectors

Nuclear Physics B - Proceedings Supplements, 2001
Abstract The Liquid Argon imaging technique, as proposed for the ICARUS detector, offers the possibility to perform complementary and simultaneous measurements of neutrinos, as those of CERN to Gran Sasso beam (CNGS) and those from cosmic ray events.
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The Homestake Neutrino Detector

Nuclear Physics B - Proceedings Supplements, 2012
Abstract Neutrino mass ordering, mixing, and potential for CP violation are some of the most important questions facing particle physics today. To address them, a Long Baseline Neutrino Experiment (LBNE) is being planned using a 700 kw beam that would be directed from Fermilab to an underground site in Lead, South Dakota – a baseline of 1300 km.
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Neutrino Detectors

2021
D. F. Cowen, I. Taboada
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MINERνA neutrino detector calibration

AIP Conference Proceedings, 2015
MINERνA is a neutrino scattering experiment that uses Fermilab’s NuMI beamline. Its goal is to measure cross-sections for neutrino scattering from different nuclei. Precise knowledge of these cross-sections is vital for current and future neutrino oscillation experiments.
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Neutrino detectors

2023
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Neutrino Detectors

2012
Franz von Feilitzsch, Jean-Côme Lanfranchi, Michael Wurm   +2 more
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Future atmospheric neutrino detectors

Plenary talk at the Neutrino 2024 conference. Session 12: Three flavour neutrino oscillations - Atmospheric ν.
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