Results 211 to 220 of about 77,537 (257)

Neutrino detector. Progress report

, 1978
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Measurements of Coherent Cerenkov Radiation in Rock Salt: Implications for GZK Neutrino Underground Detector

, 2018
R. Milincic
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A new solar neutrino detector

Nuclear Physics B - Proceedings Supplements, 1993
Abstract This paper describes the main features of the proposed low energy solar neutrino detector Borexino, planned to be installed at the Gran Sasso Laboratory. This real time detector is based on a massive, calorimetric, liquid scintillation spectroscopy technique, whose high luminosity is the base for the attempt to achieve a low signal detection
G. Alimonti, B. Alpat, C. Arpesella, G. Bellini, P. Benetti, S. Bonetti, F. Calaprice, M. Campanella, G. Cecchet, A. Debari, M. Deutsch, A. Donati, F. Elisei, F. Vonfeilitzsch, D. Franciotti, M. Giammarchi, D. Giugni, A. Golubchikov, G. Husser, T. Kovacs, I. Manno, G. Mantovani, G. Manuzio, F. Masetti, U. Mazzucato, E. Meroni, J. Mitchell, L. Oberauer, S. Pakvasa, A. Perotti, A. Preda, P. Raghavan, R. Raghavan, F. Ragusa, G. Ranucci, R. Scardaoni, S. Schonert, O. Smirnov, R. Tartaglia, G. Testera, P. Ullucci, S. Vitale, O. Zaimidoroga   +42 more
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Salt neutrino detector for ultrahigh-energy neutrinos

Physics of Atomic Nuclei, 2004
Rock salt and limestone are studied to determine their suitability for use as a radio-wave transmission medium in an ultrahigh energy (UHE) cosmic neutrino detector. A sensible radio wave would be emitted by the coherent Cherenkov radiation from negative excess charges inside an electromagnetic shower upon interaction of a UHE neutrino in a high ...
M. Chiba, T. Kamijo, O. Yasuda, Y. Chikashige, T. Kon, Y. Takeoka, R. Yoshida   +6 more
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Neutrino Detectors Review

AIP Conference Proceedings, 2005
The neutrino physics is one of the most important research field and there are several experiments made and under construction focused on it. This paper will present a review on some detectors used for Solar Neutrinos detection, Atmospheric Neutrinos detection and in Long Baseline Experiments.
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Solar flares and neutrino detectors

Physical Review Letters, 1988
Solar flares have been suggested as the cause of occasional high counting rates in the $^{37}\mathrm{Cl}$ solar-neutrino experiment. The sensitivity of neutrino detectors to flares is evaluated. Several neutrino detectors will show large signals when prominent flares are observed electromagnetically, if flares are detected in the chlorine experiment.
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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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