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1941
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1944“…With the goal of identifying signatures that select specific neutrino oscillation parameters, we test the robustness of global oscillation solutions that fit all the available solar and reactor experimental data. …”
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1945por Scapparone, E“…An estimate of the energy of neutrino-induced muons in MACRO is provided by a multiple Coulomb scattering measurement. …”
Publicado 2001
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1946por Ahrens, J, Kowalski, M, Bai, X, Barouch, G, Barwick, S W, Bay, R C, Becka, T, Becker, K, Bertrand, D, Biron, A, Boser, S, Booth, J R A, Botner, O, Bouchta, A, Boyce, M M, Carius, S, Chen, A, Chirkin, D, Conrad, J, Cooley, J, Costa, C G S, Cowen, D F, De Clercq, C, De Young, T, Desiati, P, Dewulf, J P, Doksus, P, Edsjö, J, Ekstrom, P, Feser, T, Frère, J M, Gaug, M, Gerhardt, L, Goldschmidt, A, Hallgren, A, Halzen, F, Hanson, K, Hardtke, R, Hauschildt, T, Hellwig, M, Herquet, P, Hill, C G, Hulth, P O, Hundertmark, S, Jacobsen, J, Karle, A, Kim, J, Koci, B, Köpke, L, Kühn, K, Lamoureux, J I, Leich, H, Leuthold, M, Lindahl, P, Madsen, J, Marciniewski, P, Matis, H S, Minaeva, Y, Miocinovic, P, Morse, R, Neunhoffer, T, Niessen, P, Nygren, D R, Ogelman, H, Olbrechts, P, Perez de los Heros, C, Pohl, A, Price, P B, Przybylski, G T, Rawlins, K, Reed, C, Rhode, W, Ribordy, M, Richter, S, Martino, J R, Romenesko, P, Ross, D, Sander, H G, Schmidt, T, Schneider, D, Silvestri, A, Solarz, M, Spiczak, G M, Spiering, C, Starinsky, N, Steele, D, Steffen, P, Stokstad, R G, Sudhoff, P, Sulanke, K H, Taboada, I, Donckt, M V, Walck, C, Weinheimer, C, Wiebusch, C H, Wischnewski, R, Wissing, H, Woschnagg, K, Yodh, G, Young, S“…In the winter season of 2000, the AMANDA (Antarctic Muon And Neutrino Detector Array) detector was completed to its final state. …”
Publicado 2001
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1947“…We have studied the most general neutrino mass matrices in models with SU(2) and SU(3) horizontal symmetries. …”
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1948por Benussi, L, Bruski, N, D'Ambrosio, N, Déclais, Y, Dupraz, J P, Fabre, Jean-Paul, Fanti, V, Forton, E, Frekers, D, Frenkel, A, Girerd, C, Golovkin, S V, Grégoire, G, Harrison, K, Jonkmans, G, Jonsson, P, Katsanevas, S, Kreslo, I, Marteau, J, Martellotti, G, Martínez, S, Medvedkov, A M, Moret, G, Niwa, K, Novikov, V, Van Beek, G, Penso, G, Vasilchenko, V G, Vuilleumier, J L, Wilquet, G, Zucchelli, P“…Results are given on tests of large particle trackers for the detection of neutrino interactions in long-baseline experiments. …”
Publicado 2002
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1949
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1950
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1951
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1954
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1955por Williams, J M“…This poster session explains three theoretical shortcomings of the usual neutrino oscillation theory and illustrates that theory's empirical weakness. …”
Publicado 2002
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1956por Sievers, P“…As production target for Neutrino Factories,free mercury jets with high axial velocity of about 20 m /s are being studied.For the CERN-Neutrino- Factory proposal with a 4 MW beam power,but with a relatively large beam size at 2 .2 GeV /c and pulsed at 50 Hz ,maximum energy deposition densities of below 20 J /g and average power densities of about 1 kW /g are expected in the target.Therefore a study has been made which discusses the feasibility and limits of a stationary target.It is proposed to use densely packed solid spheres of heavy material and with diameters in the millimeter range.These spheres are con fined inside a Titanium container and cooled by an e fficient water circuit or possibly by He-gas.Dynamic response,as pressure pulses and vibrations are greatly reduced in the small target granules due to relatively long beam bursts,each with a duration of 3.3 s .The encouraging results achieved in this assessment justify to pursue further experimental tests,in particular of the cooling of the target,its lifetime under repetitive thermal cycles (4.3 Mio/day) and of radiation damage,to validate this proposal.It is expected that the lifetime of this target will be adequate for the operation of the CERN- Neutrino-Factory,at least over its initial phase below 4 MW beam power.…”
Publicado 2001
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1957
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