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3201por Beck, D, Blaum, K, Block, M, Boehm, Ch, Borgmann, Ch, Breitenfeldt, M, Eliseev, S, Fedoseev, V, George, S, Herfurth, F, Herlert, A, Kluge, H -J, Kowalska, M, Kreim, S, Lunney, D, Manea, V, Naimi, S, Neidherr, D, Novikov, Yu N, Rosenbusch, M, Schwarz, S, Schweikhard, L, Seliverstov, M, Sokolov, A, Stanja, J, Wienholtz, F, Wolf, R N, Zuber, KEnlace del recurso
Publicado 2011
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3202por Alicki, Robert“…It is argued that the recently reported "superluminal neutrinos" could be accounted for a purely statistical effect due to the fact that only a very small fraction of initial protons is transformed into finally observed neutrinos. …”
Publicado 2011
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3203“…Recent data from the OPERA experiment seem to point to neutrinos propagating faster than light. One possible physics explanation for such a result is the existence of light sterile neutrinos which can propagate in a higher dimensional bulk and achieve apparent superluminal velocities when measured by an observer confined to the 4D brane of the standard model. …”
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3204por Bergsma, F, Dorenbosch, Jheroen, Jonker, M, Nieuwenhuis, C, Udo, Fred, Allaby, James V, Amaldi, Ugo, Barbiellini, Guido, Barone, L, Busi, C, Capone, A, Flegel, Wilfried, Metcalf, M, Panman, J, Winter, Klaus, Aspiazu, J, Büsser, F W, Daumann, H, Gall, P D, Metz, E, Niebergall, F, Ranitzsch, K H, Stähelin, P, Gorbunov, P, Grigoriev, E A, Kaftanov, V S, Khovanskii, V D, Rosanov, A, Baroncelli, A, Borgia, B, Bosio, C, Ferroni, F, Longo, E, Monacelli, P, De Notaristefani, F, Pistilli, P, Santoni, C, Tortora, L, Valente, VEnlace del recurso
Publicado 1982
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3205por Bolshakova, A., Boyko, I., Chelkov, G., Dedovitch, D., Elagin, A., Emelyanov, D., Gostkin, M., Guskov, A., Kroumchtein, Z., Nefedov, Yu., Nikolaev, K., Zhemchugov, A., Dydak, F., Wotschack, J., De Min, A., Ammosov, V., Gapienko, V., Koreshev, V., Semak, A., Sviridov, Yu., Usenko, E., Zaets, V.Enlace del recurso
Publicado 2011
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3206por Ellis, John, Janka, Hans-Thomas, Mavromatos, Nikolaos E., Sakharov, Alexander S., Sarkisyan, Edward K.G.“…We discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as suggested by recent two-dimensional simulations. …”
Publicado 2012
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3207por Jonker, M, Udo, Fred, Allaby, James V, Amaldi, Ugo, Barbiellini, Guido, Capone, A, Flegel, Wilfried, Kozanecki, Witold, Mess, K H, Metcalf, M, Meyer, J, Orr, R S, Panman, J, Wetherell, Alan M, Winter, Klaus, Blobel, Volker, Büsser, F W, Gall, P D, Grote, H, Kröger, B J, Metz, E, Niebergall, F, Ranitzsch, K H, Stähelin, P, Gorbunov, P, Grigoriev, E A, Kaftanov, V S, Khovanskii, V D, Rozanov, A N, Baroncelli, A, Borgia, B, Bosio, C, Ferroni, F, Longo, E, Monacelli, P, De Notaristefani, F, Pistilli, P, Santoni, C, Valente, VEnlace del recurso
Publicado 1983
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3208
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3209
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3210
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3211por Allasia, D, Angelini, C, Baldini, A, Baldo-Ceolin, Massimilla, Barlag, S, Bertanza, L, Bigi, A, Bisi, V, Bobisut, F, Bolognese, T, Borg, A, Calimani, E, Capiluppi, P, Casali, R, Ciampolillo, S, Derkaoui, J E, Faccini-Turluer, M L, Fantechi, R, Flaminio, Vincenzo, Frodesen, A G, Gamba, D, Giacomelli, G, Halsteinslid, A, Hornaes, A, Huzita, H, Jongejans, B, Lippi, I, Loreti, M, Louedec, C, Mandrioli, G, Marzari-Chiesa, A, Nappi, A, Pazzi, R, Pierazzini, G M, Riccati, L, Romero, A, Rossi, A M, Serra-Lugaresi, P, Tenner, A, van Apeldoorn, G W, van Dam, P, Vignaud, D, Visser, C, Wigmans, REnlace del recurso
Publicado 1983
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3212por Agafonova, N.Yu., Aglietta, M., Antonioli, P., Ashikhmin, V.V., Bari, G., Bertoni, R., Bressan, E., Bruno, G., Dadykin, V.L., Fulgione, W., Galeotti, P., Garbini, M., Ghia, P.L., Giusti, P., Kemp, E., Mal'gin, A.S., Miguez, B., Molinario, A., Persiani, R., Pless, I.A., Ryasny, V.G., Ryazhskaya, O.G., Saavedra, O., Sartorelli, G., Shakyrianova, I.R., Selvi, M., Trinchero, G.C., Vigorito, C., Yakushev, V.F., Zichichi, A., Razeto, A.“…We report the measurement of the time-of-flight of ~17 GeV muon neutrinos on the CNGS baseline (732 km) with the Large Volume Detector (LVD) at the Gran Sasso Laboratory. …”
Publicado 2012
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3213
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3214por Battistoni, G, Bellotti, E, Bologna, G, Campana, P, Castagnoli, C, Chiarella, V, Ciocio, A, Cundy, Donald C, D'Ettorre-Piazzoli, B, Fiorini, Ettore, Galeotti, P, Iarocci, Enzo, Liguori, C, Mannocchi, G, Murtas, G P, Negri, P, Nicoletti, G, Picchi, P, Price, M, Pullia, Antonio, Ragazzi, S, Rollier, M, Saavedra, O, Satta, L, Trasatti, L, Zanotti, LEnlace del recurso
Publicado 1983
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3215por Antonello, M, Baibussinov, B, Benetti, P, Calligarich, E, Canci, N, Centro, S, Cesana, A, Cieslik, K, Cline, D B, Cocco, A G, Dabrowska, A, Dequal, D, Dermenev, A, Dolfini, R, Farnese, C, Fava, A, Ferrari, A, Fiorillo, G, Gibin, D, Gninenko, S, Guglielmi, A, Haranczyk, M, Holeczek, J, Ivashkin, A, Kisiel, J, Kochanek, I, Lagoda, J, Mania, S, Menegolli, A, Meng, G, Montanari, C, Otwinowski, S, Piazzoli, A, Picchi, P, Pietropaolo, F, Plonski, P, Rappoldi, A, Raselli, G L, Rossella, M, Rubbia, C, Sala, P, Scantamburlo, E, Scaramelli, A, Segreto, E, Sergiampietri, F, Stefan, D, Stepaniak, J, Sulej, R, Szarska, M, Terrani, M, Varanini, F, Ventura, S, Vignoli, C, Wang, H, Yang, X, Zalewska, A, Zaremba, K“…This is compared with the small but significant backgrounds due to conventional neutrino sources. The ionization along the early part of e.m. showers, has been examined wire by wire to tag the presence of an electron emitted from the vertex of the neutrino event. …”
Publicado 2012
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3216
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3217“…We present FLUKA and MARS simulation studies of the pion production and energy deposition in the Neutrino Factory baseline target station, which consists of a 4 MW proton beam interacting with a liquid mercury jet target within a 20 T solenoidal magnetic field. …”
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3218por BIAGI, S“…The first search for neutrinos from the Fermi Bubbles is presented using data collected by the ANTARES telescope. …”
Publicado 2012
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3219
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3220