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3481
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3482por Parozzi, E, Acerbi, F, Ballerini, G, Bonesini, M, Branca, A, Brizzolari, C, Brunetti, G, Calviani, M, Carturan, S, Catanesi, M G, Cecchini, S, Cindolo, F, Collazuol, G, Conti, E, Dal Corso, F, De Rosa, G, Delogu, C, Falcone, A, Goddard, B, Gola, A, Intonti, R A, Jollet, C, Kain, V, Klicek, B, Kudenko, Y, Laveder, M, Longhin, A, Ludovici, L, Magaletti, L, Mandrioli, G, Margotti, A, Mascagna, V, Mauri, N, Meregaglia, A, Mezzetto, M, Nessi, M, Paoloni, A, Pari, M, Pasqualini, L, Paternoster, G, Patrizii, L, Piemonte, C, Pozzato, M, Pupilli, F, Prest, M, Radicioni, E, Riccio, C, Ruggeri, A C, Sirri, G, Soldani, M, Stipcevic, M, Tenti, M, Terranova, F, Torti, M, Vallazza, E, Velotti, F, Vesco, M, Votano, L“…The ENUBET ERC project (2016–2021) is studying a narrow band neutrino beam where lepton production can be monitored at single particle level. …”
Publicado 2020
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3483por Pestel, V“…The SoLid experiment is currently taking physics data close to the BR2 reactor core at SCK·CEN, Belgium, exploring very short baseline anti-neutrino oscillations. It aims to resolve the reactor anti-neutrino anomaly by measuring both anti-neutrino rate and energy spectrum. …”
Publicado 2019
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3484por Brizzolari, C, Acerbi, F, Ballerini, G, Berra, A, Bonesini, M, Branca, A, Brunetti, G, Calviani, M, Capelli, S, Carturan, S, Catanesi, M G, Cecchini, S, Charitonidis, N, Cindolo, F, Collazuol, G, Conti, E, Dal Corso, F, Delogu, C, De Rosa, G, Falcone, A, Gola, A, Intonti, R A, Jollet, C, Kain, V, Klicek, B, Kudenko, Y, Laveder, M, Longhin, A, Ludovici, L, Lutsenko, E, Magaletti, L, Mandrioli, G, Margotti, A, Mascagna, V, Mauri, N, Meazza, L, Meregaglia, A, Mezzetto, M, Nessi, M, Paoloni, A, Pari, M, Parozzi, E, Pasqualini, L, Paternoster, G, Patrizii, L, Pozzato, M, Prest, M, Pupilli, F, Radicioni, E, Riccio, C, Ruggieri, A C, Scian, C, Sirri, G, Soldani, M, Stipcevic, M, Tenti, M, Terranova, F, Torti, M, Vallazza, E, Velotti, F, Vesco, M, Votano, L“…The knowledge of initial flux, energy and flavour of current neutrino beams is currently the main limitation for a precise measurement of neutrino crosssections. …”
Publicado 2020
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3485por Brunetti, G, Acerbi, F, Ballerini, G, Bonesini, M, Branca, A, Brizzolari, C, Capelli, S, Carturan, S, Catanesi, M G, Cecchini, S, Charitonidis, N, Cindolo, F, Collazuol, G, Conti, E, Dal Corso, F, Delogu, C, De Rosa, G, Falcone, A, Goddard, B, Gola, A, Jollet, C, Kain, V, Klicek, B, Kudenko, Y, Laveder, M, Longhin, A, Ludovici, L, Lutsenko, E, Magaletti, L, Mandrioli, G, Margotti, A, Mascagna, V, Mauri, N, Meazza, L, Meregaglia, A, Mezzetto, M, Paoloni, A, Pari, M, Parozzi, E, Pasqualini, L, Paternoster, G, Patrizii, L, Pozzato, M, Prest, M, Pupilli, F, Radicioni, E, Riccio, C, Ruggieri, A C, Scian, C, Sirri, G, Soldani, M, Stipcevic, M, Tenti, M, Terranova, F, Torti, M, Vallazza, E, Velotti, F, Vesco, M, Votano, L“…The knowledge of initial flux, energy and flavor of neutrino beams is currently the main limitation for a precise measurement of neutrino cross sections. …”
Publicado 2020
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3486por Torti, M, Acerbi, F, Berra, A, Bonesini, M, Branca, A, Brizzolari, C, Brunetti, G, Calviani, M, Capelli, S, Carturan, S, Catanesi, M G, Charitonidis, N, Cecchini, S, Cindolo, F, Collazuol, G, Conti, E, Dal Corso, F, Delogu, C, De Rosa, G, Falcone, A, Gola, A, Jollet, C, Kain, V, Klićek, B, Kudenko, Y, Laveder, M, Longhin, A, Ludovici, L, Lutsenko, E, Magaletti, L, Mandrioli, G, Margotti, A, Mascagna, V, Mauri, N, Meazza, L, Meregaglia, A, Mezzetto, M, Nessi, M, Paoloni, A, Pari, M, Parozzi, E G, Pasqualini, L, Paternoster, G, Patrizii, L, Pozzato, M, Prest, M, Pupilli, F, Radicioni, E, Riccio, C, Ruggeri, A C, Scian, C, Sirri, G, Stipćevic, M, Tenti, M, Terranova, F, Vallazza, E, Velotti, F, Vesco, M, Votano, L“…The knowledge of the initial flux, energy and flavor of current neutrino beams is the main limitation for a precise measurement of neutrino cross-sections. …”
Publicado 2020
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3487
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3488
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3489
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3490“…We discuss leptogenesis in a model with heavy right-handed Majorana neutrinos propagating in a constant but otherwise generic CPT-violating axial time-like background (motivated by string theory). …”
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3491“…We introduce a novel effective electromagnetic interaction between sterile neutrinos and SM neutrinos, which can successfully explain the XENON1T event rate through inelastic scattering of the sterile neutrino dark matter from Xenon electrons. …”
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3492por Laha, Ranjan“…We derive stringent constraints on neutrino speed, weak equivalence principle violation, Lorentz invariance violation, and dual lensing from the first high-energy astrophysical neutrino source: TXS 0506+056. …”
Publicado 2018
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3493por de Kerret, H, Kryn, D, Lefievre, B, Obolensky, M, Sukhotin, S, Coutry, P, Marchand, D, Steinberg, R, Lane, C E, Wang, F C, Martemyanov, V P, Mikaelyan, L A, Skorokhvatov, M D, Vyrodov, V N, Declais, Y, Favier, J, Oriboni, A, Greenwood, Z D, Kropp, W R, Price, L, Riley, S, Sobel, H, Dieterle, B B, Reeder, REnlace del recurso
Publicado 1993
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3494por Alsharoa, Mohammad M., Ankenbrandt, Charles M., Atac, Muzaffer, Autin, Bruno R., Balbekov, Valeri I., Barger, Vernon D., Benary, Odette, Bennett, J.Roger J., Berger, Michael S., Berg, J.Scott, Berz, Martin, Black, Edgar L., Blondel, Alain, Bogacz, S.Alex, Bonesini, M., Bracker, Stephen B., Bross, Alan D., Bruno, Luca, Buckley-Geer, Elizabeth J., Caldwell, Allen C., Campanelli, Mario, Cassel, Kevin W., Catanesi, M.Gabriela, Chattopadhyay, Swapan, Chou, Weiren, Cline, David B., Coney, Linda R., Conrad, Janet M., Corlett, John N., Cremaldi, Lucien, Cummings, Mary Anne, Darve, Christine, DeJongh, Fritz, Drozhdin, Alexandr, Drumm, Paul, Elvira, V.Daniel, Errede, Deborah, Fabich, Adrian, Fawley, William M., Fernow, Richard C., Ferrario, Massimo, Finley, David A., Fisch, Nathaniel J., Fukui, Yasuo, Furman, Miguel A., Gabriel, Tony A., Galea, Raphael, Gallardo, Juan C., Garoby, Roland, Garren, Alper A., Geer, Stephen H., Gilardoni, Simone, Van Ginneken, Andreas J., Ginzburg, Ilya F., Godang, Romulus, Goodman, Maury, Gosz, Michael R., Green, Michael A., Gruber, Peter, Gunion, John F., Gupta, Ramesh, Haines, John R., Hanke, Klaus, Hanson, Gail G., Han, Tao, Haney, Michael, Hartill, Don, Hartline, Robert E., Haseroth, Helmut D., Hassanein, Ahmed, Hoffman, Kara, Holtkamp, Norbert, Holzer, E.Barbara, Johnson, Colin, Johnson, Rolland P., Johnstone, Carol, Jungmann, Klaus, Kahn, Stephen A., Kaplan, Daniel M., Keil, Eberhard K., Kim, Eun-San, Kim, Kwang-Je, King, Bruce J., Kirk, Harold G., Kuno, Yoshitaka, Ladran, Tony S., Lau, Wing W., Learned, John G., Lebedev, Valeri, Lebrun, Paul, Lee, Kevin, Lettry, Jacques A., Laveder, Marco, Li, Derun, Lombardi, Alessandra, Lu, Changguo, Makino, Kyoko, Malkin, Vladimir, Marfatia, D., McDonald, Kirk T., Mezzetto, Mauro, Miller, John R., Mills, Frederick E., Mocioiu, I., Mokhov, Nikolai V., Monroe, Jocelyn, Moretti, Alfred, Mori, Yoshiharu, Neuffer, David V., Ng, King-Yuen, Norem, James H., Onel, Yasar, Oreglia, Mark, Ozaki, Satoshi, Padamsee, Hasan, Pakvasa, Sandip, Palmer, Robert B., Parker, Brett, Parsa, Zohreh, Penn, Gregory, Pischalnikov, Yuriy, Popovic, Milorad B., Qian, Zubao, Radicioni, Emilio, Raja, Rajendran, Ravn, Helge L., Reed, Claude B., Reginato, Louis L., Rehak, Pavel, Rimmer, Robert A., Roberts, Thomas J., Roser, Thomas, Rossmanith, Robert, Samulyak, Roman V., Scanlan, Ronald M., Schlenstedt, Stefan, Schwandt, Peter, Sessler, Andrew M., Shaevitz, Michael H., Shrock, Robert, Sievers, Peter, Silvestrov, Gregory I., Simos, Nick, Skrinsky, Alexander N., Solomey, Nickolas, Spampinato, Philip T., Spentzouris, Panagiotis, Stefanski, R., Stoltz, Peter, Stumer, Iuliu, Summers, Donald J., Teng, Lee C., Thieberger, Peter A., Tigner, Maury, Todosow, Michael, Tollestrup, Alvin V., Torun, Yagmur, Trbojevic, Dejan, Usubov, Zafar U., Vsevolozhskaya, Tatiana A., Wah, Yau, Wang, Chun-xi, Wang, Haipeng, Weggel, Robert J., Whisnant, K., Willen, Erich H., Wilson, Edmund J.N., Winn, David R., Wurtele, Jonathan S., Wu, Vincent, Yokoi, Takeichiro, Yoon, Moohyun, York, Richard, Yu, Simon, Zeller, Al, Zhao, Yongxiang, Zisman, Michael S.“…We summarize the physics that can be done with neutrino factories as well as with intense cold beams of muons. …”
Publicado 2002
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3495“…We study the possible magnitudes of CP and lepton-number-violating quantities in specific GUT models of massive neutrinos with different Abelian flavour groups, taking into account experimental constraints and requiring successful leptogenesis. …”
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3496“…A proposal for a new system to capture signals in the Optical Module (OM) of an Underwater Neutrino Telescope is described. It concentrates on the problem of power consumption in relation to precision. …”
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3497“…Recently it has been shown that string instanton effects may give rise to neutrino Majorana masses in certain classes of semi-realistic string compactifications. …”
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3498“…The CERN Neutrino to Gran Sasso (CNGS) experiment uses 400GeV protons extracted from the SPS, which travel along 825 meters of beam line before reaching the CNGS target. …”
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3499
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3500