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2361
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2362por Valerius, Kathrin“…--HTML--><p><span><span><span>Precision measurements of the kinematics of weak decays offer a direct and nearly model independent approach to probe the absolute neutrino mass scale. The KArlsruhe TRItium Neutrino experiment (KATRIN) is searching for the minute imprint of the neutrino mass in the endpoint region of the tritium beta-decay spectrum. …”
Publicado 2021
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2363
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2364por Charitonidis, Nikolaos, Longhin, Andrea, Pari, Michelangelo, Parozzi, Elisabetta Giulia, Terranova, Francesco“…Neutrino oscillation physics has entered a new precision era, which poses major challenges to the level of control and diagnostics of the neutrino beams. …”
Publicado 2021
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2365por Kotera, Kumiko“…The GRAND project aims to detect ultra-high-energy neutrinos, cosmic rays and gamma rays, with an array of $200,000$ radio antennas over $200,000\,{\rm km}^2$, split into $\sim 20$ sub-arrays of $\sim 10,000\,{\rm km}^2$ deployed worldwide. …”
Publicado 2021
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2366“…We consider a class of models predicting new heavy neutral fermionic states, whose mixing with the light neutrinos can be naturally significant and produce observable effects below the threshold for their production. …”
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2367por Jacoby, Konstantin Andreas“…This study investigates the fluid flow and heat transfer due to forced and natural convection within the CERN ProtoDUNE single phase Neutrino Detector. "The CERN ProtoDUNE single phase Neutrino Detector is designed as a test bed and full-scale prototype for the elements of the first far detector module of the DUNE"\cite{CERN_Document}. …”
Publicado 2021
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2368por Bustamante, Mauricio“…Notable examples include precision tests using the flavor composition of the neutrino flux, new neutrino-neutrino interactions, and measuring the neutrino-nucleon cross section. …”
Publicado 2021
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2369
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2370por Harz, Julia“…<!--HTML--><p>With neutrino oscillations pointing us towards massive neutrinos, they are a clear hint towards physics beyond the standard model. …”
Publicado 2021
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2371por Khachatryan, M, Papadopoulou, A, Ashkenazi, A, Hauenstein, F, Nambrath, A, Hrnjic, A, Weinstein, L B, Hen, O, Piasetzky, E, Betancourt, M, Dytman, S, Mahn, K, Coloma, P, Adhikari, S, Amaryan, M J, Angelini, Giovanni, Atac, H, Barion, L, Battaglieri, M, Bedlinskiy, I, Beck, A, Benmokhtar, F, Bianconi, A, Biselli, A S, Bossu, F, Boiarinov, S, Briscoe, W J, Brooks, W K, Bulumulla, D, Burkert, V D, Carman, D S, Carvajal, J C, Celentano, A, Chatagnon, P, Chesnokov, V, Chetry, T, Ciullo, G, Clark, L, Clary, B A, Cohen, E O, Cole, P L, Contalbrigo, M, Crede, V, Cruz-Torres, R, D’Angelo, A, Dashyan, N, De Vita, R, Defurne, M, Denniston, A, Deur, A, Diehl, S, Djalali, C, Duer, M, Dupre, R, Egiyan, H, Ehrhart, M, El Alaoui, A, El Fassi, L, Elouadrhiri, L, Eugenio, P, Fersch, R, Filippi, A, Forest, T A, Gavalian, G, Gilfoyle, G P, Giovanetti, K L, Girod, F X, Glazier, D I, Golovatch, E, Gothe, R W, Griffioen, K A, Guidal, M, Guo, L, Hakobyan, H, Hattawy, M, Hayward, T B, Heddle, D, Hicks, K, Hobart, A, Holtrop, M, Ilieva, Y, Ireland, D G, Ishkhanov, B S, Isupov, E L, Jo, H S, Joo, K, Keller, D, Khanal, A, Khandaker, M, Kim, C W, Kim, W, Korover, I, Kubarovsky, V, Kuhn, S E, Lanza, L, Leali, M, Lenisa, P, Livingston, K, MacGregor, I J D, Marchand, D, Markov, N, Marsicano, L, Mascagna, V, McKinnon, B, May-Tal Beck, S, Mineeva, T, Mirazita, M, Mokeev, V, Movsisyan, A, Munoz Camacho, C, Nadel-Turonski, P, Neupane, K, Niccolai, S, Niculescu, G, Osipenko, M, Ostrovidov, A I, Paolone, M, Pappalardo, L L, Paremuzyan, R, Park, K, Pasyuk, E, Pogorelko, O, Poudel, J, Prok, Y, Protopopescu, D, Pybus, J, Ripani, M, Raue, B, Ritman, J, Rizzo, A, Rosner, G, Rossi, P, Sabati, F, Salgado, C, Schmidt, A, Schumacher, R A, Segarra, E P, Sharabian, Y G, Shrestha, U, Skorodumina, Iu, Sokhan, D, Soto, O, Sparveris, N, Stepanyan, S, Strakovsky, I I, Strauch, S, Tyler, N, Tyson, R, Ungaro, M, Venturelli, L, Voskanyan, H, Voutier, E, Watts, D, Wei, X, Wood, M H, Zachariou, N, Zhang, J, Zhao, Z W, Dolan, S, Megias, G D, Gardiner, S“…Neutrinos exist in one of three types or ‘flavours’—electron, muon and tau neutrinos—and oscillate from one flavour to another when propagating through space. …”
Publicado 2021
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2372por Ariga, Tomoko“…In addition to searches for new particles, we also aim to study high-energy neutrinos of all flavors, as there is a huge flux of neutrinos at this location. …”
Publicado 2019
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2373
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2374por Huber, Patrick“…An overview of the physics of how neutrinos are generated in reactors and how we can compute neutrino fluxes will follow. …”
Publicado 2022
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2375
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2376por Brice, Maximilien“…The experiment SND@LHC, or Scattering and Neutrino Detector at the LHC, is the facility’s ninth experiment and is complementary to FASER$v$, a neutrino subdetector of the FASER experiment, which has been installed in the LHC tunnel. …”
Publicado 2022
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2377por Gerbino, Martina, Grohs, Evan, Lattanzi, Massimiliano, Abazajian, Kevork N., Blinov, Nikita, Brinckmann, Thejs, Chen, Mu-Chun, Djurcic, Zelimir, Du, Peizhi, Escudero, Miguel, Hagstotz, Steffen, Kelly, Kevin J., Lorenz, Christiane S., Loverde, Marilena, Martínez-Miravé, Pablo, Mena, Olga, Meyers, Joel, Pettus, Walter C., Saviano, Ninetta, Suliga, Anna M., Takhistov, Volodymyr, Tórtola, Mariam, Valle, José W.F., Wallisch, Benjamin“…The intersection of the cosmic and neutrino frontiers is a rich field where much discovery space still remains. …”
Publicado 2022
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2378por Adams, D.Q., Alduino, C., Alfonso, K., Avignone, III F.T., Azzolini, O., Bari, G., Bellini, F., Benato, G., Beretta, M., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., Camilleri, J., Caminata, A., Campani, A., Canonica, L., Cao, X.G., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Celi, E., Chiesa, D., Clemenza, M., Copello, S., Cremonesi, O., Creswick, R.J., D'Addabbo, A., Dafinei, I., Dell'Oro, S., Di Domizio, S., Dompè, V., Fang, D.Q., Fantini, G., Faverzani, M., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M.A., Freedman, S.J., Fu, S.H., Fujikawa, B.K., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gutierrez, T.D., Han, K., Hansen, E.V., Heeger, K.M., Huang, R.G., Huang, H.Z., Johnston, J., Keppel, G., Kolomensky, Yu. G., Ligi, C., Liu, R., Ma, L., Ma, Y.G., Marini, L., Maruyama, R.H., Mayer, D., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nastasi, M., Nikkel, J., Nones, C., Norman, E.B., Nucciotti, A., Nutini, I., O'Donnell, T., Ouellet, J.L., Pagan, S., Pagliarone, C.E., Pagnanini, L., Pallavicini, M., Pattavina, L., Pavan, M., Pessina, G., Pettinacci, V., Pira, C., Pirro, S., Pozzi, S., Previtali, E., Puiu, A., Rosenfeld, C., Rusconi, C., Sakai, M., Sangiorgio, S., Schmidt, B., Scielzo, N.D., Sharma, V., Singh, V., Sisti, M., Speller, D., Surukuchi, P.T., Taffarello, L., Terranova, F., Tomei, C., Vetter, K.J., Vignati, M., Wagaarachchi, S.L., Wang, B.S., Welliver, B., Wilson, J., Wilson, K., Winslow, L.A., Zimmermann, S., Zucchelli, S.Enlace del recurso
Publicado 2021
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2379
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2380