Results 1 to 10 of about 20,410 (109)
Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy [PDF]
Astroparticle Physics, 2010 14 pages, 7 ...Abbasi, R., Abdou, Y., Ackermann, Markus, Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, Mark D., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K.-H., Benabderrahmane, M. L., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bissok, M., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Böser, S., Botner, O., Bradley, L., Braun, J., Breder, D., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cohen, S., Cowen, D. F., d'Agostino, M. V., Danninger, M., Day, C. T., de Clercq, C., Demirörs, L., Depaepe, O., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Feusels, T., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Ganugapati, R., Gerhardt, L., Gladstone, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Grant, D., Griesel, T., Gross, A., Grullon, S., Gunasingha, R. M., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hasegawa, Y., Heise, J., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Hoshina, K., Hubert, D., Huelsnitz, W., Hülss, J.-P., Hulth, P. O., Hultqvist, K., Hussain, S., Imlay, R. L., Inaba, M., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Joseph, J. M., Kampert, K.-H., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Klepser, S., Knops, S., Kohnen, G., Kolanoski, H., Köpke, L., Kowalski, M., Kowarik, T., Krasberg, M., Kuehn, K., Kuwabara, T., Labare, M., Lafebre, S., Laihem, K., Landsman, H., Lauer, R., Leich, H., Lennarz, D., Lucke, A., Lundberg, J., Lünemann, J., Madsen, Jens, Majumdar, P., Maruyama, R., Mase, K., Matis, H. S., Mcparland, C. P., Meagher, K., Merck, M., Mészáros, P., Middell, E., Milke, N., Miyamoto, H., Mohr, A., Montaruli, T., Morse, R., Movit, S. M., Münich, K., Nahnhauer, R., Nam, J. W., Niessen, P., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., Ono, M., Panknin, S., Patton, S., Pérez de Los Heros, C., Petrovic, J., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Potthoff, N., Price, P. B., Prikockis, M., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Rodrigues, J. P., Roth, P., Rothmaier, F., Rott, C., Roucelle, C., Rutledge, D., Ryckbosch, D., Sander, H.-G., Sarkar, S., Satalecka, K., Schlenstedt, S., Schmidt, T., Schneider, D., Schukraft, A., Schulz, O., Schunck, M., Seckel, D., Spiczak, G. M., Taboada, I., Ter-Antonyan, S., Wiebusch, C. H., Wiedemann, A., Yoshida, S. +205 more +13 more sourcesMeasurement of CNGS muon neutrino speed with Borexino [PDF]
Physics Letters B, 2012 We have measured the speed of muon neutrinos with the Borexino detector using short-bunch CNGS beams. The final result for the difference in time-of-flight between a =17 GeV muon neutrino and a particle moving at the speed of light in vacuum is t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with zero.Alvarez Sanchez, P., Barzaghi, R., Bellini, G., Benziger, J., Betti, B., Biagi, L., Bick, D., Bonfini, G., Bravo, D., Buizza-Avanzini, M., Caccianiga, B., Cadonati, L., Carraro, C., Cavalcante, P., Cerretto, G., Chavarria, A., d'Angelo, D., Davini, S., de Gaetani, C., Derbin, A., Etenko, A., Esteban, H., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, Aldo, Ianni, Andrea, Jones, M., Kayunov, A., Kobychev, V., Korablev, D., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Lewke, T., Litvinovich, E., Loer, B., Lombardi, P., Lombardi, F., Ludhova, L., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Missiaen, D., Montanari, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Passoni, D., Pinto, L., Perasso, L., Perasso, S., Pettiti, V., Plantard, C., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Sabelnikov, A., Saldanha, R., Salvo, C., Schönert, S., Serrano, J., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Spinnato, P., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Visconti, M. G., Vogelaar, R. B., von Feilitzsch, F., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., Zuzel, G. +105 moreopenaire +11 more sourcesPrecision measurement of the speed of propagation of neutrinos using the MINOS detectors
Physical Review D, 2015 10 pages, six figures, after refereeing re-submitted to ...Adamson, P, Anghel, I, Ashby, N, Aurisano, A, Barr, G, Bishai, M, Blake, A, Bock, GJ, Bogert, D, Bumgarner, R, Cao, SV, Castromonte, CM, Childress, S, Coelho, JAB, Corwin, L, Cronin-Hennessy, D, de Jong, JK, Devan, AV, Devenish, NE, Diwan, MV, Escobar, CO, Evans, JJ, Falk, E, Feldman, GJ, Fonville, B, Frohne, MV, Gallagher, HR, Gomes, RA, Goodman, MC, Gouffon, P, Graf, N, Gran, R, Grzelak, K, Habig, A, Hahn, SR, Hartnell, J, Hatcher, R, Hirschauer, J, Holin, A, Huang, J, Hylen, J, Irwin, GM, Isvan, Z, James, C, Jefferts, SR, Jensen, D, Kafka, T, Kasahara, SMS, Koizumi, G, Kordosky, M, Kreymer, A, Lang, K, Ling, J, Litchfield, PJ, Lucas, P, Mann, WA, Marshak, ML, Matsakis, D, Mayer, N, McKinley, A, McGivern, C, Medeiros, MM, Mehdiyev, R, Meier, JR, Messier, MD, Miller, WH, Mishra, SR, Mitchell, S, Sher, SM, Moore, CD, Mualem, L, Musser, J, Naples, D, Nelson, JK, Newman, HB, Nichol, RJ, Nowak, JA, O'Connor, J, Orchanian, M, Pahlka, RB, Paley, J, Parker, TE, Patterson, RB, Pawloski, G, Perch, A, Phan-Budd, S, Plunkett, RK, Poonthottathil, N, Powers, E, Qiu, X, Radovic, A, Rebel, B, Ridl, K, Roemisch, S, Rosenfeld, C, Rubin, HA, Sanchez, MC, Schneps, J, Schreckenberger, A, Schreiner, P, Sharma, R, Sousa, A, Tagg, N, Talaga, RL, Thomas, J, Thomson, MA, Tian, X, Timmons, A, Tognini, SC, Toner, R, Torretta, D, Urheim, J, Vahle, P, Viren, B, Weber, A, Webb, RC, White, C, Whitehead, L, Whitehead, LH, Wojcicki, SG, Wright, J, Zhang, V, Zwaska, R +122 more +11 more sourcesNeutrino interactions in the late universe
Journal of High Energy Physics, 2021 The cosmic neutrino background is both a dramatic prediction of the hot Big Bang and a compelling target for current and future observations. The impact of relativistic neutrinos in the early universe has been observed at high significance in a number of Daniel Green, David E. Kaplan, Surjeet Rajendran +2 moredoaj +1 more source