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3001“…We present a review of cosmological nucleosynthesis (CN) with neutrino oscillations, discussing the different effects of oscillations on CN, namely: increase of the effective degrees of freedom during CN, spectrum distortion of the oscillating neutrinos, neutrino number density depletion, and growth of neutrino-antineutrino asymmetry due to active-sterile oscillations. …”
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3002por Kachelriess, M“…After briefly reviewing the proposal that the decay products from UHE neutrinos annihilations on relic neutrinos are the observed UHE primaries, we concentrate on the suggestion that UHE neutrinos can acquire cross-sections approaching hadronic size if the string scale is as low as approximately=10 TeV. …”
Publicado 2001
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3003“…We estimate how well we will know the parameters of solar neutrino oscillations after KamLAND and Borexino. The expected error on Delta m^2 is few per-mille in the VO and QVO regions, few per-cent in the LMA region, and around 10% in the LOW region. …”
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3004por Aysto, J., Baldini, A., Blondel, A., de Gouvea, A., Ellis, J., Fetscher, W., Giudice, G.F., Jungmann, K., Lola, S., Palladino, V., Tobe, K., Vacchi, A., van der Schaaf, A., Zuber, K.“…Such a source is a necessary stage towards building the neutrino factories and muon colliders which are being considered at present. …”
Publicado 2001
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3005
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3006“…This is particularly important because at these energies $\nutau$ is a significant fraction of the expected astrophysical neutrino flux, and only a tiny portion of the atmospheric neutrino flux.…”
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3007por Kayis-Topaksu, A, Onengüt, G, Van Dantzig, R, De Jong, M, Melzer, O, Oldeman, R G C, Pesen, E, Visschers, J L, Güler, M, Serin-Zeyrek, M, Sever, R, Tolun, P, Zeyrek, M T, Armenise, N, Catanesi, M G, De Serio, M, Ieva, M, Muciaccia, M T, Radicioni, E, Simone, S, Bülte, A, Winter, Klaus, El-Aidi, R, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, S A, Chizhov, M V, Doucet, M, Kolev, D, Meinhard, H, Panman, J, Papadopoulos, I M, Ricciardi, S, Rozanov, A N, Tsenov, R V, Uiterwijk, J W E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, Song, J S, Yoon, C S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Makhlyoueva, I V, Gorbunov, P, Khovanskii, V D, Shamanov, V V, Tsukerman, I, Bruski, N, Frekers, D, Hoshino, K, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Castagneto, L, Cocco, A G, D'Ambrosio, N, De Lellis, G, Di Capua, F, De Rosa, G, Ereditato, A, Fiorillo, G, Kawamura, T, Messina, M, Migliozzi, P, Palladino, Vittorio, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, Loverre, P F, Ludovici, L, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Spada, F R, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, Tezuka, I“…During the years 1994--1997, the emulsion target of the CHORUS detector was exposed to the Wide Band Neutrino Beam from the CERN-SPS. About 170,000 neutrino interactions were successfully located in the emulsion. …”
Publicado 2002
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3008“…An updated analysis of all available neutrino oscillation evidence in Solar experiments (SK day and night spectra, global rates from Homestake, SAGE and GALLEX) including the latest SNO CC and NC data is presented. …”
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3009
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3010
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3011
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3012por Ellis, Jonathan Richard“…Aspects of neutrino physics beyond the Standard Model are emphasized, including the emerging default options for atmospheric and solar neutrino oscillations, namely nu /sub mu / to nu /sub tau / and nu /sub e/ to nu /sub mu , tau / respectively, and the need to check them, the prospects opened up by the successful starts of SNO and K2K and the opportunities for future long-baseline neutrino experiments. …”
Publicado 2000
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3013por Ravn, H L“…The heart of the system consists of a free surface Mercury jet with a high axial velocity, which allows the heat to be carried away efficiently from the production region. For the neutrino factory the secondary pions are collected and injected into the pion decay-channel by means of a magnetic horn. …”
Publicado 2002
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3014
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3015
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3016por Ozaki, S, Palmer, R B, Zisman, M S, Gallardo, J C, Goodman, M, Hassanein, A, Norem, J H, Reed, C B, Smith, D, Teng, L C, Wang, C, Anerella, M, Berg, J S, Brennan, J M, Fernow, R C, Gupta, R, Harrison, M, Hammer, M, Hseuh, H C, Iarocci, M A, Kahn, S A, King, B J, Kirk, H G, Lissauer, D, Littenberg, L S, Luccio, A U, Ludewig, H, Marneris, I M, Mills, J, Morse, W A, Musolino, S V, O'Brien, E, Oh, W, Parker, B, Parsa, Z, Pearson, C, Prigl, R, Rehak, P, Roser, T, Ruggiero, A, Samulyak, R V, Schmalzle, J D, Simos, N, Stumer, I, Sullivan, M, Tcherniatine, V, Thieberger, P, Trbojevic, D, Weggel, R, Willen, E H, Zhang, S, Zhao, Y, Silvestrov, G I, Skrinsky, A N, Vsevolozhskaya, T A, Penn, G, Wurtele, J S, Gunion, J F, Cline, David B, Fukui, Y, Garren, A A, Lee, K, Pishchalnikov, Yu M, Autin, Bruno, Garoby, R, Haseroth, H, Johnson, C, Ravn, H L, Wilson, Edmund J N, Hoffman, K, Kim, K, Oreglia, M J, Wah, Y, Wu, V, Caldwell, A C, Conrad, J M, Monroe, J, Sciulli, F, Shaevitz, M H, Willis, W J, Geng, R, Padamsee, H, Shemelin, Valery D, Tigner, Maury, Hwang, P, Naumovich, G N, Winn, D R, Ankenbrandt, C M, Atac, Muzaffer, Balbekov, V I, Buckley-Geer, E J, Carey, D C, Childress, S, Chou, W, De Jongh, F, Diehl, H T, Drozhdin, A I, Elvira, D, Finley, D A, Geer, S H, Gounder, K, Johnstone, C, Lebrun, P, Lebedev, V, Lykken, J D, Mills, F E, Mokhov, N V, Moretti, A, Neuffer, David V, Ng, K, Popovic, M, Qian, Z, Raja, R, Reid, J S, Spentzouris, P, Stefanski, R J, Striganov, S I, Tollestrup, A V, Van Ginneken, A, Vejcik, S, Blondel, A, Learned, J G, Pakvasa, S, Ferrario, M, Bogacz, S A, Chattopadhyay, S, Wang, H, Bolton, T, Kuno, Y, Mori, Y, Yokoi, T, Black, E L, Johnson, R, Kaplan, D M, Solomey, Nickolas, Torun, Y, Errede, D, Makino, K, Berger, M S, Hansen, G G, Schwandt, P, Ginzburg, I F, Önel, Y M, Caspi, S, Corlett, J, Furman, M A, Green, M A, Hartman, N, Ladran, A S, Li, D, MacGill, R A, McInturff, A D, Reginato, L L, Rimmer, R, Scanlan, R M, Sessler, Andrew M, Shadwick, B A, Turner, W C, Vanecek, D L, Yu, S, Zolotorev, M S, Minervini, J V, Schultz, J, Berz, M, Erdélyi, B, York, R, Zeller, A, Bracker, S B, Cremaldi, L M, Summers, D, Miller, J R, Prestemon, S, Blazey, G C, Cummings, M A, Hedin, D, Schellman, H M, Chesser, J B, Conner, D L, Gabriel, T A, Gallmeier, F X, Haines, J R, Holtkamp, N, McManamy, T J, Spampinato, P T, Kim, E, Yoon, M, Lü, C, McDonald, K T, Prebys, E J, Rossmanith, R, Bennett, J R J, Titus, P, Shrock, R E, Benary, O, Barger, Vernon D, Han, TEnlace del recurso
Publicado 2001
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3017por Kirilova, Daniela“…We study the distortion of electron neutrino energy spectrum due to oscillations with the sterile neutrino nu_e <-> nu_s, and its influence on BBN for different initial populations of the sterile state delta N_s at the onset of oscillations. …”
Publicado 2002
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3018“…The sensitivity of the present CNGS beam to the sub-dominant $\nu_\mu \leftrightarrow \nu_e$ oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to $\theta_{13}$ of ICARUS and OPERA combined. …”
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3019
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3020“…We calculate the CP-violating rate asymmetry of H^\pm decays into tau and neutrino at one loop in the MSSM with complex parameters. …”
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