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3761“…The authors give results for both the 350-GeV wide-band neutrino beam at CERN and the 400-GeV quadrupole triplet neutrino beam at Fermilab, including experimental cuts. …”
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3762por Holder, M, Berthelot, A, Bloch, p, Devaux, B, Dorth, W, Dydak, F, Eisele, F, Geweniger, C, Grimm, M, Hepp, V, Kleinknecht, K, Knobloch, J, Maillard, J, May, J, Navarria, Francesco Luigi, Paar, H P, Palazzi, P, Peyaud, B, Rander, J, Ranjard, F, Savoy-Navarro, A, Schlatter, W D, Spahn, G, Steinberger, J, Suter, H, Tittel, K, Turlay, René, Wahl, H, Whitaker, S, Williams, E G H, Willutzki, H J, Wotschack, J“…The authors report on the analysis of inclusive neutral current events produced in neutrino and antineutrino narrow band beams. One finds for incident neutrino energies in the range 12-200 GeV and for hadron energies above 12 GeV a neutral charged current cross-section ratio of R/sub nu /=0.293+or-0.010 for incident neutrinos, and R/sub anti nu /=0.35+or-0.03 for antineutrinos. …”
Publicado 1977
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3763por Holder, M, Bloch, P, Devaux, B, Dorth, W, Dydak, F, Eisele, F, Geweniger, C, Grimm, M, Hepp, V, Kleinknecht, K, Knobloch, J, Maillard, J, May, J, Paar, H P, Palazzi, P, Peyaud, B, Rander, J, Savoy-Navarro, A, Schlatter, W D, Spahn, G, Steinberger, J, Suter, H, Tittel, K, Turlay, René, Wahl, H, Williams, E G H, Willutzki, H J, Wotschack, JEnlace del recurso
Publicado 1977
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3764por Holder, M, Bloch, P, Devaux, B, Dorth, W, Dydak, F, Eisele, F, Geweniger, C, Grimm, M, Hepp, V, Kleinknecht, K, Knobloch, J, Maillard, J, May, J, Navarria, Francesco Luigi, Paar, H P, Palazzi, P, Peyaud, B, Rander, J, Savoy-Navarro, A, Schlatter, W D, Spahn, G, Steinberger, J, Suter, H, Tittel, K, Turlay, René, Wahl, H, Williams, E G H, Willutzki, H J, Wotschack, J“…On the basis of 315 dimuon events of opposite sign for which the nature (and energy) of the incident neutrino is known, and the momenta and hadronic energy are measured, the authors find a) very similar production by neutrinos and antineutrinos, and therefore confirmation of the GIM model for semileptonic weak interactions, b) energy spectra, excitation functions, angular correlations and transverse momentum distributions which are in remarkable agreement with the hypothesis of charm production and decay, c) evidence against models for which the second muon has a heavy lepton as origin, d) evidence against 'bottom' quark production by antineutrinos, e) the amount and the structure function for the strange quark-antiquark sea, and f) an approximate branching ratio, of 0.15 for the muonic decay of the semistable charmed meson.…”
Publicado 1977
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3765por Mulvey, J H“…These events have the general characteristics of neutrino interactions; however not all the 70 events of energy greater than 10 GeV can be attributed to conventional sources ( pi , K or hyperon decay); in particular the observation of 11 events with an emerging e/sup -/ and 4 e/sup +/ events requires a new, prompt source of neutrinos. …”
Publicado 1978
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3766por Abramowicz, H, Buchholz, P, De Groot, J G H, Dydak, F, Eisele, F, Flottmann, T, Geweniger, C, Guyot, C, He, J T, Klasen, H P, Kleinknecht, K, Knobloch, J, Królikowski, J, May, J, Merlo, J P, Palazzi, P, Para, A, Peyaud, B, Pszola, B, Rander, J, Ranjard, F, Renk, B, Rothberg, J E, Ruan, T Z, Schlatter, W D, Schuller, J P, Steinberger, J, Taureg, H, Tittel, K, Turlay, René, von Rüden, Wolfgang, Wahl, H, Willutzki, H J, Wotschack, J, Wu, W M“…In distinction to similar limits derived from muon decay or beta decay, our limits are also valid if the right handed neutrino is heavy.…”
Publicado 1982
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3767
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3768“…We find restrictions on the mass and mixing angle of the dark matter sterile neutrinos using X-ray observations of Coma and Virgo galaxy clusters.…”
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3769“…We consider in full generality the interplay between type-I and type-II seesaw for neutrino masses. We first perform a \chi^2 fit of fermion masses independent on the detailed structure of the GUT Higgs potential and show the regions in the parameter space that are preferred by the fermion mass sum rules. …”
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3770por Gross, A, Achterberg, A, Ackermann, M, Ahrens, J, Atlee, D W, Bahcall, J N, Bai, X, Baret, B, Bartelt, M, Bay, R, Barwick, S W, Beattie, K, Becka, T, Becker, K H, Becker, J K, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, D Z, Blaufuss, E, Boersma, D J, Bohm, C, Boser, S, Botner, O, Bouchta, A, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Clem, J, Conrad, J, Cooley, J, Cowen, D F, D'Agostino, M V, Davour, A, Day, C T, De Clercq, C, Desiati, P, De Young, T R, Dreyer, J, Duvoort, M R, Edwards, W R, Ehrlich, R, Ekstrom, P, Ellsworth, R W, Evenson, P A, Fazely, A R, Feser, T, Filimonov, K, Gaisser, T K, Gallagher, J, Ganugapati, R, Geenen, H, Gerhardt, L, Greene, M G, Grullon, S, Goldschmidt, A, Goodman, J, Gro, A, Gunasingha, R M, Hallgren, A, Halzen, F, Hanson, K, Hardtke, D, Hardtke, R, Harenberg, T, Hart, J E, Hauschildt, T, Hays, D, Heise, J, Helbing, K, Hellwig, M, Herquet, P, Hill, G C, Hodges, J, Hoffman, K D, Hoshina, K, Hubert, D, Hughey, B, Hulth, P O, Hultqvist, K, Hundertmark, S, Ishihara, A, Jacobsen, J, Japaridze, G S, Jones, A, Joseph, J M, Kampert, K H, Karle, A, Kawai, H, Kelley, J L, Kestel, M, Kitamura, N, Klein, S R, Klepser, S, Kohnen, G, Kolanoski, H, Köpke, L, Krasberg, M, Kühn, K, Kujawski, E, Landsman, H, Lang, R, Leich, H, Liubarsky, I, Lundberg, J, Madsen, J, Marciniewski, P, Mase, K, Matis, H S, McCauley, T, McParland, C P, Meli, A, Messarius, T, Mészáros, P, Minor, R H, Miocinovic, P, Miyamoto, H, Mokhtarani, A, Montaruli, T, Morey, A, Morse, R, Movit, S M, Munich, K, Nahnhauer, R, Nam, J W, Niessen, P, Nygren, D R, Ogelman, H, Olbrechts, P, Olivas, A, Patton, S, Peña-Garay, C, Perez de los Heros, C, Pieloth, D, Pohl, A C, Porrata, R, Pretz, J, Price, P B, Przybylski, G T, Rawlins, K, Razzaque, S, Refflinghaus, F, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Rizzo, A, Robbins, S, Rott, C, Rutledge, D, Sander, H G, Schlenstedt, S, Schneider, D, Schwarz, R, Seckel, D, Seo, S H, Silvestri, A, Smith, A J, Solarz, M, Song, C, Sopher, J E, Spiczak, G M, Spiering, C, Stamatikos, M, Stanev, T, Steffen, P, Stezelberger, T, Stokstad, R G, Stoufer, M, Stoyanov, S, Sulanke, K H, Sullivan, G W, Sumner, T J, Taboada, I, Tarasova, O, Tepe, A, Thollander, L, Tilav, S, Toale, P A, Turcan, D, van Eijndhoven, N, Vandenbroucke, J, Voigt, B, Wagner, W, Walck, C, Waldmann, H, Walter, M, Wang, Y R, Wendt, C, Wiebusch, C, Wikström, G, Williams, D, Wischnewski, R, Wissing, H, Woschnagg, K, Xu, X W, Yoshida, S, Yodh, G, Messarius, TEnlace del recurso
Publicado 2005
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3771por Münich, K, Achterberg, A, Ackermann, M, Ahrens, J, Atlee, D W, Bahcall, J N, Bai, X, Baret, B, Bartelt, M, Bay, R, Barwick, S W, Beattie, K, Becka, T, Becker, K H, Becker, J K, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, D Z, Blaufuss, E, Boersma, D J, Bohm, C, Boser, S, Botner, O, Bouchta, A, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Clem, J, Conrad, J, Cooley, J, Cowen, D F, D'Agostino, M V, Davour, A, Day, C T, De Clercq, C, Desiati, P, De Young, T R, Dreyer, J, Duvoort, M R, Edwards, W R, Ehrlich, R, Ekstrom, P, Ellsworth, R W, Evenson, P A, Fazely, A R, Feser, T, Filimonov, K, Gaisser, T K, Gallagher, J, Ganugapati, R, Geenen, H, Gerhardt, L, Greene, M G, Grullon, S, Goldschmidt, A, Goodman, J, Gro, A, Gunasingha, R M, Hallgren, A, Halzen, F, Hanson, K, Hardtke, D, Hardtke, R, Harenberg, T, Hart, J E, Hauschildt, T, Hays, D, Heise, J, Helbing, K, Hellwig, M, Herquet, P, Hill, G C, Hodges, J, Hoffman, K D, Hoshina, K, Hubert, D, Hughey, B, Hulth, P O, Hultqvist, K, Hundertmark, S, Ishihara, A, Jacobsen, J, Japaridze, G S, Jones, A, Joseph, J M, Kampert, K H, Karle, A, Kawai, H, Kelley, J L, Kestel, M, Kitamura, N, Klein, S R, Klepser, S, Kohnen, G, Kolanoski, H, Köpke, L, Krasberg, M, Kühn, K, Kujawski, E, Landsman, H, Lang, R, Leich, H, Liubarsky, I, Lundberg, J, Madsen, J, Marciniewski, P, Mase, K, Matis, H S, McCauley, T, McParland, C P, Meli, A, Messarius, T, Mészáros, P, Minor, R H, Miocinovic, P, Miyamoto, H, Mokhtarani, A, Montaruli, T, Morey, A, Morse, R, Movit, S M, Nahnhauer, R, Nam, J W, Niessen, P, Nygren, D R, Ogelman, H, Olbrechts, P, Olivas, A, Patton, S, Peña-Garay, C, Perez de los Heros, C, Pieloth, D, Pohl, A C, Porrata, R, Pretz, J, Price, P B, Przybylski, G T, Rawlins, K, Razzaque, S, Refflinghaus, F, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Rizzo, A, Robbins, S, Rott, C, Rutledge, D, Sander, H G, Schlenstedt, S, Schneider, D, Schwarz, R, Seckel, D, Seo, S H, Silvestri, A, Smith, A J, Solarz, M, Song, C, Sopher, J E, Spiczak, G M, Spiering, C, Stamatikos, M, Stanev, T, Steffen, P, Stezelberger, T, Stokstad, R G, Stoufer, M, Stoyanov, S, Sulanke, K H, Sullivan, G W, Sumner, T J, Taboada, I, Tarasova, O, Tepe, A, Thollander, L, Tilav, S, Toale, P A, Turcan, D, van Eijndhoven, N, Vandenbroucke, J, Voigt, B, Wagner, W, Walck, C, Waldmann, H, Walter, M, Wang, Y R, Wendt, C, Wiebusch, C, Wikström, G, Williams, D, Wischnewski, R, Wissing, H, Woschnagg, K, Xu, X W, Yoshida, S, Yodh, GEnlace del recurso
Publicado 2005
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3772
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3773
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3774
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3775Publicado 2006“…The new verification that oscillations exists and neutrinos have mass though not detectible easy provides the first clue to extra dimensions, dark matter, hyperspace and chilled universe acting as a platform below it. (1/2 page)…”
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3776
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3777por Bernardini, G, Bienlein, H, von Dardel, G, Faissner, H, Ferroro, F, î , Gaillard J A, J , Gerver H, Hahn, B, Kaftanov, V, Krienen, F, Reinharz, M, A , Salmeron R, G , Seller P, Staude, A, Steiner, H JEnlace del recurso
Publicado 1964
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3778“…In the framework of CERN neutrino platform project at the CERN SPS North Area, two new beam lines have been designed as extensions of the existing secondary beam lines, able to provide low energy particles in the momentum range of 0.4 to 12 GeV/c. …”
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3779“…The Galaxy is a guaranteed source of neutrinos produced by the interaction of cosmic rays (CRs) with the interstellar gas. …”
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3780por Norris, Barry, Bremer, Johan, Chalifour, Michel, Delaney, Mike, Dinnon, Mike, Doubnik, Roza, Geynisman, Michael, Hentschel, Steve, Kim, Min Jeong, Stefanik, Andy, Tillman, Justin, Zuckerbrot, Mike“…The Short-Baseline Neutrino (SBN) physics program will involve three LAr-TPC detectors located along the Booster Neutrino Beam (BNB) at Fermilab. …”
Publicado 2017
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