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1901
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1902“…Results of neutrino oscillation experiments have always been presented on the(sin^2 2theta, Delta m^2) parameter space for the case of two-flavoroscillations. …”
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1903
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1904
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1905
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1906
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1907
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1908
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1909por Deden, H, Hasert, F J, Krenz, W, Lanske, D, Morfín, J G, Pohl, M, Schultze, K, Welch, L, Bertrand-Coremans, G H, Mulkens, H, Sacton, J, Van Doninck, W K, Burmeister, H, Danilchenko, I A, Haidt, Dieter, Jobin, P, Matteuzzi, C, Musset, P, Myklebost, K, Pattison, John Bryan M, Perkins, Donald Hill, Pittuck, D J, Romano, F, Waldren, D, Blondel, A, Brisson, V, Degrange, B, François, T, Haguenauer, Maurice, Nguyen-Khac, U, Petiau, P, van Dam, P, Bellotti, E, Bonetti, S, Cavalli, D, Fiorini, Ettore, Pullia, Antonio, Rollier, M, Aubert, Bernard, Blum, D, Chounet, L M, Heusse, P, Jaffré, M, Jauneau, L, Longuemare, C, Lutz, A M, Pascaud, C, Vialle, J P, Bullock, F W, Esten, M J, Jones, T W, Michette, A G, Myatt, Gerald, Segar, A JEnlace del recurso
Publicado 2000
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1910“…We argue that any viable particle physics solution would most likely involve the resonant production of a non-interacting neutrino $\nu_s$ of mass $m_{\nu_s}\sim$ 20--50 keV. …”
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1911“…A new way of making neutrino beams has caught the attention of physicists worldwide. …”
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1912por Haseroth, H“…There is a strong interest from the physics community for high-quality, high-intensity neutrino beams as produced by a neutrino factory. With the help of other European laboratories, CERN has started a study on some of the many technological challenges of such a facility. …”
Publicado 2000
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1913por Keil, Eberhard“…The R&D needs for a neutrino factory, based on a muon storage ring, are presented. …”
Publicado 2000
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1914
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1915por Bahcall, J N“…I summarize the first four decades of solar neutrino research and suggest what may be possible to learn with extragalactic neutrinos and with solar neutrinos in the next decade.…”
Publicado 2001
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1916“…We show that massive sterile neutrinos mixed with the ordinary ones may be produced in the early universe in the right amount to be natural warm dark matter particles. …”
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1917“…Recently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino oscillations. …”
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1918por Haseroth, H“…In view of the physics interest, CERN has decided to engage in the study of a Neutrino Factory. The present paper describes our basic concept, and plans for R&D.…”
Publicado 2000
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1919por Schönauer, Horst Otto, Autin, Bruno, Bongardt, K, Cappi, R, Chanel, M, Franchetti, Giuliano, Gareyte, Jacques, Garoby, R, Giovannozzi, Massimo, Haseroth, H, Hofmann, I, Koscielniak, Shane Rupert, Martini, M, Métral, Elias, Möhl, D, Pirkl, Werner, Prior, C R, Rees, G H, Schindl, Karlheinz, Senichev, Yu V“…The paper describes the CERN approach for a proton driver for a Neutrino Factory. Two main layouts are presented: the so-called CERN Reference Scenario, based on a 2.2 GeV linac and an alternative one, based on a 30 GeV synchrotron. …”
Publicado 2000
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1920“…We show in a model independent manner that, if the magnitudes of Majorana masses of neutrinos are exactly equal at some high scale, the radiative corrections cannot reproduce the observed masses and mixing spectrum at the low scale, irrespective of the Majorana phases or the mixing angles at the high scale.…”
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