Results 131 to 140 of about 333 (166)

Report of the Solar and Atmospheric Neutrino Working Group

, 2004
H.O. Back, John N. Bahcall, J. Bernabéu, M. G. Boulay, T. Bowles, F. Calaprice, A. E. Champagne, S. J. Freedman, M. Gai, C. Galbiati, H. Gallagher, A. César González‐García, R. L. Hahn, K. M. Heeger, A. Hime, C. K. Jung, J. R. Klein, Masafumi Koike, R. E. Lanou, J. G. Learned, K. T. Lesko, J. M. LoSecco, Michele Maltoni, A. Mann, D. N. McKinsey, Sergio Palomares-Ruiz, C. Peña‐Garay, S.T. Petcov, A. Piepke, M. Pitt, R. Raghavan, R. G. H. Robertson, K. Scholberg, H. W. Sobel, Tatsu Takeuchi, R. B. Vogelaar, L. Wolfenstein   +36 more
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Three flavor neutrino oscillation constraints from accelerator, reactor, atmospheric and solar neutrino experiments [PDF]

, 1996
Osamu Yasuda, Hisakazu Minakata
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Unified treatment of solar and atmospheric neutrino oscillations [PDF]

, 1992
K. S. Babu, Qaisar Shafi
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Neutrino physics and the mirror world: how exact parity symmetry explains the solar neutrino deficit, the atmospheric neutrino anomaly and the LSND experiment

, 1995
R. Foot, Raymond R. Volkas
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Experimental Results on Neutrino Oscillations Using Atmospheric, Solar and Accelerator Beams

, 2000
Danuta Kiełczewska
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Possible neutrino gravitoelectric dipole moments and atmospheric and solar neutrino anomalies

, 2004
An. S. Kuznetsov
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Textures for atmospheric and solar neutrino oscillations

, 1998
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Kamiokande results on atmospheric neutrinos and solar neutrinos

Nuclear Physics B - Proceedings Supplements, 1994
Abstract The recent results on the atmospheric neutrinos and solar neutrinos are summarized. The double ratio, (μ/e) data /(μ/e) MC , of the fully contained atmospheric neutrino events for 6.18ktonyr is (0.59∼0.60)±0.06±0.05. The solar neutrino measurement extended till the end of July in 1993 gives almost entire coverage of the solar maximum in ...
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Solar Atmospheric Neutrino searches with the ANTARES neutrino telescope

2022
The interaction of cosmic-rays with the solar atmosphere can yield neutrinos as final state particles, the so-called Solar Atmospheric Neutrinos (SAυs). Most of these neutrinos are absorbed in the interior of the Sun. Neutrinos produced in the solar corona towards the Earth would escape the Sun and reach the Earth.
Lopez-Coto D., Navas S., Zornoza J. D., Albert A., Alves S., Andre M., Anghinolfi M., Anton G., Ardid M., Ardid S., Aubert J. -J., Aublin J., Baret B., Basa S., Belhorma B., Bendahman M., Bertin V., Biagi S., Bissinger M., Boumaaza J., Bouta M., Bouwhuis M. C., Branzas H., Bruijn R., Brunner J., Busto J., Caiffi B., Capone A., Caramete L., Carr J., Carretero V., Celli S., Chabab M., Chau T. N., El Moursli R. C., Chiarusi T., Circella M., Coleiro A., Colomer-Molla M., Coniglione R., Coyle P., Creusot A., Diaz A. F., de Wasseige G., Deschamps A., Distefano C., Di Palma I., Domi A., Donzaud C., Dornic D., Drouhin D., Eberl T., van Eeden T., van Eijk D., El Khayati N., Enzenhofer A., Fermani P., Ferrara G., Filippini F., Fusco L. A., Gatelet Y., Gay P., Glotin H., Gozzini R., Gracia Ruiz R., Graf K., Guidi C., Hallmann S., van Haren H., Heijboer A. J., Hello Y., Hernandez-Rey J. J., Hossl J., Hofestadt J., Huang F., Illuminati G., James C. W., Jisse-Jung B., de Jong M., de Jong P., Kadler M., Kalekin O., Katz U., Khan-Chowdhury N. R., Kouchner A., Kreykenbohm I., Kulikovskiy V., Lahmann R., Le Breton R., Lefevre D., Leonora E., Levi G., Lincetto M., Lopez-Coto D., Loucatos S., Maderer L., Manczak J., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J. A., Melis K., Migliozzi P., Moussa A., Muller R., Nauta L., Navas S., Nezri E., O'Fearraigh B., Paun A., Pavalas G. E., Pellegrino C., Perrin-Terrin M., Pestel V., Piattelli P., Pieterse C., Poire C., Popa V., Pradier T., Randazzo N., Reck S., Riccobene G., Romanov A., Sanchez-Losa A., Salesa Greus F., Samtleben D. F. E., Sanguineti M., Sapienza P., Schnabel J., Schumann J., Schussler F., Spurio M., Stolarczyk Th., Taiuti M., Tayalati Y., Tingay S. J., Vallage B., Van Elewyck V., Versari F., Viola S., Vivolo D., Wilms J., Zavatarelli S., Zegarelli A., Zornoza J. D., Zuniga J.   +145 more
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Three-flavor vacuum oscillations of atmospheric and solar neutrinos

Physical Review D, 1994
Vacuum oscillations of [nu][sub [mu]] into [nu][sub [tau]] and either matter-enhanced or just-so'' vacuum oscillations of [nu][sub [ital e]] into [nu][sub [mu]] are generally invoked to explain the observed discrepancies in atmospheric and solar neutrino fluxes, respectively.
, Acker, , Balantekin, , Loreti
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