Results 51 to 60 of about 41,366 (209)
Global Analysis of the post-SNO Solar Neutrino Data for Standard and
Non-Standard Oscillation Mechanisms
, 2002 What can we learn from solar neutrino observations? Is there any solution to
the solar neutrino anomaly which is favored by the present experimental
panorama? After SNO results, is it possible to affirm that neutrinos have mass?A. Bandyopadhyay, A. de Gouvea, A. Halprin, A. M. Gago, A. M. Gago, A. M. Gago, A. M. Gago, A. M. Gago, A. Piepke, A. R. Junghans, A. Romosan, A. Strumia, B. C. Chauhan, C. Athanassopoulos, C. Athanassopoulos, C. E. Ortiz, C. Giunti, C. S. Lim, C. S. Lim, D. N. Abdurashitov, D. O. Caldwell, E. Kh. Akhmedov, E. Kh. Akhmedov, E. Kh. Akhmedov, E. Roulet, G. Dvali, G. L. Fogli, G. L. Fogli, G. L. Fogli, G. L. Fogli, G. L. Fogli, G. M. Fuller, G. Ranucci, H. Murayama, H. Nunokawa, I. R. Kenyon, J. J. Gomez-Cadenas, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. Pantaleone, J. Pantaleone, J. Pulido, J. Pulido, J. Pulido, J. Schechter, J. Schechter, J. T. Peltoniemi, J. T. Peltoniemi, J. W. F. Valle, K. Lande, L. Wolfenstein, M. Altmann, M. C. Gonzalez-Garcia, M. C. Gonzalez-Garcia, M. C. Gonzalez-Garcia, M. Gasperini, M. Gasperini, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, M. M. Guzzo, N. Fornengo, N. Fornengo, N. Okada, O. G. Miranda, O. G. Miranda, O. L. G. Peres, P. C. de Holanda, P. I. Krastev, P. Lipari, Q. R. Ahmad, R. Zukanovich Funchal, S. Bergmann, S. Bergmann, S. Bergmann, S. Degl’Innocenti, S. Nakamura, S. P. Mikheyev, S. P. Mikheyev, S. W. Mansour, V. Barger, V. Barger, V. D. Barger, V. N. Gribov, V. Pleitez, W. Hampel, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Fukuda, Z. Maki +98 morecore +1 more sourceConstraints on neutrino oscillation parameters from the measurement of
day-night solar neutrino fluxes at Super-Kamiokande [PDF]
, 1998 A search for day-night variations in the solar neutrino flux resulting from
neutrino oscillations has been carried out using the 504 day sample of solar
neutrino data obtained at Super-Kamiokande.A. Dar, A. Habig, A. Hasegawa, A. Kibayashi, A. L. Stachyra, A. M. Dziewonski, A. Okada, A. Sakai, A. Suzuki, A. T. Suzuki, B. K. Kim, B. T. Cleveland, B. Viren, C. K. Jung, C. Mauger, C. McGrew, C. Saji, C. W. Walter, C. Yanagisawa, D. Casper, D. Kielczewska, D. Takemori, E. Blaufuss, E. Ichihara, E. Kearns, E. Sharkey, F. Reines, F. Tsushima, G. L. Fogli, G. W. Sullivan, H. Ishino, H. Ogawa, H. Okazawa, H. W. Sobel, I.-J. Sackman, J. A. Goodman, J. G. Learned, J. Hill, J. Hsu, J. Kameda, J. Kanzaki, J. L. Stone, J. N. Abdurashitov, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. N. Bahcall, J. S. George, J. Shirai, J. W. Flanagan, K. Fujita, K. Inoue, K. Ishihara, K. K. Young, K. Kaneyuki, K. Kobayashi, K. Martens, K. Miyano, K. Nakamura, K. Nishijima, K. Nishikawa, K. Okumura, K. S. Ganezer, K. Scholberg, L. L. Wai, L. R. Price, L. R. Sulak, L. Wolfenstein, M. D. Messier, M. Earl, M. Etoh, M. Goldhaber, M. Koga, M. Kohama, M. Koshiba, M. L. Chen, M. Miura, M. Nakahata, M. Nemoto, M. R. Vagins, M. Sakuda, M. Shiozawa, M. Smy, M. Takahata, M. Takita, M. Yoshida, N. Sakurai, O. Sasaki, P. Anselmann, P. G. Halverson, R. A. Doyle, R. J. Wilkes, R. Sanford, R. Svoboda, R. W. Ellsworth, S. B. Kim, S. Echigo, S. Hatakeyama, S. Kasuga, S. Matsuno, S. Mine, S. Nakayama, S. P. Mikheyev, S. Tasaka, S. Turck-Chièze, S. Yamada, T. Barszczak, T. Futagami, T. Hasagawa, T. Hayakawa, T. Ishii, T. Iwamoto, T. J. Haines, T. Kajita, T. Kobayashi, T. Maruyama, T. Yamaguchi, V. Gavrin, V. J. Stenger, W. Doki, W. E. Keig, W. Gajewski, W. Hampel, W. R. Kropp, X. Shi, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Hayato, Y. Itow, Y. Kanaya, Y. Kobayashi, Y. Koshio, Y. Nagashima, Y. Oyama, Y. Suzuki, Y. Takeuchi, Y. Totsuka, Y. Watanabe, Z. Conner +142 morecore +3 more sourcesSolar Neutrino Measurements
, 2018 We present the most recent results from the two currently running solar neutrino experiments, Borexino at the Gran Sasso laboratory in Italy and SuperK at Kamioka mine in Japan. SuperK has released the most precise yet measurement of the 8B solar neutrino interaction rate, with a precision better than 2\%, consistent with a constant solar neutrino ...Pocar, A., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bagdasarian, Z., Basilico, D., Bellini, G., Benziger, J., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cappelli, L., Caprioli, S., Carlini, M., Cavalcante, P., Cavanna, F., Chepurnov, A., Choi, K., Collica, L., d'Angelo, D., Davini, S., Derbin, A., Ding, X.F., Di Ludovico, A., Di Noto, L., Drachnev, I., Fomenko, K., Formozov, A., Franco, D., Gabriele, F., Galbiati, C., Gschwender, M., Ghiano, C., Giammarchi, M., Goretti, A., Gromov, M., Guffanti, D., Houdy, T., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jany, A., Jeschke, D., Kumaran, S., Kobychev, V., Korga, G., Lachenmaier, T., Laubenstein, M., Litvinovich, E., Lombardi, P., Ludhova, L., Lukyanchenko, G., Lukyanchenko, L., Machulin, I., Manuzio, G., Marcocci, S., Maricic, J., Martyn, J., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Muratova, V., Neumair, B., Nieslony, M., Oberauer, L., Orekhov, V., Ortica, F., Pallavicini, M., Papp, L., Penek, Ö., Pietrofaccia, L., Pilipenko, N., Porcelli, A., Raikov, G., Ranucci, G., Razeto, A., Re, A., Redchuk, M., Romani, A., Rossi, N., Rottenanger, S., Schönert, S., Semenov, D., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Stokes, L.F.F., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Unzhakov, E., Vishneva, A., Vogelaar, R.B., von Feilitzsch, F., Weinz, S., Wojcik, M., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G. +105 moreopenaire +4 more sourcesFirst real–time detection of solar pp neutrinos by Borexino
EPJ Web of Conferences, 2016 Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the Pallavicini M., Bellini G., Benziger J., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Caminata A., Cavalcante P., Chavarria A., Chepurnov A., D'Angelo D., Davini S., Derbin A., Empl A., Etenko A., Fomenko K., Franco D., Gabriele F., Galbiati C., Gazzana S., Ghiano C., Giammarchi M., Göger-Neff M., Goretti A., Gromov M., Hagner C., Hungerford E., Ianni Al., Ianni An., Kayser M., Kobychev V., Korablëv D., Korga G., Kryn D., Laubenstein M., Lehnert B., Lewke T., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Machulin I., Manecki S., Maneschg W., Marcocci S., Meindl Q., Meroni E., Meyer M., Miramonti L., Misiaszek M., Montuschi M., Mosteiro P., Muratova V., Oberauer L., Obolensky M., Ortica F., Otis K., Papp L., Perasso L., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Rossi N., Saldanha R., Salvo C., Schönert S., Simgen H., Skorokhvatov M., Smirnov O., Sotnikov A., Sukhotin S., Suvorov Y., Tartaglia R., Testera G., Vignaud D., Vogelaar R.B., Feilitzsch F. von, Wang H., Winter J., Wojcik M., Wurm M., Zaimidoroga O., Zavatarelli S., Zuber K., Zuzel G. +89 moredoaj +1 more sourceBilinear R-parity violating SUSY: Neutrinoless double beta decay in the
light of solar and atmospheric neutrino data [PDF]
, 2000 Neutrinoless double beta ($\znbb$) decay is considered within bilinear
R-parity breaking supersymmetry, including the full one-loop corrections to the
neutrino-neutralino mass matrix.Akeroyd, Apollonio, Baudis, Bednyakov, de Campos, Dı́az, Faessler, Hirsch, Hirsch, J.C. Romão, J.W.F. Valle, M. Hirsch, Passarino, Schechter, Schechter, Schechter +15 morecore +3 more sourcesSpectral Analysis of Flickering Gamma‐Ray Flashes Observed During the ALOFT 2023 Campaign
Journal of Geophysical Research: Atmospheres, Volume 130, Issue 23, 16 December 2025.Abstract
We examine a newly discovered category of high‐energy radiation events called flickering gamma‐ray flashes (FGF) detected during the airborne lightning observatory for FEGS and TGFs campaign in July 2023. These FGFs are characterized by highly pulsating gamma‐ray emissions that have no detectable concurrent optical or radio signals (Ostgaard ...D. Sarria, N. Østgaard, I. Bjørge‐Engeland, A. Mezentsev, M. Marisaldi, N. Lehtinen, M. Stanley, T. Lang, C. Schultz, A. Fuglestad +9 morewiley +1 more sourceRadar Polarimetry in Glaciology: Theory, Measurement Techniques, and Scientific Applications for Investigating the Anisotropy of Ice Masses
Reviews of Geophysics, Volume 63, Issue 4, December 2025.Abstract
Dielectric anisotropy in ice alters the propagation of polarized radio waves, so polarimetric radar sounding can be used to survey anisotropic properties of ice masses. Ice anisotropy is either intrinsic, associated with ice‐crystal orientation fabric (COF), or extrinsic, associated with material heterogeneity, such as bubbles, fractures, and ...Benjamin H. Hills, T. J. Young, David A. Lilien, Esther Babcock, Nicole Bienert, Donald Blankenship, John Bradford, Giancorrado Brighi, Alex Brisbourne, Jørgen Dall, Reinhard Drews, Olaf Eisen, M. Reza Ershadi, Tamara A. Gerber, Nicholas Holschuh, Daniela Jansen, Thomas M. Jordan, Nanna B. Karlsson, Jilu Li, Carlos Martín, Kenichi Matsuoka, Daniel May, Falk M. Oraschewski, John Paden, Nicholas M. Rathmann, Neil Ross, Dustin M. Schroeder, Martin Siegert, Matthew R. Siegfried, Emma Smith, Ole Zeising +30 morewiley +1 more source