Results 121 to 130 of about 1,298,977 (255)
Measurement of the νe and total 8B solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set [PDF]
, 2011 This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of ...B. Aharmim, S. N. Ahmed, J. Amsbaugh, Juan-Manuel Anaya, A. Anthony, J. Banar, N. Barros, E. Beier, A. Bellerive, B. Beltrán, M. Bergevin, M. Bergevin, S. Biller, K. Boudjemline, M. Boulay, T. Bowles, M. Browne, T. V. Bullard, T. Burritt, B. Cai, Y. Chan, D. Chauhan, M. Chen, B. Cleveland, G. Cox, C. Currat, X. Dai, X. Dai, H. Deng, J. Detwiler, M. Dimarco, P. Doe, G. Doucas, M. Dragowsky, M. Dragowsky, P.-L. Drouin, C. Duba, F. Duncan, M. Dunford, E. D. Earle, S. Elliott, H. C. Evans, G. Ewan, J. Farine, H. Fergani, F. Fleurot, R. Ford, J. Formaggio, M. Fowler, N. Gagnon, N. Gagnon, N. Gagnon, J. Germani, A. Goldschmidt, J. Goon, K. Graham, E. Guillian, S. Habib, R. Hahn, A. Hallin, E. Hallman, A. A. Hamian, G. Harper, P. Harvey, R. Hazama, K. Heeger, W. Heintzelman, J. Heise, R. Helmer, R. Henning, A. Hime, C. Howard, M. Howe, M. Huang, P. Jagam, B. Jamieson, N. Jelley, K. Keeter, J. Klein, L. Kormos, M. Kos, A. Krueger, C. Kraus, C. Krauss, T. Kutter, C. Kyba, R. Lange, J. Law, I. Lawson, K. Lesko, J. Leslie, J. Loach, J. Loach, R. Maclellan, S. Majerus, H. Mak, J. Maneira, R. Martin, N. McCauley, A. McDonald, S. Mcgee, C. Mifflin, G. Miller, M. Miller, B. Monreal, J. Monroe, B. Morissette, A. Myers, Bernie G. Nickel, A. Noble, H. O'Keeffe, N. Oblath, R. Ollerhead, G. O. Gann, S. Oser, R. Ott, S. Peeters, A. Poon, G. Prior, S. D. Reitzner, K. Rielage, B. Robertson, R. Robertson, E. Rollin, M. Schwendener, J. Secrest, S. Seibert, O. Simard, J. Simpson, P. Skensved, M. W. Smith, T. Sonley, T. D. Steiger, L. Stonehill, G. Tesic, P. Thornewell, P. Thornewell, N. Tolich, T. Tsui, C. Tunnell, T. V. Wechel, R. Berg, B. VanDevender, C. Virtue, B. Wall, D. Waller, H. Tseung, J. Wendland, N. West, J. Wilhelmy, J. Wilkerson, J. Wilson, J. Wouters, A. Wright, M. Yeh, Fajun Zhang, K. Zuber +156 moresemanticscholar +1 more sourceHighlights from Super-Kamiokande
EPJ Web of Conferences, 2016 Recent results from Super-Kamiokande experiment are reviewed in this paper; Neutrino mass hierarchy and CP violation in the lepton sector are investigated via νμ → νe oscillation of the atmospheric neutrinos.Okumura Kimihirodoaj +1 more sourceNeutrino Astrophysics [PDF]
arXiv, 2008 I review the current status of neutrino astrophysics, including solar
neutrinos; atmospheric neutrinos; neutrino mass and oscillations; supernova
neutrinos; neutrino nucleosynthesis (Big Bang nucleosynthesis, the neutrino
process, the r-process); neutrino cooling and red giants; and high energy
neutrino astronomy.arxiv Current Status of the Resonant Spin-Flavor Precession Solution to the
Solar Neutrino Problem [PDF]
, 1999 We discuss the current status of the resonant spin-flavor precession (RSFP)
solution to the solar neutrino problem. We perform a fit to all the latest
solar neutrino data for various assumed magnetic field profiles in the sun.Adelberger, Akhmedov, Akhmedov, Akhmedov, Akhmedov, Akhmedov, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Balantekin, Barger, Caso, Chauhan, Cisneros, Fiorentini, Fogli, Fogli, Fukuda, Gavrin, Gribov, Guzzo, Guzzo, Guzzo, H. Nunokawa, Hata, Kirsten, Krastev, Krastev, Lande, Lim, Lim, M.M. Guzzo, Mikheyev, Mikheyev, Minakata, Minakata, Nunokawa, Okun, Pastor, Pulido, Pulido, Pulido, Raffelt, Roulet, Schechter, Schechter, Schmitt, Shi, Suzuki, Wolfenstein +55 morecore +2 more sourcesEffects of Forbush Decreases on the Global Electric Circuit
Space Weather, Volume 22, Issue 4, April 2024.Abstract
The suppression of high‐energy cosmic rays, known as Forbush decreases (FDs), represents a promising factor in influencing the global electric circuit (GEC) system. Researchers have delved into these effects by examining variations, often disruptive, of the potential gradient (PG) in ground‐based measurements taken in fair weather regions.J. Tacza, G. Li, J.‐P. Raulinwiley +1 more sourceMeasurement of the 8B solar neutrino flux with the KamLAND liquid scintillator detector [PDF]
, 2011 We report a measurement of the neutrino-electron elastic scattering rate from ^8B solar neutrinos based on a 123 kton-day exposure of KamLAND. The background-subtracted electron recoil rate, above a 5.5-MeV analysis threshold is 1.49 ± 0.14(stat) ± 0.17 ...K. Abe, K. Furuno, A. Gando, Y. Gando, K. Ichimura, H. Ikeda, K. Inoue, Y. Kibe, W. Kimura, Y. Kishimoto, M. Koga, Y. Minekawa, T. Mitsui, T. Morikawa, N. Nagai, K. Nakajima, K. Nakamura, M. Nakamura, K. Narita, I. Shimizu, Y. Shimizu, J. Shirai, F. Suekane, A. Suzuki, H. Takahashi, N. Takahashi, Y. Takemoto, K. Tamae, H. Watanabe, B. D. Xu, H. Yabumoto, E. Yonezawa, H. Yoshida, S. Yoshida, S. Enomoto, A. Kozlov, H. Murayama, C. Grant, G. Keefer, D. Mckee, A. Piepke, T. Banks, T. Bloxham, J. Detwiler, S. Freedman, B. Fujikawa, K. Han, R. Kadel, Thomas O'Donnell, H. Steiner, L. Winslow, D. Dwyer, C. Mauger, R. Mckeown, C. Zhang, B. Berger, C. Lane, J. Maricic, T. Miletić, M. Batygov, J. Learned, S. Matsuno, S. Pakvasa, M. Sakai, G. Horton-Smith, A. Tang, K. Downum, G. Gratta, K. Tolich, Y. Efremenko, Y. Kamyshkov, O. Perevozchikov, H. Karwowski, D. Markoff, W. Tornow, K. Heeger, F. Piquemal, J. Ricol, M. Decowski +78 moresemanticscholar +1 more sourceRecent Borexino results and prospects for the near future
EPJ Web of Conferences, 2016 The Borexino experiment located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos.D’Angelo D., Agostini M., Altenmüller K., Appel S., Bellini G., Benziger J., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Caminata A., Cavalcante P., Chepurnov A., Davini S., Derbin A., Di Noto L., Drachnev I., Etenko A., Fomenko K., Franco D., Gabriele F., Galbiati C., Ghiano C., Giammarchi M., Goeger-Neff M., Goretti A., Gromov M., Hagner C., Hungerford E., Ianni Aldo, Ianni Andrea, Jedrzejczak K., Kaiser M., Kobychev V., Korablev D., Korga G., Kryn D., Laubenstein M., Lehnert B., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Machulin I., Manecki S., Maneschg W., Marcocci S., Meroni E., Meyer M., Miramonti L., Misiaszek M., Montuschi M., Mosteiro P., Muratova V., Neumair B., Oberauer L., Obolensky M., Ortica F., Pallavicini M., Papp L., Perasso L., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Roncin R., Rossi N., Schönert S., Semenov D., Simgen H., Skorokhvatov M., Smirnov O., Sotnikov A., Sukhotin S., Suvorov Y., Tartaglia R., Testera G., Thurn J., Toropova M., Unzhakov E., Vishneva A., Vogelaar R.B., von Feilitzsch F., Wang H., Weinz S., Winter J., Wojcik M., Wurm M., Yokley Z., Zaimidoroga O., Zavatarelli S., Zuber K., Zuzel G. +95 moredoaj +1 more sourceGlobal 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 sourceHeavy Elements and Electromagnetic Transients from Neutron Star Mergers
Annalen der Physik, Volume 536, Issue 2, February 2024.Astro‐(physics) has made major leaps forward through the combined information provided by both gravitational waves and electromagnetic emission from the first detected neutron star merger event. This review provides an up‐to‐date overview of today's understanding of neutron star mergers and their electromagnetic emission and it discusses possible ...Stephan Rosswog, Oleg Korobkinwiley +1 more source
