Results 141 to 150 of about 1,298,977 (255)

Solar neutrino results in Super-Kamiokande-III [PDF]

, 2010
The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results.
K. Abe, Y. Hayato, T. Iida, M. Ikeda, C. Ishihara, K. Iyogi, J. Kameda, K. Kobayashi, Y. Koshio, Y. Kozuma, M. Miura, S. Moriyama, M. Nakahata, S. Nakayama, Y. Obayashi, H. Ogawa, H. Sekiya, M. Shiozawa, Y. Suzuki, A. Takeda, Y. Takenaga, K. Ueno, K. Ueshima, H. Watanabe, S. Yamada, T. Yokozawa, S. Hazama, H. Kaji, T. Kajita, K. Kaneyuki, T. McLachlan, K. Okumura, Y. Shimizu, N. Tanimoto, M. Vagins, L. Labarga, L. Magro, F. Dufour, E. Kearns, M. Litos, J. Raaf, J. Stone, L. Sulak, W. Wang, M. Goldhaber, K. Bays, D. Casper, J. P. Cravens, W. Kropp, S. Mine, C. Regis, A. Renshaw, M. Smy, H. Sobel, K. Ganezer, J. Hill, W. Keig, J. Jang, J. Kim, I. Lim, J. Albert, R. Wendell, T. Wongjirad, K. Scholberg, C. Walter, T. Ishizuka, S. Tasaka, J. Learned, S. Matsuno, Y. Watanabe, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nishikawa, H. Nishino, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. Suzuki, Y. Takeuchi, A. Minamino, T. Nakaya, Y. Fukuda, Y. Itow, G. Mitsuka, T. Tanaka, C. Jung, G. López, C. Mcgrew, R. Terri, C. Yanagisawa, N. Tamura, H. Ishino, A. Kibayashi, S. Mino, T. Mori, M. Sakuda, H. Toyota, Y. Kuno, M. Yoshida, S. Kim, B. Yang, H. Okazawa, Y. Choi, K. Nishijima, Y. Yokosawa, M. Koshiba, Y. Totsuka, M. Yokoyama, S. Chen, Y. Heng, Z. Yang, H. Zhang, D. Kiełczewska, P. Mijakowski, K. Connolly, M. Dziomba, E. Thrane, R. Wilkes   +122 more
semanticscholar   +1 more source

Neutrino Physics & The Solar Neutrino Problem [PDF]

arXiv, 2009
A literature review of neutrino physics and the solar neutrino problem.
arxiv  

Solar neutrinos and the solar model

Physics of the Dark Universe, 2014
AbstractThis paper reviews solar neutrino observations interpreted in the context of the Solar Standard Model and neutrino oscillations. Solar neutrinos have been detected since 1968. Early results showed a significant discrepancy between measured solar neutrino rates and predictions. This fact has been known for 30 years as the “Solar Neutrino Problem”
openaire   +3 more sources

Low Energy Neutrino Physics after SNO and KamLAND

, 2004
In the recent years important discoveries in the field of low energy neutrino physics (E$_\nu$ in the $\approx$ MeV range) have been achieved. Results of the solar neutrino experiment SNO show clearly flavor transitions from $\nu_e$ to $\nu_{\mu,\tau ...
Achkar B., Apollonio M., Athanassopoulos C., Babu K. S., Gavrin V. N., Klapdor-Kleingrothaus H. V., Klapdor-Kleingrothaus H. V., L. OBERAUER, Lobashev V. M., Weinheimer Ch., Zacek G.   +10 more
core   +1 more source

The Sun and solar neutrinos

Journal of Physics: Conference Series, 2017
n ...
Vinyoles, N., Serenelli, A., Villante, F. L.   +2 more
openaire   +4 more sources

Is There a Deficit of Solar Neutrinos? [PDF]

arXiv, 2004
Measurements on the isotopic and elemental compositions of meteorites, planets, lunar samples, the solar wind, and solar flares since 1960 suggest that the standard solar model may be in error. A new solar model suggests that the observed number of solar neutrinos represents at least 87% of the number generated: There is little if any deficit of solar ...
arxiv  

Solar Neutrinos: What We Have Learned

, 1993
The four operating solar neutrino experiments confirm the hypothesis that the energy source for solar luminosity is hydrogen fusion. However, the measured rate for each of the four solar neutrino experiments differs significantly (by factors of 2.0 to 3 ...
,. R. Davis, A. Acker, A. Cisneros, A.,I. Abazov, A.I. Abazov, B. Pontecorvo, C.M. Lim, E. Akhmedov, E. Schatzman, G. Aardsma, G. Ranucci, H. Chen, J Frieman, J. Schechter, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.P. Revol, K.S. Hirata, K.S. Hirata, L. Krauss, L. Wolfenstein, L. Wolfenstein, L.B. Okun, M. Takita, M.B. Voloshin, P. Anselmann, P. Anselmann, P.I. Krastev, R. Davis, R.E. Lanou, R.S. Raghavan, S. Pakvasa, S.M. Bilenky, S.M. Bilenky, S.P. Mikheyev, S.P. Mikheyev, S.P. Mikheyev, S.P. Mikheyev, T.K. Kuo, V. Gribov, X Shi, X.-G. He, Y. Suzuki, Z.G. Berezhiani, Z.G. Berezhiani   +50 more
core   +2 more sources

A possible solution to the solar neutrino problem: Relativistic corrections to the Maxwellian velocity distribution [PDF]

arXiv, 2001
The relativistic corrections to the Maxwellian velocity distribution are needed for standard solar models. Relativistic equilibrium velocity distribution, if adopted in standard solar models, will lower solar neutrino fluxes and change solar neutrino energy spectra but keep solar sound speeds. It is possibly a solution to the solar neutrino problem.
arxiv  

CONSTRAINTS ON THE OPACITY PROFILE OF THE SUN FROM HELIOSEISMIC OBSERVABLES AND SOLAR NEUTRINO FLUX MEASUREMENTS [PDF]

, 2010
Motivated by the solar composition problem and by using the recently developed linear solar model approach, we analyze the role of opacity and metals in the Sun.
F. Villante
semanticscholar   +1 more source

ecCNO solar neutrinos: A challenge for gigantic ultra-pure liquid scintillator detectors

Physics Letters B, 2015
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low.
F.L. Villante
doaj