Results 51 to 60 of about 99,563 (256)

Mass or Gravitationally Induced Neutrino Oscillations? -- A Comparison of $\B$ Neutrino Flux Spectra in a Three--Generation Framework [PDF]

, 1995
Both gravitational and mass induced neutrino oscillation mechanisms provide possible resolutions to the Solar Neutrino Problem. The distinguishing feature between the two mechanisms is their dependence on the neutrino energy.
Abdurashidov, Ammosov, Anselmann, Athanassopoulos, Bahcall, Bahcall, Bahcall, Baldini, Borodovsky, Butler, Casper, Cleveland, Davis, Gasperini, Goodman, Halprin, Hill, Hirata, Hirata, Iida, J.R Mureika, Mikheyev, Mikheyev, Minakata, Mureika, Pantaleone, R.B Mann, Wolfenstein, Zaglauer   +28 more
core   +2 more sources

SNO and the neutrino magnetic moment solution of the solar neutrino problem [PDF]

, 2000
Assuming that the solar neutrino deficit observed in the Homestake, SAGE, Gallex, Kamiokande and Super-Kamiokande experiments is due to the interaction of the neutrino transition magnetic moment with the solar magnetic field, we calculate the expected ...
Akhmedov, E. Kh., Pulido, J.
core   +2 more sources

Solar Neutrinos

Advances in High Energy Physics, 2013
The study of solar neutrinos has given a fundamental contribution both to astroparticle and to elementary particle physics, offering an ideal test of solar models and offering at the same time relevant indications on the fundamental interactions among ...
V. Antonelli, L. Miramonti, C. Peña Garay, A. Serenelli   +3 more
doaj   +1 more source

Status of a hybrid three-neutrino interpretation of neutrino data [PDF]

, 2002
We reanalyze the non-standard interaction (NSI) solutions to the solar neutrino problem in the light of the latest solar, atmospheric and reactor neutrino data.
Abdurashitov, Abdurashitov, Ahmad, Allison, Altmann, Ambrosio, Apollonio, Bahcall, Bahcall, Bandyopadhyay, Bandyopadhyay, Barger, Barger, Barger, Barish, Beacom, Becker-Szendy, Bellotti, Berezhiani, Berezhiani, Bergmann, Bergmann, Bilenkii, Boehm, Butler, Cleveland, Creminelli, Diaz, Dziewonski, Ellis, Fogli, Fogli, Fogli, Fogli, Fogli, Fornengo, Fornengo, Fukuda, Fukuda, Fukuda, Fukuda, Fukuda, Fukuda, Gago, Gago, Gago, Gago, Gavrin, Gonzalez-Garcia, Gonzalez-Garcia, Gonzalez-Garcia, Grasso, Guzzo, Guzzo, Guzzo, H. Nunokawa, Hall, Hall, Hampel, Haug, Hempfling, Hirata, Hirsch, Hirsch, Huber, Huber, J.W.F. Valle, Kachelriess, Kuo, Kuo, Kuo, Lipari, M. Maltoni, M.A. Tórtola, M.M. Guzzo, Ma, Mikheev, Mohapatra, Nakamura, Nunokawa, P.C. de Holanda, Peres, Ross, Roulet, Schechter, Schechter, Schechter, Spurio, Surdo, Suzuki, Towner, Valle, Valle, Wolfenstein   +93 more
core   +4 more sources

Neutrino magnetic moments and the solar neutrino problem [PDF]

, 1994
Talk given at the 6th International Symposium "Neutrino Telescopes'', Venice, February 22--24, 1994, LaTex, 11 pages, FTUV/94--26, 15A-40561-INT94 ...
E. Kh. Akhmedov
openalex   +6 more sources

Three-flavor MSW solutions of the solar neutrino problem [PDF]

, 1999
We perform an updated phenomenological analysis of the Mikheyev-Smirnov-Wolfenstein (MSW) solutions of the solar neutrino problem, assuming oscillations between two and three neutrino families. The analysis includes the total rates of the Homestake, SAGE,
G. Fogli, D. Montanino, E. Lisi, A. Palazzo   +3 more
semanticscholar   +1 more source

On the vacuum oscillation solutions of the solar neutrino problem. [PDF]

Physical Review D, Particles and fields, 1995
We study the stability of the two-neutrino vacuum oscillation solution of the solar neutrino problem with respect to changes of the total fluxes of $^{8}\mathrm{B}$ and $^{7}\mathrm{Be}$ neutrinos, ${\mathrm{\ensuremath{\Phi}}}_{\mathrm{B}}$ and ...
P. Krastev, S. Petcov
semanticscholar   +1 more source

Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework [PDF]

, 2000
We study extensions of supersymmetric models without R-parity which include an anomalous U(1)_H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level of approximately $(\theta^2)^\delta$ eV where $\theta\approx 0.22$
Abada, Abada, Abreu, Apollonio, Aulakh, Babu, Banks, Barbier, Barbieri, Barbieri, Barger, Binetruy, Binetruy, Binetruy, Boehm, Borzumati, Choi, Choi, Chun, D.A. Restrepo, de Gouvea, Dimopoulos, Dudas, E. Nardi, Ellis, Enqvist, Fogli, Fornengo, Friedland, Froggatt, Fukuda, Fusaoka, Giudice, Godbole, Gonzalez-Garcia, Green, Grossman, Hall, Hempfling, Hirsch, Ibanez, J.M. Mira, J.W.F. Valle, Joshipura, Kaplunovsky, Leurer, Leurer, Mira, Nardi, Nir, Romao, Ross, Roulet, Santamaria, Santamaria, Santamaria, Silk   +56 more
core   +5 more sources

Solar Neutrinos and Lepton Mixing [PDF]

, 1995
With latest experimental data the solar neutrino problem enters new phase when crucial aspects of the problem can be formulated in an essentially (solar) model independent way.
Smirnov, A. Yu.
core   +3 more sources

Solar neutrino problem and gravitationally induced long-wavelength neutrino oscillation [PDF]

Physical Review Letters, 1999
We have reexamined the possibility of explaining the solar neutrino data through long-wavelength neutrino oscillations induced by a tiny breakdown of the weak equivalence principle of general relativity.
Gago, Nunokawa, Zukanovich Funchal R
semanticscholar   +1 more source