Results 41 to 50 of about 41,603 (215)

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 neutrinos

New Journal of Physics, 2004
11 pages, 6 figures, Proceedings of Physics in Collision Conference, Stanford, California, June ...
openaire   +3 more sources

Combined Effect of NSI and SFP on Solar Electron Neutrino Oscillation

Advances in High Energy Physics, 2016
The combined effect of spin-flavor precession (SFP) and the nonstandard neutrino interaction (NSI) on the survival probability of solar electron neutrinos (assumed to be Dirac particles) is examined for various values of ϵ11, ϵ12, and μB.
Deniz Yilmaz
doaj   +1 more source

Present Status of Neutrino Mixing [PDF]

, 2001
A short review of the status of neutrino mixing and neutrino oscillations is given. The basics of neutrino mixing and oscillations is discussed. The latest evidences of neutrino oscillations obtained in the Super-Kamiokande and the SNO solar neutrino ...
B. Pontecorvo, B. T. Cleveland, F. Boehm, F.L. Villante, H.V. Klapdor-Kleingrothaus, J. N. Abdurashitov, J.N. Bahcall, Kamiokande Collaboration, L. Landau, M. Altmann, M. Apollonio, M. Gell-Mann, M. Goldhaber, Q.R. Ahmad, S. Fukuda, S. Fukuda, S. M. Bilenky, S.M. Bilenky, S.M. Bilenky, S.M. Bilenky, S.T. Petcov, W. Hampel, Z. Maki   +22 more
core   +3 more sources

Solar ν ¯ e $$ {\overline{\nu}}_e $$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field

Journal of High Energy Physics, 2022
The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP).
Evgeny Akhmedov, Pablo Martínez-Miravé
doaj   +1 more source

Solar neutrino measurements in Super-Kamiokande-I [PDF]

, 2005
The details of Super--Kamiokande--I's solar neutrino analysis are given. Solar neutrino measurement in Super--Kamiokande is a high statistics collection of $^8$B solar neutrinos via neutrino-electron scattering.
A. Habig, A. K. Ichikawa, A. Kibayashi, A. L. Stachyra, A. Minamino, A. Morel, A. Okada, A. Sarrat, A. Suzuki, A. T. Suzuki, B. K. Kim, C. K. Jung, C. Mauger, C. McGrew, C. Mitsuda, C. Saji, C. W. Sterner, C. W. Walter, C. Yanagisawa, D. Casper, D. Kielczewska, D. Turcan, D. W. Liu, E. Blaufuss, E. Blaufuss, E. Kearns, E. Sharkey, G. Guillian, G. Mitsuka, G. W. Sullivan, H. G. Berns, H. Ishino, H. K. Seo, H. Kume, H. Maesaka, H. Nishino, H. Okazawa, H. Sato, H. W. Sobel, I. Higuchi, I. Kato, I. T. Lim, J. A. Goodman, J. Cooley, J. G. Learned, J. Hill, J. Hosaka, J. Kameda, J. L. Stone, J. P. Cravens, J. S. Jang, J. Shirai, J. Y. Kim, J. Yoo, J. Zalipska, K. B. Lee, K. Inoue, K. Ishihara, K. K. Shiraishi, K. Kaneyuki, K. Kobayashi, K. Martens, K. Nakamura, K. Nishijima, K. Nishikawa, K. Nitta, K. Okumura, K. S. Ganezer, K. Scholberg, K. Washburnand, L. R. Sulak, M. B. Smy, M. D. Messier, M. Goldhaber, M. Hasegawa, M. Ishitsuka, M. Koshiba, M. Malek, M. Miura, M. Nakahata, M. Nemoto, M. R. Vagins, M. Sakuda, M. Shiozawa, M. Yokoyama, M. Yoshida, N. Sakurai, N. Tamura, R. Gran, R. J. Wilkes, R. Svoboda, R. W. Ellsworth, S. B. Kim, S. Clark, S. Dazeley, S. Desai, S. Hatakeyama, S. Likhoded, S. Matsuno, S. Mine, S. Moriyama, S. Nakayama, S. Tasaka, S. Yamada, S. Yamamoto, S. P. Mikheyev, T. Hasegawa, T. Ishida, T. Ishii, T. Ishizuka, T. Iwashita, T. J. Haines, T. Kajita, T. Kato, T. Kobayashi, T. Nakadaira, T. Nakaya, T. Namba, T. Sasaki, T. Sato, W. E. Keig, W. R. Kropp, W. Wang, Y. Choi, Y. Fukuda, Y. Gando, Y. Hayato, Y. Itow, Y. Koshio, Y. Kuno, Y. Obayashi, Y. Oyama, Y. Suzuki, Y. Takenaga, Y. Takeuchi, Y. Totsuka, Y. Watanabe   +136 more
core   +1 more source

Solar models and solar neutrino oscillations [PDF]

, 2004
We provide a summary of the current knowledge, theoretical and experimental, of solar neutrino fluxes and of the masses and mixing angles that characterize solar neutrino oscillations.
, , Adelberger E G, Asplund M, Asplund M, Asplund M, Asplund M, Baby L T, Bahcall J N, Bahcall J N, Bahcall J N, Bahcall J N, Bahcall J N, Boehm F, Carlos Peña-Garay, Coleman S R, Colladay D, de Holanda P C Smirnov A Y, Friedland A Lunardini C Peña-Garay C, Gonzalez-Garcia M C, Haxton W C, John N Bahcall, Jung C K, Junghans A R, McDonald A, Messiah A O Fackler J Tran Thanh Van, Mikheev S P Smirnov A Y O Fackler J Tran Thanh Van, Mikheyev S P, Murayama H, Murayama H, Park T S, Smirnov A Yu M B Ceolin, Wolfenstein L   +32 more
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Detecting Solar Neutrino Flare in Megaton and km^3 detectors

, 2009
To foresee a solar flare neutrino signal we infer its upper and lower bound. The upper bound was derived since a few years by general energy equipartition arguments on observed solar particle flare.
Daniele Fargion, Fargion, Fargion, Fargion, Grechnev, Kistler, Paola Di Giacomo   +6 more
core   +1 more source

Solar neutrino with Borexino: results and perspectives [PDF]

, 2014
Borexino is a unique detector able to perform measurement of solar neutrinos fluxes in the energy region around 1 MeV or below due to its low level of radioactive background. It was constructed at the LNGS underground laboratory with a goal of solar $^{7}
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., Fiorentini, G., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Hagner, C., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Kobychev, V., Korablev, 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., Mantovani, F., Marcocci, S., Meindl, Q., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Ricci, B., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G.   +89 more
core   +3 more sources

On Stellar Evolution in a Neutrino Hertzsprung–Russell Diagram

The Astrophysical Journal, 2020
We explore the evolution of a select grid of solar metallicity stellar models from their pre-main-sequence phase to near their final fates in a neutrino Hertzsprung–Russell diagram, where the neutrino luminosity replaces the traditional photon luminosity.
Ebraheem Farag, F. X. Timmes, Morgan Taylor, Kelly M. Patton, R. Farmer   +4 more
doaj   +1 more source