Results 1 to 10 of about 239,431 (169)

Standard Solar Neutrinos [PDF]

, 1996
An improved standard solar model has been used to calculate the fluxes of standard solar neutrinos. It includes premain sequence evolution, element diffusion, partial ionization effects, and all the possible nuclear reactions between the main elements ...
Anders, Anselmann, Arnon Dar, Bahcall, Bahcall, Bahcall, Barker, Caughlan, Christensen-Dalsgaard, Cleveland, Dar, Dar, Dawarakanath, Dzitko, Filippone, Geiss, Giora Shaviv, Greife, Grevesse, Grevesse, Grevesse, Hata, Hata, Hernandez, Hilgemeier, Johnson, Kamionkowski, Kavanagh, Kim, Kovetz, Krauss, Krawinkel, Langanke, Mikheyev, Motobayashi, Osborne, Parke, Parker, Parker, Parker, Rogers, Shaviv, Shaviv, Sturenburg, Vaughn, Volk, Wolfenstein, Wolfenstein   +47 more
core   +2 more sources

Three-generation neutrino mixing and LSND dark matter neutrinos [PDF]

, 1996
The reported signal at the LSND experiment, when interpreted as neutrino mixing with $\delta m^2 = 6 \;\rm{eV}^2$, provides evidence for neutrinos with a cosmologically significant mass.
Adeva, Athanassopoulos, Athanassopoulos, Berezhianai, Bilenky, Bilenky, Buskulic, Caldwell, Cardall, Cardall, Casper, Chen, Christian Y. Cardall, Chun, Enqvist, Fogli, Fogli, Fogli, Foot, Fukuda, Fuller, George M. Fuller, Kitamura, Krastev, Krastev, Krastev, Kwong, Lee, Ma, Ma, Michael, Montanet, Primack, Qian, Qian, Qian, Saltzberg, Shi, Totsuka, Yasuda   +39 more
core   +3 more sources

Neutrino Effects in Nucleosynthesis [PDF]

, 2000
The nucleosynthesis within a Type II supernova occurs in an intense neutrino flux. I discuss some of the effects associated with neutrino interactions, including direct synthesis in the neutrino process, the role of neutrinos in controlling the r-process
Haxton, W. C.
core   +3 more sources

High-energy neutrino-nucleus interactions [PDF]

, 2018
High-energy neutrino-nucleus interactions are discussed by considering neutrino-oscillation experiments and ultra-high-energy cosmic neutrino interactions.
Kumano, S.
core   +2 more sources

Progress in neutrino oscillation searches and their implications

, 2003
Neutrino Oscillation, in which a given flavour of neutrino transforms into another is a powerful tool for probing small neutrino masses. The intrinsic neutrino properties involved are neutrino mass squared difference $\Delta m^2$ and the mixing angle in ...
A Bandyopadhyay, A Bandyopadhyay, B T Cleveland, C Athanassopoulos, Ch Berger, Ch. Berger, D Buskulic, D Casper, E A Hawker, E Fiorini, F Terranova, G L Fogli, H Ejiri, H V Klapdor-Kleingrothaus, J N Abdurashitov, J N Bahcall, L Borodovsky, L Wolfenstein, M Agiletta, M Altmann, M Goodman, M Honda, M Maltoni, Q R Ahmad, R Becker-Szendy, S Choubey, S Choubey, S H Ahn, S M Bilenky, S M Bilenky, S P Mikheyev, S T Petcov, S T Petcov, Srubabati Goswami, T K Gaisser, V D Barger, V Paolone, W Hampel, Y Farzan, Y Fukuda, Y Fukuda, Y Fukuda   +41 more
core   +1 more source

Effects of nonstandard neutrino interactions at PINGU

, 2013
Neutrino oscillation experiments in the past decades have greatly improved our knowledge on neutrinos by measuring the fundamental neutrino parameters. The ongoing and upcoming neutrino oscillation experiments are intended to pin down the neutrino mass ...
Ohlsson, Tommy, Zhang, He, Zhou, Shun
core   +1 more source

Neutrino Oscillations: from Standard and Non-standard Viewpoints [PDF]

, 2011
In the standard model of neutrino oscillations, the neutrino flavor states are mixtures of mass-eigenstates, and the phenomena are well described by the neutrino mixing matrix, i.e., the PMNS matrix. I review the recent progress on parametrization of the
Ma, Bo-Qiang
core   +1 more source

Neutrino mass matrix with U(2) flavor symmetry and neutrino oscillations

, 1997
The three neutrino mass matrices in the $SU(5)\times U(2)$ model are studied focusing on the neutrino oscillation experiments. The atmospheric neutrino anomaly could be explained by the large $\nu_{\mu} - \nu_{\tau}$ oscillation.
A. Pomarol, B. Achkar, C. Athanassopoulos, C. Athanassopoulos, C. Athanassopoulos, C. D. Carone, G. Fiorentini, J. E. Hill, K. Winter, L. Borodovsky, L. Wolfenstein, L. Wolfenstein, M. Dine, Morimitsu Tanimoto, N. Hata, P. H. Frampton, P. H. Frampton, P. I. Krastev, P. I. Krastev, P. Pouliot, R. Barbieri, R. Barbieri, R. Barbieri, R. M. Barnett, S. Ahlen, S. P. Mikheyev, S. Wojcicki, W. W. M. Allison, Y. Fukuda   +28 more
core   +1 more source

Effect of Coulomb collisions on time variations of the solar neutrino flux

, 1999
We consider the possibility of time variations of the solar neutrino flux due to the radial motion of the Earth and neutrino interference effects. We calculate the time variations of the detected neutrino flux and the extent to which they are suppressed ...
Bahcall J. N., Bahcall J. N., L. Malyshkin, Mikheev S. P., R. Kulsrud, Stodolsky L.   +5 more
core   +3 more sources

Neutrino Opacities in Neutron Stars with Kaon Condensates [PDF]

, 2003
The neutrino mean free paths in hot neutron-star matter are obtained in the presence of kaon condensates. The kaon-induced neutrino absorption process, which is allowed only in the presence of kaon condensates, is considered for both nondegenerate and ...
A. E. Nelson, B. L. Friman, C.-H. Lee, C.-R. Ji, D. B. Kaplan, D. B. Kaplan, D. N. Voskresensky, E. E. Kolomeitsev, G. E. Brown, G. E. Brown, H. Fujii, H. Fujii, H. Fujii, H. Heiselberg, J. A. Pons, J. A. Pons, J. A. Pons, J. M. Lattimer, J. Navarro, M. Christiansen, M. Prakash, M. Prakash, M. Prakash, M. Prakash, M. Takahara, M. Yasuhira, M. Yasuhira, M. Yasuhira, Masatomi Yasuhira, N. Iwamoto, N. K. Glendenning, N. K. Glendenning, Naoki Iwamoto, O. G. Benvenuto, P. Haensel, R. F. Sawyer, R. Niembro, S. Reddy, S. Reddy, S. Reddy, S. Yamada, T. Maruyama, T. Muto, T. Muto, T. Muto, T. Muto, T. Muto, T. Norsen, T. Norsen, T. Takatsuka, T. Takatsuka, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. W. Baumgarte, T. W. Baumgarte, Takumi Muto, Toshitaka Tatsumi, V. Thorsson, W. Keil   +62 more
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