Results 1 to 10 of about 333 (166)
Solar and atmospheric neutrinos [PDF]
Pramana, 1994 Possible explanations of solar neutrino and atmospheric neutrino anomalies are summarized and future tests discussed.
Sandip Pakvasa
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Solar and atmospheric neutrino oscillations [PDF]
Physica Scripta, 2001 8 pages, LaTeX, 6 figures.
M.C. González-García +1 more
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Solar and atmospheric neutrino oscillations with three flavors [PDF]
Physical Review D, 1996 We analyze the solar and the atmospheric neutrino problems in the context of three flavour neutrino oscillations. We assume a mass hierarchy in the vacuum mass eigenvalues $ _3^2 \gg _2^2 \geq _1^2$, but make no approximation regarding the magnitudes of the mixing angles.
Mohan Narayan +3 more
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Implications of Solar and Atmospheric Neutrinos [PDF]
Nuclear Physics B - Proceedings Supplements, 1993 Latex, DPF92, 4 pages, 1 figure (available on request), UPR ...
Paul Langacker
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A Supersymmetric Resolution of Solar and Atmospheric Neutrino Puzzles [PDF]
Physical Review D, 1997 9 ...
M. Drees +3 more
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Reconciling dark matter, solar and atmospheric neutrinos [PDF]
Nuclear Physics B, 1993 We present models that can reconcile the solar and atmospheric neutrino data with the existence of a hot dark matter component in the universe. This dark matter is a quasi-Dirac neutrino whose mass $m_{DM}$ arises at the one-loop level. The solar neutrino deficit is explained via nonadiabatic conversions of electron neutrino to a sterile neutrino and ...
J. Peltoniemi, J. W. F. Valle
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Democratic approach to atmospheric and solar neutrino oscillations
Physics Letters B, 2002 Working with a ${\cal U}(1)$ flavor symmetry, we show how the hierarchical structure in the charged fermion sector and a democratic approach for neutrinos that yields large solar and atmospheric neutrino mixings can be simultaneously realized in the MSSM framework. However, in SU(5) due to the unified multiplets we encounter difficulties.
Qaisar Shafi, Zurab Tavartkiladze
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Atmospheric and solar neutrino oscillations in νMSSM and beyond [PDF]
Physics Letters B, 1999 We show how a unified description of the various two-flavor neutrino oscillation solutions, allowed by the atmospheric and solar neutrino experiments, are naturally realized within the framework of $ $MSSM (MSSM augmented with the seesaw mechanism) and beyond, especially grand unified theories.
Qaisar Shafi, Zurab Tavartkiladze
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Solar atmospheric neutrino search with IceCube [PDF]
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017), 2017 Cosmic rays interacting in the solar atmosphere can produce high energy neutrinos, which could be detected with IceCube. Neutrinos are produced through the decay of pions and kaons, similar to cosmic ray air showers in the Earth’s atmosphere. Due to the lower solar atmospheric density, the neutrino spectrum from the Sun is expected to be harder as ...
Minjin Jeong, Seongjin In
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Solar, Supernova, and Atmospheric Neutrinos [PDF]
, 1999 To be published in the Proceedings of the 1998 Australian National University Nuclear Physics Summer School; S. Kuyucak, Ed.
A. B. Balantekin, W. C. Haxton
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