Topic
Solar neutrino problem
About: Solar neutrino problem is a research topic. Over the lifetime, 7441 publications have been published within this topic receiving 175940 citations.
Papers published on a yearly basis
Papers
More filters
TL;DR: In this article, the effect of coherent forward scattering on neutrinos traveling through matter is taken into account when considering the oscillations of neutrino traveling through the matter, where the neutral current has an off-diagonal piece connecting different neutrini types.
Abstract: The effect of coherent forward scattering must be taken into account when considering the oscillations of neutrinos traveling through matter. In particular, for the case of massless neutrinos for which vacuum oscillations cannot occur, oscillations can occur in matter if the neutral current has an off-diagonal piece connecting different neutrino types. Applications discussed are solar neutrinos and a proposed experiment involving transmission of neutrinos through 1000 km of rock.
3,050 citations
TL;DR: Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported, providing strong evidence for solar nu(e) flavor transformation.
Abstract: Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported. Using the neutral current (NC), elastic scattering, and charged current reactions and assuming the standard 8B shape, the nu(e) component of the 8B solar flux is phis(e) = 1.76(+0.05)(-0.05)(stat)(+0.09)(-0.09)(syst) x 10(6) cm(-2) s(-1) for a kinetic energy threshold of 5 MeV. The non-nu(e) component is phi(mu)(tau) = 3.41(+0.45)(-0.45)(stat)(+0.48)(-0.45)(syst) x 10(6) cm(-2) s(-1), 5.3sigma greater than zero, providing strong evidence for solar nu(e) flavor transformation. The total flux measured with the NC reaction is phi(NC) = 5.09(+0.44)(-0.43)(stat)(+0.46)(-0.43)(syst) x 10(6) cm(-2) s(-1), consistent with solar models.
2,732 citations
Tohoku University1, University of Alabama2, University of California, Berkeley3, California Institute of Technology4, Drexel University5, Louisiana State University6, University of New Mexico7, Stanford University8, University of Tennessee9, University of North Carolina at Chapel Hill10, Duke University11
TL;DR: In the context of two-flavor neutrino oscillations with CPT invariance, all solutions to the solar neutrinos problem except for the "large mixing angle" region are excluded.
Abstract: KamLAND has measured the flux of ν _e’s from distant nuclear reactors. We find fewer ν _e events than expected from standard assumptions about ν _e propagation at the 99.95% C.L. In a 162 ton·yr exposure the ratio of the observed inverse β-decay events to the expected number without ν _e disappearance is 0.611±0.085(stat)±0.041(syst) for ν _e energies >3.4 MeV. In the context of two-flavor neutrino oscillations with CPT invariance, all solutions to the solar neutrino problem except for the “large mixing angle” region are excluded.
2,108 citations
University of Adelaide1, University of Wisconsin-Madison2, Ghent University3, University of Canterbury4, University of Geneva5, Humboldt University of Berlin6, University of California, Irvine7, University of Mainz8, University of California, Berkeley9, Ohio State University10, Université libre de Bruxelles11, Ruhr University Bochum12, University of Wuppertal13, University of Maryland, College Park14, University of Kansas15, Lawrence Berkeley National Laboratory16, RWTH Aachen University17, Uppsala University18, University of Alberta19, Stockholm University20, Vrije Universiteit Brussel21, University of Bonn22, École Polytechnique Fédérale de Lausanne23, Georgia Institute of Technology24, Pennsylvania State University25, Technical University of Dortmund26, Southern University and A&M College27
TL;DR: The presence of a high-energy neutrino flux containing the most energetic neutrinos ever observed is revealed, including 28 events at energies between 30 and 1200 TeV, although the origin of this flux is unknown and the findings are consistent with expectations for a neutRino population with origins outside the solar system.
Abstract: We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to about 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the 28 events at the 4 sigma level. These 28 events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected from the atmospheric muon and neutrino backgrounds. These properties are, however, consistent with generic predictions for an additional component of extraterrestrial origin.
1,490 citations
TL;DR: In this article, the authors give simple mass-matrices leading to tri-bimaximal mixing, and discuss its relation to the Fritzsch-Xing democratic ansatz.
1,347 citations