Dark Matter in Astro- And Particle Physics 2002
DOI: 10.1007/978-3-642-55739-2_38
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Neutrinos: Summarizing the State-of-the-Art

Abstract: I review oscillation solutions to the neutrino anomalies and discuss how to account for the required pattern of neutrino masses and mixings from first principles. Unification and low-energy bottom-up approaches are discussed, the latter open up the possibility of testing neutrino mixing at high energy colliders, such as the LHC. Large νe mixing is consistent with Supernova (SN) astrophysics and may serve to probe galactic SN parameters at Cherenkov detectors. I discuss the robustness of the atmospheric neutrin… Show more

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Cited by 4 publications
(11 citation statements)
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“…26) This LMA solution for the solar neutrino problem gives the best to the present experimental data. 27) Finally, we would like to make a comment on an interesting feature of this scenario, which is also seen in the SO(10) model. 14) In addition to Eq.…”
Section: A Higgs Field That Includes the Higgs Doublets: H(27)mentioning
confidence: 90%
See 2 more Smart Citations
“…26) This LMA solution for the solar neutrino problem gives the best to the present experimental data. 27) Finally, we would like to make a comment on an interesting feature of this scenario, which is also seen in the SO(10) model. 14) In addition to Eq.…”
Section: A Higgs Field That Includes the Higgs Doublets: H(27)mentioning
confidence: 90%
“…Throughout this paper we denote all the superfields with uppercase letters and their anomalous U (1) A charges with the corresponding lowercase letters. Assigning negative R-parity to the ordinary matter Ψ i (27), as usual, and using a field Θ with charge −1, the U (1) A invariant superpotential for low energy Yukawa terms becomes…”
Section: A Higgs Field That Includes the Higgs Doublets: H(27)mentioning
confidence: 99%
See 1 more Smart Citation
“…This is not possible since different particles all have different gauge quantum numbers. 5 In principle we are allowed to do this since the cancellation of the FI D-term only imposes…”
Section: Mass Matrices After the Fayet-iliopoulos Breakingmentioning
confidence: 99%
“…In addition one would like to understand the mixings and hierarchies of neutrinos. The global analysis of solar, atmospheric and reactor data [5] indicates that they have masses given by ∆m 2 21 ≈ 2.4 × 10 −5 to 2.4 × 10 −4 eV 2 , ∆m 2 32 ≈ 1.4 × 10 −3 to 6 × 10 −3 eV 2 , (3) and a Maki-Nakagawa-Sakata (MNS) weak coupling matrix [6] with the charged leptons [5]:…”
Section: Introductionmentioning
confidence: 99%