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Proceedings of the first workshop on Flavor Symmetries and consequences in Accelerators and Cosmology (FLASY2011)
High Energy Physics - Phenomenology · Submitted 26 Jan 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The main goals of the first "Workshop on FLAvor SYmmetries and consequences in accelerators and cosmology" (FLASY) was to summarize the theoretical status of flavor symmetries, bringing together young researchers in the field to stimulate discussions and new collaborations, with the aim of investigating possible new physics scenarios to be tested at the LHC, as well as in future neutrino, cosmology experiments and dark matter searches.
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The main goals of the first "Workshop on FLAvor SYmmetries and consequences in accelerators and cosmology" (FLASY) was to summarize the theoretical status of flavor symmetries, bringing together young researchers in the field to stimulate discussions and new collaborations, with the aim of investigating possible new physics scenarios to be tested at the LHC, as well as in future neutrino, cosmology experiments and dark matter searches.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The main goals of the first "Workshop on FLAvor SYmmetries and consequences in accelerators and cosmology" (FLASY) was to summarize the theoretical status of flavor symmetries, bringing together young researchers in the field to stimulate discussions and new collaborations, with the aim of investigating possible new physics scenarios to be tested at the LHC, as well as in future neutrino, cosmology experiments and dark matter searches. | contribution 0.62 | 0.21 | 0.12 | asserted 0.97 |
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Original abstract
The main goals of the first "Workshop on FLAvor SYmmetries and consequences in accelerators and cosmology" (FLASY) was to summarize the theoretical status of flavor symmetries, bringing together young researchers in the field to stimulate discussions and new collaborations, with the aim of investigating possible new physics scenarios to be tested at the LHC, as well as in future neutrino, cosmology experiments and dark matter searches.
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References
How the literature uses it
5 arXiv papers cite this in 6 sentences
Papers citing it · 1 sentence without a confident label
Builds on it 1 paper
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The last case is completely new and here we will present a model from first principles, implementing the inverse seesaw mechanism [ref] as well as a non-Abelian flavor symmetry [ref] , along the lines of Ref. [ref] , but adopting $S_4$, instead of $A_4$.
A new neutrino mass sum rule from inverse seesaw · Introduction · 0.80
Cites it as background 4 papers
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One of the common ideas, often discussed in the literature [ref] , is using flavor symmetries, and one of the most attractive ideas in this regard is the $μ$–$τ$ symmetry [ref] .
Neutrino Mass Textures and Partial $\mu$-$\tau$ Symmetry · Introduction · 0.94
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Of the numerous neutrino mixing scenarios discussed in the literature [ref] , several have \(μ-τ\) symmetry, such as tri-bimaximal mixing (TBM) [ref] , bimaximal mixing (BM) [ref] , hexagonal mixing (HM) [ref] and scenarios of \(A_5\) mixing [ref] .
Perturbations to \mu-\tau\ symmetry in neutrino mixing · Introduction · 0.99
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Several alternative ideas have come out, invoking non-Abelian flavor symmetries [ref] , such as the $A_4$ symmetry [ref] .
Generalized Bottom-Tau unification, neutrino oscillations and dark matter: predictions from a lepton quarticity flavor approach · Introduction · 0.97
What it cites · 25 sentences without a confident label
Uses data or values from 5 papers
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Without entering into further details, the results [ref] for the $0ν2β$ effective mass are shown in fig.
Tri-bimaximal Neutrino Mixing and Quark Masses from a Discrete Flavour Symmetry · Flavour Symmetries in the $0ν2β$ Decay · 0.95
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In the conservative scenario of only 3 active neutrinos, their oscillations can be described by two frequencies, $Δm^2_sol≡m^2_2-m^2_1≈7.6×10^-5 eV^2$ and $Δm^2_atm≡|m^2_3-m^2_1|≈2.5×10^-2 eV^2$, and three mixing angles, the solar $sin^2θ_12≈0.31$, the atmospheric $sin^2θ_23≈0.5$ and the reactor $sin^2θ_13≈0.015$ [ref] .
Where we are on $\theta_{13}$: addendum to "Global neutrino data and recent reactor fluxes: status of three-flavour oscillation parameters" · Introduction · 0.94
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[ref](a), the table shows the recent results [ref] considering two contexts and different combination of the cosmological data: the Blue corresponds to the standard cosmological model $Λ$CDM with massive neutrinos and the Red the generalization with non-vanishing curvature and with $ω≠-1$ in the Dark Matter equation of state.
Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results · The $0ν2β$ Effective Mass · 0.89
Cites as background 2 papers
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The second realization I consider is the Niemeyer model [ref] , that is also based on the $A_4$ group.
Tri-bimaximal neutrino mixing and neutrinoless double beta decay · Flavour Symmetries in the $0ν2β$ Decay · 0.82
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A more complete list of exotic mechanisms can be found in [ref] .
Neutrino-less Double Beta Decay and Particle Physics · The $0ν2β$ Decay · 0.93
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