RECORD
Neutrino Hierarchies from a Gauge Symmetry
High Energy Physics - Phenomenology · Submitted 14 Mar 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Breaking the B + 3 (L_e - L_mu - L_tau) symmetry spontaneously below the seesaw scale generates low energy neutrino mass matrices with the approximate symmetries L_e (leading to normal hierarchy) or L_e - L_mu - L_tau (inverted hierarchy).
The compiled record
The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
Open the compiled record
The abstract, sentence by sentence
We consider the phenomenology of the gauged abelian symmetry B + 3 (L_e - L_mu - L_tau). Right-handed neutrinos necessary to cancel triangle anomalies are used in a type-I seesaw scheme to create active neutrino masses. Breaking the B + 3 (L_e - L_mu - L_tau) symmetry spontaneously below the seesaw scale generates low energy neutrino mass matrices with the approximate symmetries L_e (leading to normal hierarchy) or L_e - L_mu - L_tau (inverted hierarchy). For the latter we need to introduce a Z_2 symmetry which decouples one of the right-handed neutrinos. If exact, this Z_2 leads to a Majorana dark matter candidate that interacts with the Standard Model via the Z' and a scalar s originating from spontaneous breaking of the new symmetry. The measured relic abundance of the dark matter particle can be obtained around the scalar and Z' resonances, while direct detection experiments are mainly sensitive to scalar exchange, which is induced by mass mixing of s with the standard Higgs.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We consider the phenomenology of the gauged abelian symmetry B + 3 (L_e - L_mu - L_tau). | contribution 0.87 | 0.64 | 0.04 | unclear 0.57 |
| s1 | Right-handed neutrinos necessary to cancel triangle anomalies are used in a type-I seesaw scheme to create active neutrino masses. | method 0.89 | 0.43 | 0.06 | asserted 1.00 |
| s2 | Breaking the B + 3 (L_e - L_mu - L_tau) symmetry spontaneously below the seesaw scale generates low energy neutrino mass matrices with the approximate symmetries L_e (leading to normal hierarchy) or L_e - L_mu - L_tau (inverted hierarchy). | result 0.89 | 0.71 | 0.63 | asserted 0.96 |
| s3 | For the latter we need to introduce a Z_2 symmetry which decouples one of the right-handed neutrinos. | method 0.78 | 0.63 | 0.07 | asserted 0.98 |
| s4 | If exact, this Z_2 leads to a Majorana dark matter candidate that interacts with the Standard Model via the Z' and a scalar s originating from spontaneous breaking of the new symmetry. | result 0.44 | 0.55 | 0.12 | asserted 0.88 |
| s5 | The measured relic abundance of the dark matter particle can be obtained around the scalar and Z' resonances, while direct detection experiments are mainly sensitive to scalar exchange, which is induced by mass mixing of s with the standard Higgs. | result 0.82 | 0.55 | 0.14 | asserted 0.61 |
What was examined, and what was not
- arXiv listing abstract v2
- full text
- figures and tables
- references and citing sentences
- relations to other papers
- P abstract
- S sections
- T body sentences
- C citations
- R cross-paper relations
The paper
Original abstract
We consider the phenomenology of the gauged abelian symmetry B + 3 (L_e - L_mu - L_tau). Right-handed neutrinos necessary to cancel triangle anomalies are used in a type-I seesaw scheme to create active neutrino masses. Breaking the B + 3 (L_e - L_mu - L_tau) symmetry spontaneously below the seesaw scale generates low energy neutrino mass matrices with the approximate symmetries L_e (leading to normal hierarchy) or L_e - L_mu - L_tau (inverted hierarchy). For the latter we need to introduce a Z_2 symmetry which decouples one of the right-handed neutrinos. If exact, this Z_2 leads to a Majorana dark matter candidate that interacts with the Standard Model via the Z' and a scalar s originating from spontaneous breaking of the new symmetry. The measured relic abundance of the dark matter particle can be obtained around the scalar and Z' resonances, while direct detection experiments are mainly sensitive to scalar exchange, which is induced by mass mixing of s with the standard Higgs.
Human review
References
How the literature uses it
8 arXiv papers cite this in 9 sentences
Papers citing it · 7 sentences without a confident label
Cites it as background 2 papers
-
Models based on gauge symmetries that are linear combinations of the baryon number $B$ and the individual lepton flavor numbers $L_α$ ($α=e,μ,τ$) have also been extensively discussed [ref] .
Anomaly-free U(1) gauge symmetries in neutrino seesaw flavor models · Introduction · 0.89
-
Well-known examples are $B-3L_τ$ [ref] , $L_μ-L_τ$ [ref] , $B+3(L_e-L_μ-L_τ)$ [ref] etc.
$U(1)_{B-3L_{\alpha}}$ Extended Scotogenic Models and Single-zero Textures of Neutrino Mass Matrices · Introduction · 0.97
What it cites · 28 sentences without a confident label
Builds on 1 paper
-
Since in Ref. [ref] it is only briefly mentioned that the mass matrix for the right-handed neutrinos has no vanishing entries in the broken case, we feel it is still worth discussing the neutrino masses in more detail, due to their interesting structure.
Gauged B-x_i L origin of R parity and its implications · Gauged B + 3 (Le-Lmu-Ltau) Symmetry · 0.86
Uses the method or tool of 2 papers
-
Using a modified version of GAPP [ref] to fit our model with an arbitrary scalar sector we obtain the $95%$ C.L. limit $|g'sinθ|≲10^-4$ (see Fig. [ref]) from electroweak precision data.
Constraints on Extended Neutral Gauge Structures · Gauge Sector · 1.00
-
This would however necessitate a more complicated model, so Occam's razor suggests an exact $2$.] We show the relic abundance of $χ$ as a function of its mass and the $h$-$s$ mixing angle $α$ in Fig. [ref], as calculated with a modified version of microMEGAs [ref] .
micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model · Dark Matter · 1.00
Uses data or values from 2 papers
-
[ref] , because the $Z'$ couples strongly to the electron ($Y'(e) = 3$).
A Combination of Preliminary Electroweak Measurements and Constraints on the Standard Model · Gauge Sector · 0.89
-
The measured relic density [ref] $Ω_χh^2 = 0.1123 ±0.0035$ can be obtained around either of the scalar $s$-channel resonances $M_χ≃m_i/2$, but for the $ϕ_1$-resonance one needs a large mixing angle $α$.
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation · Dark Matter · 1.00
Compares with 1 paper
-
The arising effects are nearly identical to the highly discussed minimal $B-L$ scalar sector [ref] , the main difference being a larger $Z'$ coupling to leptons, right-handed neutrinos and the scalar $s$; for these particles, $B-L$ results can be translated via $g'3 g'$, while the coupling strength to quarks does not change.
Phenomenology of the minimal B-L extension of the Standard model: Z' and neutrinos · Minimal Scalar Sector · 0.94
Cites as background 15 papers
-
As far as continuous abelian symmetries of lepton numbers go, three interesting linear combinations have been identified for the zeroth-order approximation: $$, $≡L_e - L_μ- L_τ$ and $$, leading to normal hierarchy (NH), inverted hierarchy (IH) and quasi-degeneracy in the neutrino mass spectrum [ref] .
A Flavor Symmetry for quasi-degenerate Neutrinos: L_mu-L_tau · Introduction · 0.91
-
The other two symmetries have been considered as global symmetries [ref] (or as an anomalous $U(1)$ [ref] ), but no effort has been put forward to construct a local version.
Vacuum Solutions of Neutrino Anomalies Through a Softly Broken U(1) symmetry · Introduction · 0.88
-
The other two symmetries have been considered as global symmetries [ref] (or as an anomalous $U(1)$ [ref] ), but no effort has been put forward to construct a local version.
Oscillations of solar and atmospheric neutrinos · Introduction · 0.88
Discussion
Know something about this paper? Leave a comment, or highlight any passage above to comment on it.