Lepton number violation and $h\to \gamma\gamma$ in a radiative inverse seesaw dark matter model

Bo Ren; Gang Guo; Guan-Nan Li; Xiao-Gang He; Ya-Juan Zheng

RECORD

Lepton number violation and $h\to \gamma\gamma$ in a radiative inverse seesaw dark matter model

Guan-nan Li, Gang Guo, Bo Ren, Ya-Juan Zheng, Xiao-Gang He

High Energy Physics - Phenomenology · Submitted 21 Dec 2012

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim The model is able to explain the deviation between the SM prediction and the LHC data.

how it is stated · asserted 0.92 read the record →

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arXiv ID1212.5528 (version 4)

Pith IDVFHL3RFD, Pith's permanent record of this paper and its review

CitationBo Ren, Gang Guo, Guan-Nan Li, Xiao-Gang He, Ya-Juan Zheng. "Lepton number violation and $h\to \gamma\gamma$ in a radiative inverse seesaw dark matter model." arXiv:1212.5528 (2012). https://pith.science/paper/VFHL3RFD

Claim paper

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.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,058 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.13 · randomized assignment 0.01 · states quantitative result 0.47 · compares with prior results 0.52 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v4. Results and the main claim are underlined; show every role.

We study phenomenological implications of a radiative inverse seesaw dark matter model. In this model, because neutrino masses are generated at two loop level with inverse seesaw, the new physics mass scale can be as low as a few hundred GeV and the model also naturally contain dark matter candidate. The Yukawa couplings linking the SM leptons and new particles can be large. This can lead to large lepton flavor violating effects. We find that future experimental data on $\mu \to e \gamma$ and $\mu - e$ conversion can further test the model. The new charged particles can affect significantly the $h \to \gamma \gamma$ branching ratio in the SM. The model is able to explain the deviation between the SM prediction and the LHC data. We also study some LHC signatures of the new particles in the model.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	We study phenomenological implications of a radiative inverse seesaw dark matter model.	contribution 1.00	0.91	0.06	asserted 0.79
s1	In this model, because neutrino masses are generated at two loop level with inverse seesaw, the new physics mass scale can be as low as a few hundred GeV and the model also naturally contain dark matter candidate.	method 0.44	0.23	0.09	asserted 0.72
s2	The Yukawa couplings linking the SM leptons and new particles can be large.	background 0.46	0.26	0.03	asserted 0.91
s3	This can lead to large lepton flavor violating effects.	interpretation 0.69	0.33	0.07	hedged possibility 0.88
s4	We find that future experimental data on $\mu \to e \gamma$ and $\mu - e$ conversion can further test the model.	result 0.41	0.90	0.13	asserted 0.91
s5	The new charged particles can affect significantly the $h \to \gamma \gamma$ branching ratio in the SM.	result 0.94	0.53	0.19	asserted 0.60
s6	The model is able to explain the deviation between the SM prediction and the LHC data.	result 0.71	0.74	0.33	asserted 0.92
s7	We also study some LHC signatures of the new particles in the model.	contribution 1.00	0.91	0.06	asserted 0.91

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from argument 0.49.

What was examined, and what was not

sources read

arXiv listing abstract v4

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

We study phenomenological implications of a radiative inverse seesaw dark matter model. In this model, because neutrino masses are generated at two loop level with inverse seesaw, the new physics mass scale can be as low as a few hundred GeV and the model also naturally contain dark matter candidate. The Yukawa couplings linking the SM leptons and new particles can be large. This can lead to large lepton flavor violating effects. We find that future experimental data on $\mu \to e \gamma$ and $\mu - e$ conversion can further test the model. The new charged particles can affect significantly the $h \to \gamma \gamma$ branching ratio in the SM. The model is able to explain the deviation between the SM prediction and the LHC data. We also study some LHC signatures of the new particles in the model.

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References

How the literature uses it

3 arXiv papers cite this in 4 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 3 sentences without a confident label

Cites it as background 1 paper

Some similar scenarios have already been explored in Refs. [ref] .

New Scalar Contributions to $h\to Z\gamma$ · Introduction · 0.94

What it cites · 15 sentences without a confident label

Builds on 1 paper

The model we will study is the $U(1)_D$ model discussed in Ref. [ref] .

Radiative Two Loop Inverse Seesaw and Dark Matter · Introduction · 0.83

Uses data or values from 4 papers

The experimental value [ref] for this channel is $1.8±0.5$ (ATLAS) ($1.56±0.43$(CMS)) times that predicted by the SM.

Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC · $h →γγ$ · 0.94
In our later calculations we will use the central values from recent global fit data in Ref. [ref] for neutrino mixing angles and mass squared differences for both normal and inverted hierarchies (NH and IH) for our discussions [equation]

Global analysis of neutrino masses, mixings and phases: entering the era of leptonic CP violation searches · Neutrino masses and LFV · 1.00
We have [ref] [equation] where [equation] and [equation] The parameters $D(A)$, $V^(p,n)(A)$ are nuclei dependent quantities.

$\mu - e$ Conversion With Four Generations · Neutrino masses and LFV · 0.82

Cites as background 1 paper

There have been extensive studies for similar triplet scalar contributions to $h →γγ$ [ref] .

New Scalar Contributions to $h\to Z\gamma$ · $h →γγ$ · 0.99

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