Constraining the new contributions to electron <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>g</mml:mi> <mml:mo>−</mml:mo> <mml:mn>2</mml:mn> </mml:math> in a radiative neutrino mass model

We examine electron and muon anomalous magnetic dipole moments within a radiative neutrino mass model featuring TeV-scale scalar leptoquarks <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>S</a:mi> <a:mo stretchy="false">(</a:mo> <a:mn>3</a:mn> <a:mo>,</a:mo> <a:mn>1</a:mn> <a:mo>,</a:mo> <a:mo>−</a:mo> <a:mn>1</a:mn> <a:mo>/</a:mo> <a:mn>3</a:mn> <a:mo stretchy="false">)</a:mo> </a:math> and <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:mi>R</e:mi> <e:mo stretchy="false">(</e:mo> <e:mn>3</e:mn> <e:mo>,</e:mo> <e:mn>2</e:mn> <e:mo>,</e:mo> <e:mn>1</e:mn> <e:mo>/</e:mo> <e:mn>6</e:mn> <e:mo stretchy="false">)</e:mo> </e:math> . We utilize textures with decoupling electron and muon sectors, so that both electron and muon anomalous magnetic dipole moments could receive internal chiral enhancements from different heavy up-type quarks while in the same time evading the stringent <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"> <i:mi>μ</i:mi> <i:mo stretchy="false">→</i:mo> <i:mi>e</i:mi> <i:mi>γ</i:mi> </i:math> constraint. A successful fit to neutrino oscillation data requires the simultaneous presence of one- and two-loop neutrino mass contributions. This severely constrains the parameter space of the model, which results in a negligible new physics correction to the muon <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"> <l:mi>g</l:mi> <l:mo>−</l:mo> <l:mn>2</l:mn> </l:math> . The electron <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"> <n:mi>g</n:mi> <n:mo>−</n:mo> <n:mn>2</n:mn> </n:math> discrepancy implied by the rubidium experiment, on the other hand, can be resolved within <p:math xmlns:p="http://www.w3.org/1998/Math/MathML" display="inline"> <p:mn>2</p:mn> <p:mi>σ</p:mi> </p:math> uncertainty provided that neutrino mass ordering is inverted. Lepton-flavor-violating tau decay rates, such as <r:math xmlns:r="http://www.w3.org/1998/Math/MathML" display="inline"> <r:mi>τ</r:mi> <r:mo stretchy="false">→</r:mo> <r:mi>e</r:mi> <r:mi>γ</r:mi> </r:math> and <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mi>τ</u:mi> <u:mo stretchy="false">→</u:mo> <u:mn>3</u:mn> <u:mi>e</u:mi> </u:math> , are predicted to be within the sensitivities of next-generation experiments.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2026-01-29
DOI
https://doi.org/10.1103/ptm1-rmsm
Primary Topic
Particle physics theoretical and experimental studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Constraining the new contributions to electron <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>g</mml:mi> <mml:mo>−</mml:mo> <mml:mn>2</mml:mn> </mml:math> in a radiative neutrino mass model

Bayu Dirgantara, J. Julio
Physical review. D/Physical review. D.
Particle physics theoretical and experimental studies
article

Constraining the new contributions to electron <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>g</mml:mi> <mml:mo>−</mml:mo> <mml:mn>2</mml:mn> </mml:math> in a radiative neutrino mass model

Bayu Dirgantara, J. Julio
article en

Abstract

We examine electron and muon anomalous magnetic dipole moments within a radiative neutrino mass model featuring TeV-scale scalar leptoquarks <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>S</a:mi> <a:mo stretchy="false">(</a:mo> <a:mn>3</a:mn> <a:mo>,</a:mo> <a:mn>1</a:mn> <a:mo>,</a:mo> <a:mo>−</a:mo> <a:mn>1</a:mn> <a:mo>/</a:mo> <a:mn>3</a:mn> <a:mo stretchy="false">)</a:mo> </a:math> and <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:mi>R</e:mi> <e:mo stretchy="false">(</e:mo> <e:mn>3</e:mn> <e:mo>,</e:mo> <e:mn>2</e:mn> <e:mo>,</e:mo> <e:mn>1</e:mn> <e:mo>/</e:mo> <e:mn>6</e:mn> <e:mo stretchy="false">)</e:mo> </e:math> . We utilize textures with decoupling electron and muon sectors, so that both electron and muon anomalous magnetic dipole moments could receive internal chiral enhancements from different heavy up-type quarks while in the same time evading the stringent <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"> <i:mi>μ</i:mi> <i:mo stretchy="false">→</i:mo> <i:mi>e</i:mi> <i:mi>γ</i:mi> </i:math> constraint. A successful fit to neutrino oscillation data requires the simultaneous presence of one- and two-loop neutrino mass contributions. This severely constrains the parameter space of the model, which results in a negligible new physics correction to the muon <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"> <l:mi>g</l:mi> <l:mo>−</l:mo> <l:mn>2</l:mn> </l:math> . The electron <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"> <n:mi>g</n:mi> <n:mo>−</n:mo> <n:mn>2</n:mn> </n:math> discrepancy implied by the rubidium experiment, on the other hand, can be resolved within <p:math xmlns:p="http://www.w3.org/1998/Math/MathML" display="inline"> <p:mn>2</p:mn> <p:mi>σ</p:mi> </p:math> uncertainty provided that neutrino mass ordering is inverted. Lepton-flavor-violating tau decay rates, such as <r:math xmlns:r="http://www.w3.org/1998/Math/MathML" display="inline"> <r:mi>τ</r:mi> <r:mo stretchy="false">→</r:mo> <r:mi>e</r:mi> <r:mi>γ</r:mi> </r:math> and <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mi>τ</u:mi> <u:mo stretchy="false">→</u:mo> <u:mn>3</u:mn> <u:mi>e</u:mi> </u:math> , are predicted to be within the sensitivities of next-generation experiments.

Physical review. D/Physical review. D.Vol. 113(3)
National Research, Development and Innovation Office (HU), National Research and Innovation Agency (ID), Suranaree University of Technology (TH), Hasanuddin University (ID)
Badan Riset dan Inovasi Nasional
Openalex Percentile: Top 97%
Particle physics theoretical and experimental studies
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