Litcius/Paper detail

Neutrino phenomenology, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>W</mml:mi></mml:math>-mass anomaly, and muon (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>−</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math>) in a minimal type-III seesaw model using a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math> modular symmetry

Priya Mishra, Mitesh Kumar Behera, Rukmani Mohanta

2023Physical review. D/Physical review. D.21 citationsDOIOpen Access PDF

Abstract

In this study, we introduce a model to illustrate neutrino phenomenology by incorporating two right-handed fermion triplet superfields, i.e., ${\mathrm{\ensuremath{\Sigma}}}_{{R}_{j}}$, in the presence of the modular symmetry ${\mathrm{\ensuremath{\Gamma}}}_{3}^{\ensuremath{'}}\ensuremath{\simeq}{A}_{4}^{\ensuremath{'}}$, a double cover of the ${A}_{4}$ modular symmetry. The motivation in utilizing double cover is that, so far, only even modular forms have been considered for constructing modular invariant models, but, in this case, it is possible to extend the modular invariance approach to general integral weight modular forms, i.e., the odd weight modular forms. Hence, this type of amalgamation between ${T}^{\ensuremath{'}}$ modular symmetry and minimally extending the seesaw can correctly explain the neutrino phenomenology. Additionally, we accommodate the most recent measurement of the $W$-boson mass, published by the CDF-II Collaboration, and shed some light on the recent results of muon ($g\ensuremath{-}2$). Finally, we discuss lepton flavor violation in order to establish a constraint on the mass of right-handed fermion.

Topics & Concepts

MuonNeutrinoPhenomenology (philosophy)PhysicsParticle physicsPhilosophyEpistemologyParticle physics theoretical and experimental studiesNeutrino Physics ResearchAstrophysics and Cosmic Phenomena
Neutrino phenomenology, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>W</mml:mi></mml:math>-mass anomaly, and muon (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>−</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math>) in a minimal type-III seesaw model using a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math> modular symmetry | Litcius