Dark Matter and $(g-2)_{e,\mu}$ in ISS(2,3) based Gauged $U(1)_{L_{e}-L{\mu}}$ Symmetric Model
Rishu Verma, Ankush, B. C. Chauhan

TL;DR
This paper presents a unified model incorporating ISS(2,3), a $U(1)_{L_{e}-L_{}}$ gauge symmetry, explaining neutrino properties, dark matter, and the anomalous magnetic moments of electron and muon with testable TeV-scale physics.
Contribution
It introduces a minimal $U(1)_{L_{e}-L_{}}$ gauge symmetry integrated with ISS(2,3) to simultaneously address neutrino phenomenology, dark matter, and $(g-2)$ anomalies.
Findings
Viable dark matter candidate from sterile neutrino state.
MeV scale gauge boson explains $(g-2)_{e,}$ anomalies.
Neutrino phenomenology consistent with experimental data.
Abstract
We proposed a model which can explain the neutrino phenomenology, dark matter and anomalous magnetic moment in a common framework. The inverted sea saw (ISS)(2,3) mechanism has been incorporated, in which we get an extra sterile state and this state act as a viable dark matter candidate. The right handed neutrino mass is obtained in TeV scale, which is accessible at LHC. The anomaly free gauge symmetry is introduced to explain the anomalous magnetic moment of electron and muon because it provides a natural origin of in a very minimal setup. The corresponding MeV scale gauge boson successfully explain the anomalous magnetic moment of electron and muon, simultaneously. Thus obtained neutrino phenomenology and relic abundance of dark matter are compatible with experimental results.
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Computational Physics and Python Applications · Dark Matter and Cosmic Phenomena
