Thermal Leptophilic Light Vector Dark Matter with Spinor Mediator and Muon (g-2) Anomaly
arXiv:2112.01029 · doi:10.1007/s10773-022-05252-1
Abstract
Inspired by the recently new measurement of at FermiLab and reported upper bound for electron-dark matter (DM) recoil by the XENON1T collaboration, we revisited phenomenology of a light MeV scale vector dark matter in a leptophilic extension of standard model while a new spinor field plays the role of mediator. A viable parameter space is considered to discuss the possibility of light dark matter relic density as well as anomalous magnetic moment of the muon. We study DM-electron direct detection and cosmological bounds on the parameters space of the model. It is shown that although new bound of anomaly greatly confines the parametric space of the model, the thermal light dark matter can exist for .
15 pages, 6 figures
References in corpus (16)
- Observation of an anomalous positron abundance in the cosmic radiation
- Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm
- The of charged leptons, and the hyperfine splitting of muonium
- Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
- Hadronic contribution to the muon anomalous magnetic moment to next-to-next-to-leading order
- The DArk Matter Particle Explorer mission
- Big Bang Nucleosynthesis as a Probe of New Physics
- The muon -2 and connection
- Energy Spectrum of Cosmic-ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station
- Electron and muon magnetic moments and implications for dark matter and model characterisation in non-universal supersymmetric models
- Non-Abelian Vector Dark Matter and Lepton
- General Kinetic Mixing in Gauged Model for Muon and Dark Matter
- Light dark matter, rare decays with missing energy in model with a scalar leptoquark
- The new and Right-Handed Sneutrino Dark Matter
- Muon g-2, Dark Matter and the Higgs mass in No-Scale Supergravity
- Scalar dark matter and Muon in a model