Relativistic Correction to the Magnetic Moment of the Charged Lepton
arXiv:2501.07610 · doi:10.1088/1402-4896/ae1170
Abstract
We derive a general relativistic Hamiltonian valid for both bound and scattering systems by reducing the four-component Dirac equation to a two-component Dirac-Pauli form. Unlike conventional approaches, our formulation includes first-order relativistic corrections in a compact, gauge-consistent expression applicable to arbitrary electromagnetic fields - including non-uniform and time-dependent configurations. As an application, we compute the O(alpha^2) relativistic correction to the Lande g-factor in hydrogen-like atoms, revealing a novel mj^2-dependent term that generalizes the Breit result. This correction is experimentally testable in Penning trap spectroscopy. We further show that relativistic effects become comparable to QFT corrections in highly charged ions where Z ~ 1/sqrt(alpha)
References in corpus (16)
- The anomalous magnetic moment of the muon in the Standard Model
- Physics of Strongly Magnetized Neutron Stars
- Measurement of the Positive Muon Anomalous Magnetic Moment to 0.20 ppm
- High-precision measurement of the atomic mass of the electron
- Complete two-loop correction to the bound-electron g factor
- The anomalous magnetic moment of the muon in the Standard Model: an update
- Proton size anomaly
- Nonrelativistic QED approach to the bound-electron g factor
- Direct Bound-Electron factor Difference Measurement with Coupled Ions
- Recent progress on the description of relativistic spin: vector model of spinning particle and rotating body with gravimagnetic moment in General Relativity
- -factor of Boronlike Argon
- Electron self-energy in the presence of magnetic field: hyperfine splitting and g factor
- Relativistic corrections to the algebra of position variables and spin-orbital interaction
- Binding two-loop vacuum-polarization corrections to the bound-electron g factor
- QED calculations of the nuclear recoil effect on the bound-electron factor
- Relativistic Calculation of Energies, Transition Parameters Hyperfine Structure, Landé g and Isotope shifts factors for Ar, Kr and Xe ions