Relativistic Contributions to the Magnetic Moment ofS13Helium

Abstract
Some relativistic contributions of order α2(137)2 to the magnetic moment of helium in the lowest-energy triplet state S13 have been calculated. These contributions arise from the effect of the electrostatic and Breit interactions in a relativistic wave equation. The purpose of the calculation was to isolate to order α2 the quantum-electrodynamic radiative contributions to the magnetic moment of a bound two-electron system for comparison with experiment. The method of calculation was to evaluate the sixteen-component form of the matrix element of magnetic interaction energy in terms of nonrelativistic wave functions in Pauli approximation and to use the angular and spin symmetry properties of the S13 state. This procedure was possible because Russell-Saunders coupling in the Pauli approximation could be shown to hold rigorously to order α2. The result derived was that the g value for two interacting electrons bound in a S13 state is 2(113T16e2r12) where T is the expectation value of total kinetic energy and e2r12 of electrostatic interaction in the S13 state, in units mc2. The contribution 13T corresponds to the Breit-Margenau result for one electron and 16e2r12 arises from the Breit interaction. For S13 helium the preceding g value was evaluated numerically as 2[1-(38.7+2.3)×106]. Comparison of theory and experiment tends to substantiate the nonradiative contribution 13T and the additivity properties of radiative and nonradiative contributions to the magnetic moment of S13 helium. The fourth-order radiative contribution is not contradicted. The Breit interaction contribution is too small to be noticed, with the present experimental error.

This publication has 29 references indexed in Scilit: