Abstract
In connection with a recent experiment of Sandars and Stewart, the atomic quadrupole moments for the excited states np5ns (n=n+1) of the rare gases have been calculated, in particular, the induced moment due to the nsd excitation produced by the quadrupole potential due to the vacancy in the np shell. Sandars and Stewart have written the total quadrupole moment Θatom as: Θatom=Θ(np)(1RΘ), where Θ(np) is the quadrupole moment due to the np vacancy, and RΘ is a suitable shielding factor associated with nsd. In the present work, RΘ was calculated by obtaining the perturbation ν1(nsd) of the ns wave function due to the quadrupole potential of the np vacancy. It was found that the calculated values of RΘ are in very good agreement with the experimental values for all four cases (Ne, Ar, Kr, and Xe). The calculated values of RΘ range from 0.82 for Ne to 1.33 for Xe, in good agreement with the experimental results.