Inner-shell electrons partly cancel the nucleus's pull on a valence electron by repelling it -- this is the shielding (screening) effect -- so the net attractive charge a valence electron actually feels, the effective nuclear charge, is less than the full nuclear charge:
Zeff=Z−S
where S, the screening constant, is estimated by Slater's rules:
- Group the electron configuration as (1s)(2s,2p)(3s,3p)(3d)(4s,4p)(4d)(4f)(5s,5p)…
- Electrons in a group to the right of the electron of interest contribute nothing; electrons in the same group contribute 0.35 each (0.30 if the electron of interest is 1s).
- For an s or p electron of interest: electrons one group inward (n−1) contribute 0.85 each; electrons two or more groups inward contribute the full 1.00 each. For a d or f electron of interest: every electron to its left contributes the full 1.00, with no intermediate 0.85 tier.
- Sum all contributions to get S.
Worked on scandium (Z=21, config (1s)2(2s,2p)8(3s,3p)8(3d)1(4s)2): the 4s electron feels S=(1)(0.35)+(9)(0.85)+(10)(1.00)=18.00, giving Zeff=3; the 3d electron feels S=(0)(0.35)+(18)(1.00)=18 (the two 4s electrons sit to the right of 3d in the Slater ordering and so do not shield it at all), also giving Zeff=3.
Slater's rules are the mechanism behind both major radius/energy trends: effective nuclear charge rises across a period (driving atomic radius down and ionisation energy up) and the growing number of inner shells down a group increases total shielding (driving atomic radius up and ionisation energy down). The same Slater Zeff calculation, applied to an ion rather than a neutral atom, is also the basis of Pauling's method for finding ionic radii.