Three interactions of very different size act on the same electrons, and which you treat first decides which quantum numbers survive to label the answer.
§11.1a left carbon as — one configuration, one energy. That is not what a spectrometer sees. Carbon’s ground configuration contains fifteen states at five distinct energies, and this section recovers them.
Two corrections are responsible. The first is residual electron–electron repulsion residual electron–electron repulsion The part of the electron–electron interaction that no central potential can absorb. It splits a single configuration into several terms — carbon's (2p)² becomes ³P, ¹D and ¹S — because states of different exchange symmetry and different L keep the electrons apart to different degrees. defined in ch. 11 — open in glossary : the part of the repulsion that no central potential could absorb. The second is spin–orbit coupling, the same interaction §9.6 applied to hydrogen. Before either can be discussed, the states need better labels than a configuration.
Conventions first, because the notation is dense
Four rules, and the book states them as bullets because there is no deriving them:
Any angular momentum has magnitude and component , with any non-negative multiple of and running from down to in integer steps. Two of them combine (Eq. 8.6) to
Two ways to add up the angular momenta
An atom has several electrons, each with an and an . There are two sensible orders in which to combine them — – coupling l–s coupling Combine all the electrons' orbital angular momenta into L and all their spins into S, then couple L and S into J. Appropriate when residual electron–electron repulsion is larger than spin–orbit coupling — that is, for light atoms. Also called Russell–Saunders coupling. defined in ch. 11 — open in glossary and – coupling j–j coupling Couple each electron's own l and s into a j first, then combine the j's into J. Appropriate when spin–orbit coupling dominates residual repulsion, which is the case for heavy atoms. defined in ch. 11 — open in glossary — and which is right depends on which interaction is stronger.
Carbon’s fifteen states
Take and ask what is actually available.
The closed subshells contribute nothing. The two 1s electrons have a symmetric spatial wave function (both in the same orbital), so Eq. (10.23) forces an antisymmetric spin state — the singlet, . Their orbital angular momenta are both zero. Same for 2s. A closed subshell always has and can be ignored entirely.
So everything rests on the two 2p electrons. Each has , so Eq. (8.6) allows ; each has , so or . That is six combinations — and only three survive.
The reason is ch10’s, applied to orbital angular momentum instead of spin. The book states the orbital exchange symmetry:
and we already know is symmetric, antisymmetric. The total must be antisymmetric, so the two factors must have opposite symmetry:
which in term-symbol term symbol The label ^{2S+1}L_J: multiplicity 2S+1, a capital letter S, P, D, F for L = 0, 1, 2, 3, and total angular momentum J as a subscript. Carbon's ground term is ³P₀. CAUTION: the letter S for L = 0 is unrelated to the spin quantum number S in the superscript. defined in ch. 11 — open in glossary notation are , and .
| ML \ MS | +1 | 0 | -1 |
|---|---|---|---|
| +2 | · | 1 | · |
| +1 | 1 | 2 | 1 |
| 0 | 1 | 3 | 1 |
| -1 | 1 | 2 | 1 |
| -2 | · | 1 | · |
15 micro-states. Peeling removes one whole (2L+1)(2S+1) block at a time.
| term | L | S | (2S+1)(2L+1) | J = |L−S| … L+S |
|---|---|---|---|---|
| 1D | 2 | 0 | 1 × 5 = 5 | 1D2 |
| 3P | 1 | 1 | 3 × 3 = 9 | 3P0, 3P1, 3P2 |
| 1S | 0 | 0 | 1 × 1 = 1 | 1S0 |
| total | 15 | matches the micro-state count ✓ | ||
Why the missing terms are missing. With S = 1 the spins are parallel, so the two electrons must differ in ml — look at the MS = +1 column, which stops short of the top row. The largest ML available with parallel spins is 1, not 2, so no triplet with L = 2 can exist. Nothing was forbidden by hand; the table simply has no cell to build it from.
Three approximations, three orders of magnitude
Fig. 11.3 is the chapter’s best picture: the same configuration described three times, each more precisely than the last.
Selection rules
Most of what is known about atomic levels comes from the light emitted between them, and not every transition is allowed. §9.4 gave for one electron; for a many-electron atom the rules are richer.
Always, for electric dipole radiation:
And when – coupling describes the states well:
plus the parity rule: the parity must change. For a configuration the parity is even if is even and odd if that sum is odd.
Where this is going
Carbon’s ground state is : of the fifteen states, the one with the largest , then the largest , then the smallest for a less-than-half-filled subshell. That ordering rule is Hund’s, and its origin is ch10’s exchange integral — parallel spins keep electrons apart, which lowers the Coulomb energy.
§11.2 steps back down to configurations, where the periodic table lives, and none of this notation is needed again until you read a real spectrum.
Check yourself
0 / 6 answered
Two 2p electrons could in principle have combined with — six combinations.
1.Why do only three of them exist?
2.In the widget's micro-state table, why are the columns shorter than the column?
3.Fig. 11.3 splits the configuration by electronvolts and then by milli-electronvolts. Which interaction does which?
4.Why does spin–orbit coupling split into three levels but leave and alone?
5.Configuration gives three terms and gives six. What accounts for the difference?
6.The selection rule makes many transitions "forbidden". Does that mean they never happen?