§11.3What If? — a world without the Pauli principle

Part IV Phillips pp. 241–246 · ~14 min read

  • electron–electron avoidance parameter
  • Pauli exclusion principle

Delete one rule and rebuild the periodic table. Everything else in the theory is left untouched, so whatever changes can only have been the exclusion principle holding it up.

§11.2 built the periodic table from two ideas. One of them — that electrons occupy orbitals with definite energies — is ordinary quantum mechanics. The other is the Pauli exclusion principle , which has no classical analogue at all: it is a statement about the symmetry of a wave function under relabelling.

So the book ends by asking the obvious question. What would atoms be like without it?

The answer is not a hand-wave. It is a calculation, built on nothing more than the uncertainty principle and Coulomb’s law, and it produces a specific prediction that can be laid beside the measured properties of real atoms.

The model: two terms and a minimum

Confine an electron to a region of size RR around a nucleus of charge ee. Its potential energy is about

Vˉe24πϵ0R\bar V \approx -\frac{e^2}{4\pi\epsilon_0 R}

and its kinetic energy cannot be less than the localization cost. The uncertainty principle gives Δp/R\Delta p \gtrsim \hbar/R, and since the average momentum is comparable to its own uncertainty,

Tˉ22meR2\bar T \approx \frac{\hbar^2}{2m_eR^2}

So the total is

E22meR2e24πϵ0R(11.9)E \approx \frac{\hbar^2}{2m_eR^2} - \frac{e^2}{4\pi\epsilon_0 R}\tag{11.9}

which the book abbreviates

E=A1R2B1R,A1=22me,B1=e24πϵ0(11.10–11.11)E = \frac{A_1}{R^2} - \frac{B_1}{R}, \qquad A_1 = \frac{\hbar^2}{2m_e}, \quad B_1 = \frac{e^2}{4\pi\epsilon_0}\tag{11.10–11.11}

Minimising it — and hydrogen falls out exactly

step 1 of 4

Two competing terms: localization is expensive and attraction is cheap, and they scale differently with R. One derivative finds the balance.

  1. 1Write the energy as a function of one variable. The 1/R-squared term is the cost of squeezing the electron; the 1/R term is the reward for keeping it near the nucleus.

    At large R the attraction dominates and E rises toward zero; at small R the kinetic cost blows up. So there is a minimum in between, and that is the atom.

E1=ER=13.6 eVandR1=a0(11.12–11.13)E_1 = -E_R = -13.6\ \mathrm{eV} \qquad\text{and}\qquad R_1 = a_0\tag{11.12–11.13}

Helium, and the one fitted number

Two electrons around a nucleus of charge 2e2e, both in the same single-particle state — which is allowed, since two electrons of opposite spin may share an orbital:

E2222meR24e24πϵ0R+e24πϵ0Ree(11.14)E_2 \approx 2\frac{\hbar^2}{2m_eR^2} - 4\frac{e^2}{4\pi\epsilon_0 R} + \frac{e^2}{4\pi\epsilon_0 R_{ee}}\tag{11.14}

Two kinetic terms; attraction 2×2e22 \times 2e^2; and one new term, the repulsion between the electrons themselves at separation ReeR_{ee}. That separation is not known, so the book parametrizes it:

Ree=fR(11.15)R_{ee} = fR\tag{11.15}

where ff is the electron–electron avoidance parameter — expected to be around 1, and larger than 1 if the electrons are good at keeping apart. With that,

E=A2R2B2R,A2=2A1,B2=(41f)B1(11.16–11.17)E = \frac{A_2}{R^2} - \frac{B_2}{R}, \qquad A_2 = 2A_1, \quad B_2 = \left(4 - \frac{1}{f}\right)B_1\tag{11.16–11.17}

and the same minimisation gives

E2=(41f)22ERR2=241fa0(11.18)E_2 = -\frac{\left(4 - \tfrac1f\right)^2}{2}E_R \qquad R_2 = \frac{2}{4 - \tfrac1f}\,a_0\tag{11.18}

Now remove the Pauli principle

Here is the move the whole section exists for. Put all ZZ electrons in the same single-particle state. Nothing in electrostatics forbids it; only Pauli does, and Pauli is what we are removing.

There are now ZZ kinetic terms, an attraction Z×Ze2Z \times Ze^2, and 12Z(Z1)\tfrac12 Z(Z-1) pairs each repelling:

EZ22meR2Ze24πϵ0R[Z2Z(Z1)2f](11.19–11.21)E_Z \approx \frac{\hbar^2}{2m_eR^2}Z - \frac{e^2}{4\pi\epsilon_0R}\left[Z^2 - \frac{Z(Z-1)}{2f}\right]\tag{11.19–11.21}

Minimising exactly as before:

EZ=[Z2Z(Z1)2f]2ZERRZ=ZZ2Z(Z1)2fa0(11.22)E_Z = -\frac{\left[Z^2 - \frac{Z(Z-1)}{2f}\right]^2}{Z}E_R \qquad R_Z = \frac{Z}{Z^2 - \frac{Z(Z-1)}{2f}}\,a_0\tag{11.22}

Removing one electron gives the corresponding ion (problem 8),

EZ=[Z(Z1)(Z1)(Z2)2f]2Z1ER(11.23)E_{Z^-} = -\frac{\left[Z(Z-1) - \frac{(Z-1)(Z-2)}{2f}\right]^2}{Z-1}E_R\tag{11.23}

and the ionization energy is the difference:

EI=EZEZ(11.24)E_I = E_{Z^-} - E_Z\tag{11.24}

which the book fits with

EI(0.07Z2+0.57Z+0.36)ERRZ10.7Z+0.3a0(11.25)E_I \approx (0.07Z^2 + 0.57Z + 0.36)E_R \qquad R_Z \approx \frac{1}{0.7Z + 0.3}\,a_0\tag{11.25}

Look at the form of those. The ionization energy grows like Z2Z^2 — smoothly, monotonically, forever. The radius shrinks like 1/Z1/Z — smoothly, monotonically, forever. There is no structure in either, because there is nothing in the model that could produce structure.

Fig. 11.5 — atoms with the Pauli principle, and atoms without it
0481216HHeLiBeBCNOFNeNaatomic number Zionization energy (E_R)
0123HHeLiBeBCNOFNeNaatomic number Zradius (a₀)
real atoms — Pauli in forcehypothetical atoms — no Pauli principle
helium, the atom that fixes f: E = -5.78 E_R, R = 0.588 a₀ vs measured 5.81 and 0.586
lithium, where they part: 2.71 vs 0.40 E_R — a factor of 6.8

Move f and watch what does not change. The hypothetical curve shifts up and down, but it never develops a kink — no value of f produces a peak at helium or a collapse at lithium, because a model in which every electron occupies the same state has no shell to close. The measured points oscillate; the model cannot. That gap is the Pauli principle, and it is the whole of chemistry. Note also that hydrogen and helium sit on top of each other in both panels: with one electron, or two in the same state, Pauli forbids nothing and the hypothetical atom is the real one. They separate at lithium — the first element whose third electron has nowhere legal to go.

What the world would be like

Read the two panels as a chemist would.

Without the Pauli principle, ionization energy rises steadily with ZZ and radius falls steadily. There are no families. Nothing is especially inert and nothing is especially reactive; each element is simply a slightly smaller, slightly more tightly bound version of the one before. Every atom would be less reactive than helium, and getting steadily more so.

There would be no valence, because valence is about what sits outside a closed shell and nothing ever closes. There would be no periodic table, because there is no period. There would be no ionic bonding, because that needs one atom eager to give and another eager to take.

The book’s closing line is worth quoting exactly:

A world without the Pauli exclusion principle would be very different. One thing is for certain: it would be a world with no chemists.

The problems extend the model to ions — problem 9 applies it to seven two-electron ions and reproduces every measured ionization energy to within about half a per cent, which is a striking return for a model with one fitted constant.

Check yourself

0 / 6 answered

  1. 1.The model of §11.3 reproduces hydrogen's binding energy and radius exactly, with no fitted parameter. Why should you not be too impressed?

  2. The avoidance parameter is defined by and fitted to helium at .

    2.What is standing in for?

  3. 3.In Fig. 11.5 the hypothetical and real curves coincide at and . Why is that reassuring rather than suspicious?

  4. 4.Moving the slider changes the hypothetical curve's height but never its shape. Why does that matter more than the numerical disagreement?

  5. 5.Without the Pauli principle, what would chemistry look like?

  6. 6.This section is the site's closing argument. What is it really measuring?