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Periodic Table from Quantum Mechanics

The periodic table is an empirical organization of the chemical elements by atomic number and recurring properties. Quantum mechanics explains why this recurrence is possible: a Coulomb-bound electron has discrete angular-momentum channels, electron spin doubles their one-particle capacity, fermionic antisymmetry limits their occupation, and electron–electron interactions turn those capacities into a nonhydrogenic sequence of valence structures.

That explanation is powerful but not a one-line derivation. Pauli exclusion does not determine which subshell fills next. The Madelung sequence is not an exact spectrum of the many-electron Hamiltonian. A ground-state configuration does not by itself determine chemistry. Periodicity emerges from several ingredients whose relative importance changes with nuclear charge, ionization state, and environment.

The useful summary is

  • symmetry and spin determine one-particle capacities;
  • Coulomb interactions produce screening and penetration;
  • antisymmetry and correlation organize term and configuration energies;
  • relativity supplies increasingly important heavy-atom corrections;
  • the environment creates new low-energy states and response scales.

This page owns the bridge from atomic quantum mechanics to periodic structure:

  • why ss, pp, dd, and ff blocks have capacities 22, 66, 1010, and 1414;
  • why period lengths are not simply the hydrogenic shell capacities 2n22n^2;
  • how screening and penetration produce recurring valence patterns;
  • how first and successive ionization energies expose shell closure;
  • why broad atomic and chemical trends have local reversals;
  • where correlation, relativity, and chemical environment limit a simple orbital picture.

Neighboring pages keep their canonical subjects. Electron Configurations owns occupation notation, the Aufbau construction, the Madelung mnemonic, and configuration mixing. Pauli Principle in Atoms owns antisymmetry and state counting. Central-Field Approximation owns the radial screening problem and effective-potential diagnostics. Hund’s Rules owns approximate term ordering within a declared configuration.

This page does not derive molecular bonding from isolated-atom configurations. It identifies the atomic energy and length scales that chemical bonding later reorganizes.

For a nucleus of charge +Ze+Ze and NN electrons, the clamped-nucleus nonrelativistic Hamiltonian in atomic units is

HZ(0)(N)=∑i=1N(−12∇i2−Zri)+∑i<jN1rij.H_Z^{(0)}(N) = \sum_{i=1}^{N} \left( -\frac{1}{2}\nabla_i^2 -\frac{Z}{r_i} \right) + \sum_{i<j}^{N} \frac{1}{r_{ij}}.

A neutral atom has N=ZN=Z. Moving one place to the right in the periodic table changes both the nuclear charge and the neutral-electron number:

(Z,N=Z)⟶(Z+1,N=Z+1).(Z,N=Z) \longrightarrow (Z+1,N=Z+1).

The Hamiltonians of adjacent elements are therefore different many-body problems. Periodicity means that their low-energy valence sectors recur approximately after compact core structures have formed; it does not mean that the full Hamiltonian or wavefunction repeats.

For quantitative heavy-atom work one adds nuclear recoil, relativistic interactions, finite-nuclear-size effects, and radiative corrections:

HZ=HZ(0)+Hrecoil+Hrel+HQED+⋯ .\begin{aligned} H_Z &= H_Z^{(0)} +H_{\mathrm{recoil}} +H_{\mathrm{rel}}\\ &\quad +H_{\mathrm{QED}} +\cdots . \end{aligned}

Chemical applications then add other nuclei, external fields, or an embedding environment. The boundary between an atomic trend and a chemical trend should always be stated.

IngredientStructural role and boundary
central rotational symmetryGives angular labels and magnetic degeneracy; it does not order interacting subshell energies.
electron spinGives two spin states per nonrelativistic spatial orbital; it does not choose the lowest spin coupling.
fermionic antisymmetryLimits each complete spin-orbital to one electron; it does not determine radial binding.
electromagnetic interactionsProduce binding, screening, exchange, relaxation, and correlation; they do not imply one environment-independent chemical rule.

The periodic table needs all four rows. Statements such as “Pauli explains the table” are useful only as shorthand for this larger structure.

In a spherical one-electron reference potential, a spin-orbital can be labeled schematically by

α=(n,ℓ,mℓ,ms),\alpha=(n,\ell,m_\ell,m_s),

with

mℓ=−ℓ,…,ℓ,ms=±12.m_\ell=-\ell,\ldots,\ell, \qquad m_s=\pm\frac12.

For a fixed orbital angular momentum ℓ\ell, there are 2ℓ+12\ell+1 magnetic orbitals and two spin projections. The nonrelativistic subshell capacity is therefore

gℓ=2(2ℓ+1).g_\ell = 2(2\ell+1).
Subshellℓ\ellSpatial orbitalsSpin-orbital capacity
ss001122
pp113366
dd22551010
ff33771414

These capacities explain the widths of the familiar blocks. They are exact state counts for the chosen central-field labels, even though the corresponding orbitals and their energies are approximate in a real atom.

For the Coulomb problem, all values

ℓ=0,1,…,n−1\ell=0,1,\ldots,n-1

occur at principal quantum number nn. Including spin gives

gn=∑ℓ=0n−12(2ℓ+1)=2n2.\begin{aligned} g_n &= \sum_{\ell=0}^{n-1}2(2\ell+1)\\ &= 2n^2. \end{aligned}

This is a degeneracy count for an ideal hydrogenic shell. It is not the sequence of observed period lengths. Electron–electron interactions remove the accidental hydrogenic degeneracy between different ℓ\ell values, and subshells with different nn then interleave in energy.

The conventional long-form table can be summarized by the subshell families that dominate each period:

PeriodNominal sequenceLength
11s1s22
22s, 2p2s,\ 2p88
33s, 3p3s,\ 3p88
44s, 3d, 4p4s,\ 3d,\ 4p1818
55s, 4d, 5p5s,\ 4d,\ 5p1818
66s, 4f, 5d, 6p6s,\ 4f,\ 5d,\ 6p3232
77s, 5f, 6d, 7p7s,\ 5f,\ 6d,\ 7p3232

This table is a structural map, not an assertion that every neutral ground configuration is obtained by rigidly filling orbitals in that printed order. Near-degenerate subshells rearrange, especially in the dd and ff regions.

For a complete spin-orbital α\alpha, the fermionic number operator has eigenvalues

nα∈{0,1}.n_\alpha\in\{0,1\}.

Consequently, at most gℓg_\ell electrons can occupy one nonrelativistic ℓ\ell subshell. Filled subshells have a particularly simple rotational structure, and recurring nearly filled or nearly empty valence subshells create recurring state spaces.

This counting does not compare 2s2s with 2p2p, 4s4s with 3d3d, or any other pair of orbital energies. Those comparisons require a Hamiltonian and a specified approximation. In particular:

  • Pauli exclusion forces electrons to occupy distinct complete modes;
  • the central field supplies candidate modes;
  • the interacting energy determines which admissible occupation pattern is lowest;
  • residual electrostatic and spin–orbit interactions determine the term and level within that pattern.

The distinction matters whenever an orbital-box diagram is used as if it were an energy calculation.

A central-field reference replaces the coupled electronic problem by radial equations of the form

−12d2Pnℓdr2+[ℓ(ℓ+1)2r2+Veff(r)]Pnℓ=εnℓPnℓ.\begin{aligned} -\frac12\frac{d^2P_{n\ell}}{dr^2} &+ \left[ \frac{\ell(\ell+1)}{2r^2} +V_{\mathrm{eff}}(r) \right]P_{n\ell}\\ &= \varepsilon_{n\ell}P_{n\ell}. \end{aligned}

The effective potential includes nuclear attraction and an averaged response of the other electrons. It is useful to define a radius-dependent effective charge by

Zeff(r)≡−rVeff(r).Z_{\mathrm{eff}}(r) \equiv -rV_{\mathrm{eff}}(r).

For a regular electronic density, the nuclear singularity dominates near the origin. Far outside an atom with charge q=Z−Nq=Z-N, a test electron sees the net charge of the nucleus plus the other N−1N-1 electrons:

Veff(r)∼−Zr,r→0,Veff(r)∼−q+1r,r→∞.\begin{aligned} V_{\mathrm{eff}}(r) &\sim -\frac{Z}{r}, &&r\to0,\\ V_{\mathrm{eff}}(r) &\sim -\frac{q+1}{r}, &&r\to\infty. \end{aligned}

For a neutral atom, the outer tail is therefore −1/r-1/r, not −Zeff/r-Z_{\mathrm{eff}}/r with one universal constant. A quoted scalar effective charge is an orbital- and model-dependent summary of a radial function.

The centrifugal term suppresses high-ℓ\ell amplitude near the nucleus:

Vcent(r)=ℓ(ℓ+1)2r2.V_{\mathrm{cent}}(r) = \frac{\ell(\ell+1)}{2r^2}.

At comparable principal scale, an ss orbital usually penetrates the core more strongly than a pp orbital, which penetrates more strongly than a dd or ff orbital. Greater penetration samples a less-screened nuclear attraction and tends to increase binding.

This qualitative ordering explains why nsns and npnp are split in multi-electron atoms even though hydrogenic energies depend only on nn. It also helps explain why an outer nsns family can begin a new period before the nominally lower-principal (n−1)d(n-1)d family has filled.

Penetration is a radial statement, not a claim that one orbital lives entirely “inside” another. Atomic radial densities overlap.

In an interacting atom, an orbital energy carries model and state dependence:

εnℓ=εnℓ[Z,N,ρ,configuration,approximation].\begin{aligned} \varepsilon_{n\ell} = \varepsilon_{n\ell} \bigl[ Z,N,\rho, &\text{configuration},\\ &\text{approximation} \bigr]. \end{aligned}

There is no fixed universal ladder that all neutral atoms traverse unchanged. As ZZ and NN increase together:

  1. compact occupied orbitals screen part of the nuclear charge;
  2. penetrating valence orbitals respond strongly to the increased ZZ;
  3. direct, exchange, and correlation energies change with occupation;
  4. orbital relaxation moves the reference energies;
  5. relativistic shifts grow and can reorder heavy-atom subshells.

The familiar filling sequence is therefore a successful pattern extracted from self-consistent atomic energetics and data, not an independent postulate of quantum mechanics.

Outside a compact core, the main-group patterns are approximately

alkali-like:[core] ns,alkaline earth:[core] ns2,p block:[core] ns2npq,q=1,…,6.\begin{gathered} \text{alkali-like:}\quad [\mathrm{core}]\,ns,\\ \text{alkaline earth:}\quad [\mathrm{core}]\,ns^2,\\ \text{p block:}\quad [\mathrm{core}]\,ns^2np^q,\\ q=1,\ldots,6. \end{gathered}

After an np6np^6 closure, the next low-energy valence electron often enters a more extended (n+1)s(n+1)s orbital. This resets several observables: the first ionization energy drops, the characteristic radius grows, and a one-electron-outside-a-core structure reappears.

Lithium and sodium are not copies. Their valence orbitals have different radial scales, polarizabilities, excitation energies, and core responses. They nevertheless share a low-energy one-valence-electron architecture, which is why their chemistry has a recognizable family resemblance.

Helium is an instructive exception to any purely outer-configuration rule. Its closed 1s21s^2 shell places it with the noble gases chemically even though the generic main-group closure is ns2np6ns^2np^6.

Transition regions contain near-degenerate subshells with different radial character:

nsand(n−1)d,ns \quad\text{and}\quad (n-1)d,

or

ns,(n−1)d,(n−2)f.ns,\quad (n-1)d,\quad (n-2)f.

Small changes in direct, exchange, correlation, or relativistic energy can then alter the leading neutral configuration. Ionization can reorder the same orbitals again; for many transition atoms, an nsns electron is removed before a (n−1)d(n-1)d electron even though the neutral Aufbau mnemonic placed nsns first.

The block label identifies the broad valence sector being developed. It does not guarantee a pure configuration, a unique oxidation state, or a simple monotonic property trend.

The first ionization energy is a total-energy difference between separately relaxed systems:

I1(Z)=EZ(N=Z−1)−EZ(N=Z).I_1(Z) = E_Z(N=Z-1) - E_Z(N=Z).

More generally, the kkth ionization energy is

Ik(Z)=EZ(Z−k)−EZ(Z−k+1).I_k(Z) = E_Z(Z-k) - E_Z(Z-k+1).

These equations define positive threshold energies when each EZ(N)E_Z(N) is the ground-state energy of the indicated charge sector. They make clear why an ionization energy is not, in general, just “the energy of the last electron.”

In frozen-orbital Hartree–Fock, Koopmans’ approximation gives

I1≈−εHOMOHF.I_1 \approx -\varepsilon_{\mathrm{HOMO}}^{\mathrm{HF}}.

The difference from experiment includes orbital relaxation and correlation, together with relativistic, recoil, and radiative corrections at the precision where they matter. An approximate orbital eigenvalue and an observed removal threshold are different objects.

First ionization energies from hydrogen through calcium, showing noble-gas peaks and alkali-metal resets

First ionization energies for neutral atoms with 1≤Z≤201\le Z\le20, using NIST ASD 5.12 evaluated values. The broad rise across each main-group period and the sharp drops after He, Ne, and Ar reveal periodic shell closure. Local reversals are physical many-electron effects, not measurement noise.

Across the second and third periods, the first ionization energy broadly rises as increasing nuclear charge contracts and binds the valence region. At a noble-gas closure it is relatively large. Adding the next electron begins a more diffuse ss family, producing the sharp He-to-Li, Ne-to-Na, and Ar-to-K drops.

The pattern is periodic, not monotonic. Four useful local comparisons are:

Pair and first ionization energiesMain qualitative lesson
Be, B: 9.322699, 8.298019 eV9.322699,\ 8.298019\ \mathrm{eV}The first 2p2p electron in B is easier to remove than a 2s2s electron from Be.
N, O: 14.53413, 13.618055 eV14.53413,\ 13.618055\ \mathrm{eV}Interaction and term energies make removal from 2p42p^4 easier than a smooth trend predicts.
Mg, Al: 7.646236, 5.985769 eV7.646236,\ 5.985769\ \mathrm{eV}The 3s3s-to-3p3p change repeats the Be–B mechanism.
P, S: 10.486686, 10.3600167 eV10.486686,\ 10.3600167\ \mathrm{eV}The half-filled and more-than-half-filled 3p3p sectors differ in exchange and relaxation energy.

Orbital penetration gives the first and third comparisons a useful starting intuition. The second and fourth require the many-electron terms of both the neutral atom and its ion. “Paired electrons repel” is too compressed to be a derivation: the measured threshold is a difference of two optimized correlated energies.

Neutral sodium has the leading structure [Ne] 3s[\mathrm{Ne}]\,3s. NIST gives

I1(Na)=5.13907696 eV,I2(Na)=47.28636 eV.\begin{aligned} I_1(\mathrm{Na}) &= 5.13907696\ \mathrm{eV},\\ I_2(\mathrm{Na}) &= 47.28636\ \mathrm{eV}. \end{aligned}

The large jump does not mean that a classical shell wall has been crossed. After the diffuse 3s3s electron is removed, the next threshold starts from the compact neon-like ion Na+\mathrm{Na}^+. Successive ionization energies are therefore a direct empirical probe of changing charge sectors and core closure.

A one-parameter estimate sometimes writes a valence binding scale as

Enℓeff∼−Zeff22(n∗)2.E_{n\ell}^{\mathrm{eff}} \sim -\frac{Z_{\mathrm{eff}}^2}{2(n^*)^2}.

Here n∗n^* may include a quantum defect, and ZeffZ_{\mathrm{eff}} is fitted or defined within a particular model. The expression is useful for trend reasoning but should not be inverted into a unique experimentally measured effective charge.

As ZZ increases while electrons enter the same broad valence shell:

  • core screening changes less rapidly than the nuclear charge;
  • the valence region generally contracts;
  • first ionization energies generally rise;
  • static polarizabilities generally fall;
  • electron-accepting and bond-polarizing tendencies often increase.

Every “generally” matters. Subshell changes, term structure, correlation, and relativistic effects create local reversals.

Moving down a group introduces a valence orbital with a larger principal radial scale:

  • the characteristic atomic size generally grows;
  • the outer electron is usually more screened and easier to remove;
  • excitation energies often decrease;
  • the electron cloud is often more polarizable.

Core penetration and relativistic contraction can weaken or reverse a naive extrapolation. The heavy 6s6s and 7s7s sectors, for example, cannot be understood quantitatively by scaling a nonrelativistic hydrogen orbital.

Chemistry compares energies of atoms, ions, molecules, solids, and their environments. An isolated neutral-atom configuration is useful input, but it is not the output of a bonding calculation.

Trend languageQuantum content and boundary
atomic sizeRadial density and response of a specified state; no single radius operator equals every tabulated atomic radius.
ionization energyA total-energy difference between charge sectors, not exactly one orbital eigenvalue.
electron affinityAn energy difference after attachment; some anions are weakly bound, metastable, or environment-stabilized.
electronegativityA tendency inferred from molecular or thermochemical data; several inequivalent scales exist.
polarizabilityAn induced-dipole response through excited states; it is tensorial and frequency-dependent in general.
oxidation stateAn electron-counting convention tied to bonding, not a direct isolated-atom observable.

For a nondegenerate isotropic atomic ground state, the static dipole polarizability has the spectral form

α(0)=23∑n≠0∣⟨n∣D∣0⟩∣2En−E0.\alpha(0) = \frac{2}{3} \sum_{n\ne0} \frac{ \left| \langle n|\mathbf D|0\rangle \right|^2 }{ E_n-E_0 }.

Diffuse valence states and low excitation gaps tend to increase α(0)\alpha(0). This helps connect the low first ionization energies of alkali atoms with their large response, but the relation is not an identity: transition matrix elements and the full excited spectrum also matter.

Elements in a group often present the same number and angular type of low-energy valence electrons outside a compact core. Their valence Hilbert spaces and dominant bonding channels then resemble one another.

The resemblance is approximate because the core changes:

  • radial nodes and characteristic length scales differ;
  • core polarization and core–valence correlation differ;
  • accessible dd or ff channels can enter;
  • spin–orbit coupling grows;
  • oxidation and bonding energies need not scale together.

Group membership is therefore a highly successful structural classification, not a symmetry equivalence between different elements.

Partially filled dd and ff subshells support many Pauli-allowed terms, several oxidation sectors, and dense low-energy spectra. Their chemistry depends on a competition among:

crystal or ligand fields,pairing and exchange,spin–orbit coupling,covalency and correlation.\begin{gathered} \text{crystal or ligand fields},\\ \text{pairing and exchange},\\ \text{spin–orbit coupling},\\ \text{covalency and correlation}. \end{gathered}

The lanthanide contraction is associated with increasing nuclear charge across the 4f4f series combined with incomplete screening by the compact 4f4f electrons; relativistic effects refine the quantitative trend. It is not evidence that screening disappears.

The microscopic Hamiltonian does not contain labels such as “group 1,” “halogen,” or “transition metal.” These classifications summarize recurring low-energy behavior after a hierarchy of scales has emerged.

An exact eigenstate can mix configuration-state functions with the same exact JJ and parity. The leading configuration may remain an excellent label, but a percentage attached to it depends on the orbital basis and model space.

When two configurations are near degenerate, small exchange, correlation, relaxation, or relativistic contributions can change their order. A universal n+ℓn+\ell rule cannot encode all of those species-dependent energy differences.

The characteristic relativistic parameter grows roughly as

Zα,Z\alpha,

with α\alpha the fine-structure constant. Direct relativistic contraction is strongest for orbitals with substantial nuclear penetration, especially s1/2s_{1/2} and p1/2p_{1/2} spinors, while indirect screening changes can expand other orbitals. Heavy-element trends therefore reflect a coupled relativistic many-electron response.

In a molecule or solid, spherical symmetry is broken and atomic orbitals hybridize into environment-dependent states. Ionization energies, electron affinities, ligand fields, band formation, and collective screening all participate. Free-atom periodicity remains a guide, not a substitute for solving the new system.

For short-lived superheavy nuclei, experimental chemistry can be atom-at-a-time and theory must combine relativistic electronic structure with nuclear lifetimes and production constraints. Predictions should be labeled as predictions, and uncertainty should not be hidden behind a familiar group label.

When using the periodic table as a quantum-mechanical argument:

  1. Name the system. Specify the element, isotope if relevant, charge state, and environment.
  2. Name the observable. Configuration, term, ionization threshold, radius, polarizability, and bond energy are different quantities.
  3. Separate counting from energetics. Use Pauli for capacities and a Hamiltonian for energy order.
  4. Choose the reference model. State whether orbitals come from a central field, Hartree–Fock, density-functional, or relativistic calculation.
  5. Use total-energy differences for thresholds. Include relaxation and correlation at the required accuracy.
  6. Treat filling rules as proposals. Verify near-degenerate configurations against calculation or evaluated spectroscopy.
  7. Check the regime. Relativity, open-shell correlation, and chemical environment can change the dominant picture.
  8. Compare with evaluated data. Preserve reported uncertainties and distinctions between measured, inferred, and calculated values.

This workflow turns a trend into a testable physical statement.

“The nth period contains 2n² elements”

Section titled ““The nth period contains 2n² elements””

The number 2n22n^2 counts all spin-orbitals in an ideal hydrogenic principal shell. Real periods follow interleaved subshell energies; period 3 ends after 3p63p^6, while 3d3d is developed in period 4.

Pauli limits admissible occupations. It does not compare the energies of different admissible configurations.

“Effective nuclear charge is Z minus the number of inner electrons”

Section titled ““Effective nuclear charge is Z minus the number of inner electrons””

That may be a rough mnemonic for a selected valence orbital. In a self-consistent atom, screening is radial, orbital dependent, and incomplete in overlapping regions.

“Ionization energy is minus the last orbital energy”

Section titled ““Ionization energy is minus the last orbital energy””

This is a model-dependent approximation. The exact threshold is a difference between states with different electron numbers.

A trend is a coarse-grained pattern. Local reversals encode subshell changes, term energies, relaxation, correlation, and relativity; they are part of the explanation.

“Atoms in one group have the same chemistry”

Section titled ““Atoms in one group have the same chemistry””

They share recurring valence structure, not identical Hamiltonians. Radial scale, accessible oxidation sectors, relativistic effects, and environment all evolve down a group.

“A neutral ground configuration specifies bonding”

Section titled ““A neutral ground configuration specifies bonding””

Bonding reorganizes the electronic state in the field of other nuclei or a solid. Atomic configurations are inputs and labels, not complete molecular wavefunctions.

Exercise 1: Derive the subshell and shell capacities

Section titled “Exercise 1: Derive the subshell and shell capacities”

Show that a nonrelativistic ℓ\ell subshell holds 2(2ℓ+1)2(2\ell+1) electrons. Then sum over ℓ=0,…,n−1\ell=0,\ldots,n-1 to obtain 2n22n^2.

Solution

There are 2ℓ+12\ell+1 possible values of mℓm_\ell and two values of msm_s. Pauli exclusion allows each complete spin-orbital only once, so

gℓ=2(2ℓ+1).g_\ell = 2(2\ell+1).

Summing the odd integers gives

gn=2∑ℓ=0n−1(2ℓ+1)=2n2.\begin{aligned} g_n &= 2\sum_{\ell=0}^{n-1}(2\ell+1)\\ &= 2n^2. \end{aligned}

The result counts a hydrogenic principal shell. It does not determine a period length once interactions split and interleave subshells.

Exercise 2: Why period 3 has eight elements

Section titled “Exercise 2: Why period 3 has eight elements”

Hydrogenic counting assigns the n=3n=3 shell a capacity of 1818. Explain why the third period nevertheless runs from Na to Ar and has length 88.

Solution

The n=3n=3 hydrogenic shell contains 3s3s, 3p3p, and 3d3d, with capacities

2+6+10=18.2+6+10=18.

In neutral multi-electron atoms, screening and penetration remove the hydrogenic degeneracy. The 4s4s valence family becomes relevant before the 3d3d family is developed across the neutral sequence. Period 3 therefore consists nominally of

3s2 3p6,3s^2\,3p^6,

with length 88. The 3d3d block appears between 4s4s and 4p4p in period 4. This is energetic interleaving, not a change in the state capacity of 3d3d.

An atom has nuclear charge ZZ, NN bound electrons, and ionic charge q=Z−Nq=Z-N. Determine the leading central potential seen by one electron near the nucleus and far outside the other N−1N-1 electrons.

Solution

Near the nucleus, the electronic Hartree-like potential is finite for a regular density, while the nuclear attraction is singular:

Veff(r)∼−Zr,r→0.V_{\mathrm{eff}}(r) \sim -\frac{Z}{r}, \qquad r\to0.

Far outside, the electron encloses the nucleus and the other N−1N-1 electrons. Their net charge is

Z−(N−1)=q+1,Z-(N-1) = q+1,

so

Veff(r)∼−q+1r,r→∞.V_{\mathrm{eff}}(r) \sim -\frac{q+1}{r}, \qquad r\to\infty.

For a neutral atom, q=0q=0 and the tail is −1/r-1/r. The interpolation between these limits is radial and cannot generally be replaced by one constant effective charge.

Exercise 4: Read the local ionization reversals

Section titled “Exercise 4: Read the local ionization reversals”

Use the table above to explain why I1(B)<I1(Be)I_1(\mathrm B)<I_1(\mathrm{Be}) and I1(O)<I1(N)I_1(\mathrm O)<I_1(\mathrm N) do not contradict the broad rise across period 2.

Solution

Boron begins the 2p2p subshell:

Be:1s2 2s2,B:1s2 2s2 2p.\mathrm{Be}:1s^2\,2s^2, \qquad \mathrm{B}:1s^2\,2s^2\,2p.

The 2p2p electron penetrates less strongly and is more weakly bound than a 2s2s electron in the neighboring system, so the first threshold drops at B.

Nitrogen and oxygen both ionize from 2p2p, but their many-electron terms differ. Nitrogen’s half-filled 2p32p^3 ground sector is strongly exchange stabilized. Removing one electron from oxygen’s 2p42p^4 sector produces the favorable 2p32p^3 ion. The exact comparison is still a difference of separately relaxed total energies; “pairing” is only shorthand for that term, exchange, and correlation balance.

Using the NIST values on this page, compute the ratio I2/I1I_2/I_1 for sodium and explain its physical meaning.

Solution

The ratio is

I2I1=47.286365.13907696≈9.20.\frac{I_2}{I_1} = \frac{47.28636}{5.13907696} \approx 9.20.

The first ionization removes the diffuse 3s3s valence electron. The second starts from the compact neon-like Na+\mathrm{Na}^+ ion and removes a core electron. The large ratio is evidence for a change in electronic sector and shell closure, not a literal discontinuity in a classical radial shell.

Why can −εHOMOHF-\varepsilon_{\mathrm{HOMO}}^{\mathrm{HF}} approximate an ionization energy, and what physics does the approximation omit?

Solution

In Hartree–Fock, removing an electron from an occupied canonical orbital while freezing every remaining orbital changes the determinant energy by the negative orbital eigenvalue. This is Koopmans’ construction:

I1frozen=−εHOMOHF.I_1^{\mathrm{frozen}} = -\varepsilon_{\mathrm{HOMO}}^{\mathrm{HF}}.

The actual ion relaxes: its orbitals and mean field reoptimize. Correlation energy also differs between the neutral atom and ion. Relativistic, recoil, and radiative effects may matter at higher precision. Thus the exact observable remains

I1=EZ(Z−1)−EZ(Z).I_1 = E_Z(Z-1)-E_Z(Z).

Lithium and sodium both have one ss electron outside a closed core. Give three reasons their atomic or chemical properties are not identical.

Solution

Any three of the following suffice:

  • Li uses a 2s2s valence orbital, while Na uses 3s3s; their radial nodes and sizes differ.
  • The closed cores have different polarizabilities and core-excitation spectra.
  • Their ionization and excitation energies differ.
  • Core–valence correlation and exchange differ.
  • Relativistic corrections, though modest here, are not identical.
  • Molecular bond energies depend on partner atoms and geometry, not only the isolated neutral configuration.

The shared one-valence-electron structure explains family resemblance. It does not define a symmetry mapping one element’s Hamiltonian into the other’s.

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  3. NIST Atomic Spectra Database, Ionization Energies Form, critically evaluated ground states and ionization thresholds, accessed 2026-07-21.
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  7. D. R. Hartree, “The Wave Mechanics of an Atom with a Non-Coulomb Central Field. Part I. Theory and Methods,” Proceedings of the Cambridge Philosophical Society 24, 89–110 (1928), doi:10.1017/S0305004100011919.
  8. V. Fock, “Näherungsmethode zur Lösung des quantenmechanischen Mehrkörperproblems,” Zeitschrift für Physik 61, 126–148 (1930), doi:10.1007/BF01340294.
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