Pairing Energy and Magnetic Moments

Hold a small vial of [Fe(H2O)6]2+\text{[Fe(H}_2\text{O)}_6\text{]}^{2+} near a strong magnet. It visibly tugs toward the poles. Do the same with [Fe(CN)6]4−\text{[Fe(CN)}_6\text{]}^{4-}, and nothing happens. Both are octahedral iron(II) complexes. They share the same metal, oxidation state, and six-coordinate geometry. Yet one is paramagnetic and one is not. The difference is not the number of electrons. That number is identical in both (six dd-electrons). Instead, it is how those six electrons are distributed among the dd-orbitals. That distribution is decided by a single energetic contest. The crystal field splitting energy Δo\Delta_o competes against the electron pairing energy PP. This article is about making that contest quantitative. Magnetism in transition-metal complexes is one of the few places in inorganic chemistry where a bench measurement reads out microscopic electronic structure almost directly. That measurement is the Gouy or Evans-method magnetic moment. A measured μeff\mu_{\text{eff}} of 4.9 μB\mu_B versus 0 μB\mu_B for the same d6d^6 ion is not a subtlety. It is a fingerprint of whether Δo\Delta_o exceeds PP or not. Getting from "d6d^6, octahedral" to "paramagnetic or diamagnetic" requires exactly three ingredients. First, a rule for counting unpaired electrons given a high-spin or low-spin configuration. Second, a formula connecting that count to a predicted magnetic moment. Third, a physical account of what pairing energy actually costs in Coulomb and exchange terms. This third ingredient lets the high-spin/low-spin choice itself be predicted rather than assumed. The intellectual payoff is large relative to the arithmetic required. Once you have the spin-only formula μeff=n(n+2) μB\mu_{\text{eff}} = \sqrt{n(n+2)}\,\mu_B, you can predict the moments of essentially every first-row octahedral and tetrahedral complex you will meet. You can then check those predictions against real data. Once you have the decomposition of PP into a Coulombic part Πc\Pi_c and an exchange part Πe\Pi_e, you can explain something important. You can explain why pairing is expensive specifically for electrons that would otherwise occupy different orbitals with parallel spin. You can also explain why the pairing energy is a property of the free ion. It is tabulated and depends on dd-electron count. This property competes against a ligand-and-geometry-dependent Δo\Delta_o. This piece builds outward from High-Spin vs Low-Spin Complexes. That article established qualitatively that weak-field ligands favor maximal unpaired spin. It also showed that strong-field ligands favor pairing. Here that qualitative statement is turned into numbers. We determine how many unpaired electrons exist for each dnd^n configuration in each geometry. We determine what magnetic moment each configuration predicts. We also show how the magnitude of PP relative to Δo\Delta_o is actually computed from Racah parameters. The natural next destination is Crystal Field Stabilization Energy. There, the same splitting diagrams are used to compute the thermodynamic stabilization that crystal fields provide. That is the energetic partner to the magnetic story told here.

Key takeaways
  • Magnetic moment is measured experimentally and compared with the spin-only formula μeff=n(n+2) μB\mu_{\text{eff}} = \sqrt{n(n+2)}\,\mu_B, where nn is the number of unpaired electrons.
  • The number of unpaired electrons in d4d^4–d7d^7 octahedral complexes depends on whether Δo>P\Delta_o > P (low-spin) or Δo<P\Delta_o < P (high-spin); d1d^1–d3d^3 and d8d^8–d10d^{10} have only one possible configuration.
  • Pairing energy PP has two physical origins: a Coulombic repulsion cost Πc\Pi_c for putting two electrons in the same orbital, and a loss of exchange stabilization Πe\Pi_e for reducing the number of parallel-spin pairs.
  • PP is tabulated per metal ion (roughly 15,000–28,000 cm⁻¹ for first-row M2+/M3+M^{2+}/M^{3+}) and is compared directly against Δo\Delta_o, which depends on the ligand via the spectrochemical series.
  • Tetrahedral complexes are almost always high-spin because Δt≈49Δo\Delta_t \approx \tfrac{4}{9}\Delta_o is nearly always smaller than PP.
  • Deviations from the spin-only value (orbital contribution, spin–orbit coupling) are real but usually small for first-row 3d ions with AA or EE ground terms; they grow for second/third-row metals and for ions with unquenched orbital angular momentum (TT ground terms).
  • Key idea: whether electrons pair up or spread out across dd-orbitals is decided by comparing two energies, Δo\Delta_o and PP, and that comparison alone fixes the measurable magnetic moment.

Where this lives today

Magnetic moment measurements remain a routine, cheap, and diagnostic tool in synthetic inorganic and bioinorganic chemistry labs: the Evans NMR method, requiring only a standard NMR spectrometer and no specialized magnetometer, lets a chemist confirm the oxidation state and spin state of a newly synthesized complex in minutes, cross-checking against the same Δo\Delta_o-versus-PP logic developed here. In bioinorganic chemistry, the spin state of iron in heme proteins is a direct functional switch. Deoxyhemoglobin's iron(II) is five-coordinate and high-spin (S=2S=2); on binding O₂, the iron becomes six-coordinate and switches to low-spin (S=0S=0), a spin-state change that physically pulls the iron into the porphyrin plane and triggers the conformational signal underlying cooperative oxygen binding — the same electronic competition between Δo\Delta_o-like ligand field splitting and pairing energy, now doing physiological work. In molecular magnetism and materials science, spin-crossover complexes are engineered so that Δo\Delta_o and PP are deliberately balanced to be nearly equal, so that temperature, pressure, or light can flip the complex between high-spin and low-spin states — the basis of proposed molecular switches, displays, and memory devices, where the same Δo\Delta_o vs PP inequality developed here becomes a tunable, externally-triggerable bistability rather than a fixed property of one compound. In catalysis and organometallic chemistry, predicting whether an intermediate is high-spin or low-spin (and hence how many d-orbitals are available for bonding, and how reactive/labile the complex will be) is a standard first diagnostic step before invoking a mechanism — low-spin d6d^6 octahedral complexes, with fully occupied nonbonding t2gt_{2g} orbitals, are characteristically substitution-inert (as flagged in Worked Example 3 for cobalt(III) ammines), while high-spin configurations with occupied eg∗e_g^* orbitals are typically far more labile — a link this article shares directly with Crystal Field Stabilization Energy, where the thermodynamic (rather than magnetic) consequences of the same splitting diagram are quantified.

Ask the tutor: For a given metal ion, how would you estimate whether a tetrahedral complex could ever become low-spin, and what ligand field strength would that require relative to Δo\Delta_o?

The physical picture

Take a free gaseous transition-metal ion with nn electrons to place among five degenerate dd-orbitals. Hund's rules say: maximize total spin first, then maximize orbital angular momentum. Maximizing spin means spreading electrons across as many of the five orbitals as possible before doubly occupying any of them — this is simply lower in energy because parallel-spin electrons in different orbitals avoid each other more effectively (lower Coulomb repulsion, plus a genuine quantum-mechanical exchange stabilization) than either antiparallel electrons in different orbitals or two electrons forced into the same orbital. Now put that ion in an octahedral field of six ligands. The five-fold degeneracy is broken into a lower t2gt_{2g} set (three orbitals) and an upper ege_g set (two orbitals), separated by Δo\Delta_o. For d1d^1, d2d^2, d3d^3 there is no dilemma: three electrons fit into three different t2gt_{2g} orbitals with parallel spin, satisfying Hund's rule at zero pairing cost, regardless of how large or small Δo\Delta_o is. The same absence-of-choice happens at the top of the shell: d8d^8, d9d^9, d10d^{10} have only one way to distribute electrons once you insist on filling t2gt_{2g} first (three doubly-occupied orbitals are unavoidable by d6d^6 already in t2gt_{2g}, and ege_g is forced to hold the remainder). The interesting cases are d4d^4 through d7d^7. Here the electron count is large enough that Hund's-rule spreading would require promoting an electron across the t2gt_{2g}–ege_g gap, and small enough that pairing within t2gt_{2g} is a real alternative. The system must decide: pay Δo\Delta_o to promote an electron to ege_g and keep it unpaired (high-spin), or pay PP to pair it up within t2gt_2g and avoid the promotion (low-spin). This is a direct energetic comparison, and its outcome is read out experimentally through the number of unpaired electrons via the magnetic moment.

Figure
Octahedral splitting and the four ambiguous configurations, d⁴–d⁷
High-spin (Δₒ < P) vs Low-spin (Δₒ > P), d⁴–d⁷ d⁴ HS, n=4 t₂g ↑↑↑ eg ↑ d⁴ LS, n=2 t₂g ↑↓↑↑ d⁵ HS, n=5 t₂g ↑↑↑ ↑↑ d⁵ LS, n=1 t₂g ↑↓↑↓↑ d⁶ HS, n=4 ↑↓↑↑ ↑↑ d⁶ LS, n=0 ↑↓↑↓↑↓ d⁷ HS, n=3 ↑↓↑↓↑ ↑↑ d⁷ LS, n=1 ↑↓↑↓↑↓ ↑ Filling order: electrons occupy t₂g singly first (Hund), then either promote to eg (HS, cost Δₒ) or pair in t₂g (LS, cost P), depending on Δₒ vs P. Only d⁴–d⁷ show this ambiguity; d¹–d³ and d⁸–d¹⁰ have one configuration regardless of Δₒ/P.

The magnetic consequence of all this bookkeeping is that unpaired electrons act as tiny magnetic dipoles due to their spin (and, in principle, their orbital motion). A sample containing many such dipoles is pulled into a magnetic field gradient — it is paramagnetic — with a strength proportional to how many unpaired electrons each ion carries. Complexes with all electrons paired have no net spin dipole and are weakly repelled from a field (diamagnetic), a much smaller effect arising from induced circulation of paired electrons.

Figure
Spin-only moment vs unpaired-electron count
μ_eff = √[n(n+2)] μB — values for n = 0..5 μ (μB) n (unpaired e⁻) 0 1 2 3 4 5 0.00 1.73 2.83 3.87 4.90 5.92

The core ideas

The spin-only magnetic moment. For a first-row transition-metal ion where orbital angular momentum is largely quenched by the ligand field (true for most AA- and EE-term ground states), the effective magnetic moment is well approximated by counting only spin contributions:

μeff=n(n+2) μB\mu_{\text{eff}} = \sqrt{n(n+2)}\ \mu_B

where: nn = number of unpaired electrons, μB\mu_B = the Bohr magneton (9.274×10−24 J T−19.274\times10^{-24}\ \mathrm{J\,T^{-1}}), and μeff\mu_{\text{eff}} is reported in units of μB\mu_B. This comes from μeff=gsS(S+1) μB\mu_{\text{eff}} = g_s\sqrt{S(S+1)}\,\mu_B with gs≈2g_s \approx 2 (the free-electron gg-factor) and total spin S=n/2S = n/2, so S(S+1)=n2(n2+1)=n(n+2)4S(S+1) = \frac{n}{2}\left(\frac{n}{2}+1\right) = \frac{n(n+2)}{4}, and gsS(S+1)=2n(n+2)/4=n(n+2)g_s\sqrt{S(S+1)} = 2\sqrt{n(n+2)/4} = \sqrt{n(n+2)}.

Reading: this single formula converts a count of unpaired electrons — an integer you can read straight off an orbital-filling diagram — into a number with units of μB\mu_B that is directly comparable to what a Gouy balance or Evans NMR method measures. It says nothing about why electrons paired or didn't; that decision is made separately by comparing Δo\Delta_o and PP.

The high-spin/low-spin criterion. For d4d^4–d7d^7 octahedral complexes, the configuration adopted minimizes total electronic energy, which reduces to a direct comparison:

low-spin if Δo>P,high-spin if Δo<P\text{low-spin if } \Delta_o > P, \qquad \text{high-spin if } \Delta_o < P

where: Δo\Delta_o = octahedral crystal field splitting energy (ligand- and metal-dependent, read from the spectrochemical series and tabulated spectroscopically), and PP = the mean pairing energy required to force a second electron into an already-singly-occupied orbital (an intrinsic, largely ligand-independent property of the free ion, though it is somewhat reduced — the nephelauxetic effect — by covalent delocalization onto ligands).

Reading: this is the master inequality of the whole subject. Everything about whether a complex is paramagnetic with a large moment or nearly diamagnetic follows from which side of this inequality a given dnd^n/ligand/geometry combination falls on.

Decomposing the pairing energy. PP is not a single elementary quantity; it is a sum of two physically distinct penalties incurred when an electron is forced into an orbital that is already singly occupied rather than into a still-empty orbital of the same energy:

P=Πc+ΠeP = \Pi_c + \Pi_e

where: Πc\Pi_c = the Coulombic pairing energy, the extra electrostatic repulsion of confining two electrons to the same spatial orbital rather than to two different ones, and Πe\Pi_e = the exchange pairing energy, the stabilization lost because pairing removes one same-spin electron pair (exchange stabilization exists only between electrons of parallel spin in different orbitals, a purely quantum mechanical, Pauli-exclusion-related effect with no classical analogue).

Reading: Πc\Pi_c is repulsive and always opposes pairing (same-orbital electrons are, on average, closer together than electrons in different orbitals, even accounting for correlation). Πe\Pi_e is a stabilization that is lost upon pairing, because reducing the number of unpaired, parallel-spin electrons reduces the number of stabilizing same-spin exchange pairs. Both effects push PP in the same direction — both make pairing costly — which is exactly why PP is a positive quantity of a few thousand to tens of thousands of cm⁻¹, tabulated per free ion (see Worked Example 3).

Derivation ACounting unpaired electrons for every d^n, both spin states, octahedral field

Goal. Produce the complete table of nn (unpaired electrons) for d1d^1 through d10d^{10} in an octahedral field, in both the high-spin and low-spin limits where both exist, and identify exactly which configurations are ambiguous (depend on Δo\Delta_o vs PP).

Step 1 — set up the orbital scaffold. An octahedral field splits the five dd-orbitals into t2gt_{2g} (three orbitals, lower) and ege_g (two orbitals, higher), separated by Δo\Delta_o. Electrons fill according to the aufbau principle modified by the competition between promotion (cost Δo\Delta_o per electron promoted to ege_g rather than pairing in t2gt_{2g}) and pairing (cost PP per pair forced into one orbital).

Step 2 — fill d1d^1–d3d^3: no ambiguity. With one, two, or three electrons, Hund's rule is satisfiable at zero extra cost: put each electron in a separate t2gt_{2g} orbital with parallel spin. There is no competing lower-energy option because ege_g is strictly higher and t2gt_{2g} has three empty orbitals to offer. So n=1,2,3n = 1, 2, 3 for d1,d2,d3d^1, d^2, d^3 respectively, regardless of Δo\Delta_o or PP.

Step 3 — fill d4d^4: the first real choice. The fourth electron can either go into ege_g (cost Δo\Delta_o, keeping all four electrons unpaired, n=4n=4 — high spin) or pair up with one of the three t2gt_{2g} electrons (cost PP, giving configuration t2g4eg0t_{2g}^4 e_g^0 with one paired and two unpaired, n=2n=2 — low spin). Comparing costs: choose promotion (HS) if Δo<P\Delta_o < P; choose pairing (LS) if Δo>P\Delta_o > P.

Step 4 — fill d5d^5: the same logic, more electrons. High spin (Δo<P\Delta_o < P): t2g3eg2t_{2g}^3 e_g^2, all five orbitals singly occupied, n=5n = 5 — this is the famous "half-filled shell, maximum spin" case, e.g. high-spin Fe³⁺ or Mn²⁺. Low spin (Δo>P\Delta_o > P): t2g5eg0t_{2g}^5 e_g^0, meaning t2gt_{2g} holds five electrons across three orbitals — two orbitals doubly occupied, one singly occupied — giving n=1n=1.

Step 5 — fill d6d^6: same logic again. High spin: t2g4eg2t_{2g}^4 e_g^2 — one t2gt_{2g} orbital pairs (unavoidable, since only five orbitals exist for six electrons even at maximum spreading), giving n=4n=4. Low spin: t2g6eg0t_{2g}^6 e_g^0 — all three t2gt_{2g} orbitals doubly occupied, n=0n=0, fully diamagnetic. This is the Fe(II) case from the opening hook.

Step 6 — fill d7d^7: same logic, last ambiguous case. High spin: t2g5eg2t_{2g}^5 e_g^2, i.e. t2gt_{2g} has one doubly-occupied orbital plus two singly occupied, and ege_g has two singly occupied — n=3n=3. Low spin: t2g6eg1t_{2g}^6 e_g^1, t2gt_{2g} fully paired, one electron alone in ege_g, n=1n=1.

Step 7 — fill d8d^8–d10d^{10}: ambiguity disappears again. For d8d^8, t2g6eg2t_{2g}^6 e_g^2 is the only sensible arrangement (three t2gt_{2g} orbitals must pair regardless, and the remaining two electrons occupy the two ege_g orbitals singly, by Hund's rule, at zero extra pairing cost) — n=2n=2, always, high or low spin makes no difference. d9d^9: t2g6eg3t_{2g}^6 e_g^3 forces one ege_g orbital to pair, n=1n=1, unavoidably. d10d^{10}: everything is paired, n=0n=0, unavoidably. There is no spin-state choice left because there are no longer enough empty orbitals to offer an alternative to pairing.

Result — the complete table:

dnd^nHS configHS nnLS configLS nnAmbiguous?
d1d^1t2g1t_{2g}^11——no
d2d^2t2g2t_{2g}^22——no
d3d^3t2g3t_{2g}^33——no
d4d^4t2g3eg1t_{2g}^3 e_g^14t2g4t_{2g}^42yes
d5d^5t2g3eg2t_{2g}^3 e_g^25t2g5t_{2g}^51yes
d6d^6t2g4eg2t_{2g}^4 e_g^24t2g6t_{2g}^60yes
d7d^7t2g5eg2t_{2g}^5 e_g^23t2g6eg1t_{2g}^6 e_g^11yes
d8d^8t2g6eg2t_{2g}^6 e_g^22——no
d9d^9t2g6eg3t_{2g}^6 e_g^31——no
d10d^{10}t2g6eg4t_{2g}^6 e_g^40——no

Limiting check. As Δo→0\Delta_o \to 0 (a free ion, no field), the distinction between t2gt_{2g}/ege_g disappears and every dnd^n reduces to the atomic Hund's-rule ground state — consistent with d4d^4 HS (n=4n=4, matching free-ion S=2S=2) being the correct limit, not the LS value. As Δo→∞\Delta_o \to \infty (an idealized, impossibly strong field), every ambiguous configuration collapses to its LS value, consistent with the strong-field limit used to build molecular-orbital diagrams for d6d^6 complexes like [Co(NH3)6]3+\text{[Co(NH}_3)_6\text{]}^{3+}.

Go deeper · Derivation B · 3 minDecomposing pairing energy P into Coulombic and exchange contributions
Derivation BDecomposing pairing energy P into Coulombic and exchange contributions

Goal. Show explicitly why P=Πc+ΠeP = \Pi_c + \Pi_e, using the microstate/Racah-parameter description of dd-electron repulsion, and connect this to why PP is tabulated as a positive, ion-specific quantity independent of the ligand field.

Step 1 — electron repulsion in a multi-electron ion is not a single number. In a free ion, the electrostatic repulsion between any pair of dd-electrons depends on which specific orbitals they occupy and on their relative spin, not just on "two electrons repel each other." This is captured by the Racah parameters BB and CC, which parametrize the electron-electron repulsion integrals within the dd-shell after removing the average (spherical) part already absorbed into orbital energies.

Step 2 — the Coulombic part, Πc\Pi_c. Two electrons confined to the same dd-orbital (necessarily opposite spin, by Pauli exclusion) experience larger direct Coulomb repulsion than two electrons in different orbitals, because same-orbital electrons share more spatial overlap on average. This purely classical-repulsion penalty is Πc\Pi_c: it must be paid every time pairing forces two electrons into one orbital instead of two.

Step 3 — the exchange part, Πe\Pi_e. Independently of repulsion, quantum mechanics (via the Pauli principle) stabilizes configurations with more parallel-spin electron pairs occupying different orbitals: the antisymmetry requirement keeps same-spin electrons further apart on average ("Fermi hole"), lowering their mutual repulsion relative to a naive classical estimate, and this lowering is called exchange stabilization. Every distinct pair of parallel-spin electrons in different orbitals contributes one unit of this stabilization. When a promoted electron is instead paired up, the number of such parallel-spin pairs decreases, and that lost stabilization is Πe\Pi_e — an energy penalty from the point of view of the pairing process, even though its origin is a stabilization that pairing forfeits.

Step 4 — counting pairs explicitly for a small case. Consider promoting the fifth electron in d5d^5: high spin has five parallel-spin electrons in five different orbitals, giving (52)=10\binom{5}{2} = 10 same-spin pairs, each contributing exchange stabilization KK (an exchange integral, itself expressible via Racah parameters). Low spin (t2g5t_{2g}^5) has only three unpaired-compatible orbitals occupied by five electrons: two orbitals hold spin-paired electrons and one orbital holds a single electron, leaving only (32)=3\binom{3}{2}=3 same-spin pairs among the three "spin-up" representative electrons (a simplified counting that captures the qualitative trend: many fewer same-spin pairs survive). The difference in exchange-pair count, multiplied by KK, is the exchange contribution to PP; the extra direct repulsion of forcing two full orbitals is the Coulombic contribution.

Step 5 — assembling PP as a tabulated, ligand-independent quantity. Because Πc\Pi_c and Πe\Pi_e are both expressed through Racah parameters BB and CC — properties of the free gaseous ion's electron-repulsion structure, essentially independent of what ligands are attached — PP itself is tabulated per free ion (e.g., P(Fe2+)≈17,600 cm−1P(\text{Fe}^{2+}) \approx 17{,}600\ \mathrm{cm^{-1}}, P(Co3+)≈21,000 cm−1P(\text{Co}^{3+}) \approx 21{,}000\ \mathrm{cm^{-1}}, both from spectroscopic Racah-parameter fits) and treated as a fixed number when compared against the ligand-dependent Δo\Delta_o. In real complexes PP is somewhat reduced from its bare free-ion value by covalent delocalization of dd-electron density onto ligands (the nephelauxetic effect, "cloud-expanding"), because delocalized electrons repel each other less — but this correction is secondary to the basic Coulomb-plus-exchange decomposition.

Limiting check. If exchange stabilization were switched off entirely (Πe→0\Pi_e \to 0, an unphysical but useful limit), PP would reduce to pure Coulombic repulsion Πc\Pi_c, and Hund's-rule spin-maximization would lose its energetic basis — configurations would then be decided by orbital energy alone, contradicting the well-established atomic spectroscopy (e.g., the ground term of free Fe²⁺ is 5D^5D, a maximum-multiplicity term, which requires Πe>0\Pi_e > 0 to be favored). This confirms exchange stabilization is a real, necessary, non-zero contributor, not a bookkeeping fiction.

Worked examples

Example 1 (foundational): [Fe(H2O)6]2+\text{[Fe(H}_2\text{O)}_6\text{]}^{2+}, a high-spin d6d^6 ion. Fe²⁺ is d6d^6. Water is a weak-field ligand (spectrochemical series places H2O\mathrm{H_2O} well below CN−\mathrm{CN^-} or NH3\mathrm{NH_3}), giving a modest Δo≈10,400 cm−1\Delta_o \approx 10{,}400\ \mathrm{cm^{-1}} for this complex (from dd–dd absorption spectroscopy). The pairing energy for free Fe²⁺ is P≈17,600 cm−1P \approx 17{,}600\ \mathrm{cm^{-1}}.

Δo(10,400 cm−1)<P(17,600 cm−1)  ⟹  high spin\Delta_o (10{,}400\ \mathrm{cm^{-1}}) < P (17{,}600\ \mathrm{cm^{-1}}) \implies \text{high spin}

From Step 5 of the first derivation, HS d6d^6 is t2g4eg2t_{2g}^4 e_g^2 with n=4n=4 unpaired electrons. Applying the spin-only formula:

μeff=4(4+2) μB=24 μB=4.90 μB\mu_{\text{eff}} = \sqrt{4(4+2)}\ \mu_B = \sqrt{24}\ \mu_B = 4.90\ \mu_B

This matches the experimental range for high-spin octahedral Fe(II) complexes, typically 5.15.1–5.7 μB5.7\ \mu_B (the small excess above the spin-only value comes from a residual orbital contribution in the TT ground term of octahedral d6d^6, discussed under Limiting Cases). The qualitative conclusion — paramagnetic, four unpaired electrons — is exactly right; the magnitude match to within about 15% confirms the spin-only approach is a good zeroth approximation even where orbital contributions are not fully quenched.

Example 2 (applied): [Fe(CN)6]4−\text{[Fe(CN)}_6\text{]}^{4-} versus [FeF6]4−\text{[FeF}_6\text{]}^{4-}, same ion, opposite outcome. Both are Fe²⁺, d6d^6, octahedral, with P≈17,600 cm−1P \approx 17{,}600\ \mathrm{cm^{-1}} fixed. The ligand field splitting differs enormously: cyanide is a strong-field, π\pi-accepting ligand giving Δo(CN−)≈33,000 cm−1\Delta_o(\text{CN}^-) \approx 33{,}000\ \mathrm{cm^{-1}} for this complex, while fluoride is weak-field, giving Δo(F−)≈13,000 cm−1\Delta_o(\text{F}^-) \approx 13{,}000\ \mathrm{cm^{-1}}. For [Fe(CN)6]4−\text{[Fe(CN)}_6\text{]}^{4-}:

Δo(33,000 cm−1)>P(17,600 cm−1)  ⟹  low spin,n=0\Delta_o (33{,}000\ \mathrm{cm^{-1}}) > P (17{,}600\ \mathrm{cm^{-1}}) \implies \text{low spin}, \quad n = 0
μeff=0(0+2) μB=0 μB(diamagnetic)\mu_{\text{eff}} = \sqrt{0(0+2)}\ \mu_B = 0\ \mu_B \quad (\text{diamagnetic})

For [FeF6]4−\text{[FeF}_6\text{]}^{4-}:

Δo(13,000 cm−1)<P(17,600 cm−1)  ⟹  high spin,n=4\Delta_o (13{,}000\ \mathrm{cm^{-1}}) < P (17{,}600\ \mathrm{cm^{-1}}) \implies \text{high spin}, \quad n = 4
μeff=4(4+2) μB=4.90 μB(paramagnetic)\mu_{\text{eff}} = \sqrt{4(4+2)}\ \mu_B = 4.90\ \mu_B \quad (\text{paramagnetic})

Experimentally, ferrocyanide salts are indeed diamagnetic and [FeF6]4−\text{[FeF}_6\text{]}^{4-}-type high-spin Fe(II) fluorides show moments near 5.0–5.4 μB\mu_B. This pair is the cleanest textbook demonstration that Δo\Delta_o, not PP, is the variable doing the work when comparing complexes of the same metal ion in different ligand environments — PP stays essentially fixed at ~17,600 cm⁻¹ throughout, while Δo\Delta_o swings by a factor of 2.5.

Example 3 (exam/competition level): predicting the moment of [Co(NH3)5Cl]2+\text{[Co(NH}_3)_5\text{Cl]}^{2+}, an asymmetric ligand set, and cross-checking against the pairing-energy decomposition. Cobalt here is Co²⁺ (since the complex overall is 2+2+ and five neutral NH₃ plus one Cl−\mathrm{Cl^-} contribute −1-1, so metal oxidation state =+2−(−1)=+2= +2 - (-1) = +2... more carefully: total charge 2+2+ = (metal oxidation state) + 5(0) + (−1), so metal oxidation state =+3= +3). Co³⁺ is d6d^6. Take Δo\Delta_o for this mixed-ligand complex as approximately Δo≈23,000 cm−1\Delta_o \approx 23{,}000\ \mathrm{cm^{-1}} (intermediate between pure [Co(NH3)6]3+\text{[Co(NH}_3)_6\text{]}^{3+}, Δo≈22,900 cm−1\Delta_o \approx 22{,}900\ \mathrm{cm^{-1}}, and the weaker chloride perturbation on one site, which lowers the average ligand field only slightly since five of six sites remain strong-field ammine). The pairing energy for free Co³⁺ is P≈21,000 cm−1P \approx 21{,}000\ \mathrm{cm^{-1}} (Co³⁺ pairing energies run higher than Fe²⁺ because of the higher ionic charge, which contracts the dd-orbitals and increases electron-electron repulsion, hence increases both Πc\Pi_c and Πe\Pi_e).

Δo(23,000 cm−1)>P(21,000 cm−1)  ⟹  low spin,n=0\Delta_o (23{,}000\ \mathrm{cm^{-1}}) > P (21{,}000\ \mathrm{cm^{-1}}) \implies \text{low spin}, \quad n = 0
μeff=0(0+2) μB=0 μB\mu_{\text{eff}} = \sqrt{0(0+2)}\ \mu_B = 0\ \mu_B

Experimentally, cobalt(III) ammine complexes — with very few exceptions involving weak-field halide-rich coordination spheres — are diamagnetic low-spin d6d^6, consistent with μeff≈0\mu_{\text{eff}} \approx 0 measured for [Co(NH3)5Cl]2+\text{[Co(NH}_3)_5\text{Cl]}^{2+} and related pentaamminecobalt(III) salts. As a limiting-case sanity check: if the single ammine ligand were replaced progressively by more chlorides, Δo\Delta_o would fall (Cl⁻ is a weaker-field ligand than NH₃), and once enough substitution pushed Δo\Delta_o below P≈21,000 cm−1P \approx 21{,}000\ \mathrm{cm^{-1}}, the complex would cross over to high spin — consistent with the empirical observation that highly halide-substituted Co(III) complexes are far rarer and less kinetically inert than the ammine-rich ones, partly because the low-spin d6d^6 configuration itself, with all electrons in nonbonding t2gt_{2g}, is what confers Co(III) ammines their famous substitution inertness in the first place.

Limiting cases, scope & common traps

SituationWhat happensWhy
d1d^1–d3d^3, d8d^8–d10d^{10}, octahedralnn fixed, no HS/LS choiceNot enough (or too many) electrons to create a pairing-vs-promotion dilemma
d4d^4–d7d^7, octahedralnn depends on Δo\Delta_o vs PPGenuine competition between two energies of comparable magnitude
Tetrahedral complexesAlmost always high spinΔt≈49Δo\Delta_t \approx \tfrac{4}{9}\Delta_o is rarely large enough to exceed PP
Second/third-row transition metals (4d, 5d)Low spin strongly favored, even for weak-field ligandsΔo\Delta_o increases sharply down a group (better orbital overlap) while PP decreases (larger, more diffuse dd-orbitals reduce repulsion)
AA/EE ground-term ions (e.g. HS d5d^5, LS d6d^6)Spin-only formula very accurateOrbital angular momentum fully quenched by the ligand field symmetry
TT ground-term ions (e.g. HS d6d^6, d7d^7; LS d4d^4)Measured μ\mu modestly exceeds spin-only valueResidual orbital angular momentum contributes via spin–orbit coupling
Strongly covalent / heavy-ligand complexesPeffectiveP_{\text{effective}} reduced below free-ion tabulated valueNephelauxetic effect: delocalization onto ligands lowers electron-electron repulsion

The chemist behind it

Origins · 1 minLeopold Alexander Pauling? — no: Linus Pauling and how this was discovered
LA
Leopold Alexander Pauling? — no: Linus Pauling
1901–1994 · early valence-bond magnetochemistry of coordination complexes

The correct attribution for the specific spin-only formula and the systematic use of magnetic moments to determine electronic structure in coordination compounds belongs jointly to Linus Pauling, who in the 1930s connected valence-bond theory to observed magnetic moments of transition-metal complexes, and to Hans Bethe and John Van Vleck, whose crystal-field and ligand-field theoretical framework (Bethe's 1929 group-theoretical treatment of ions in crystal fields, and Van Vleck's development of magnetochemical theory through the 1930s–1960s) supplied the quantitative machinery — Δo\Delta_o, PP, Racah parameters — used throughout this article. Van Vleck in particular deserves the central credit for magnetochemistry as a predictive, quantitative science. Working largely at Harvard and later at the University of Minnesota and back at Harvard, Van Vleck developed the theory connecting molecular and ionic electronic structure to bulk magnetic susceptibility — what became known as the Van Vleck equation, the general statistical-mechanical formula from which the spin-only limit used throughout ordinary coordination chemistry is recovered as a special case for ions with negligible spin-orbit coupling and no low-lying excited states. He shared the 1977 Nobel Prize in Physics (with Philip Anderson and Nevill Mott) for fundamental theoretical work on the electronic structure of magnetic and disordered systems — work whose everyday chemical payoff is exactly the ability to read Δo\Delta_o vs PP off a measured magnetic moment, as this article has done throughout.

Origins · 1 minhow this was discovered
History
- 1929 — Hans Bethe publishes the group-theoretical treatment of ions in crystalline electric fields, founding crystal field theory.
- 1932 — Linus Pauling applies valence-bond ideas to rationalize magnetic moments of coordination complexes, distinguishing "ionic" (high-spin) from "covalent" (low-spin) bonding descriptions.
- 1932–1940s — John Van Vleck develops the general quantum-statistical theory of magnetic susceptibility (the Van Vleck equation), unifying crystal field theory with observable magnetism.
- 1950s — Racah parameters (BB, CC) become standard tools, via optical spectroscopy, for extracting quantitative pairing energies and interelectronic repulsion terms for real complexes.
- 1977 — John Van Vleck shares the Nobel Prize in Physics for theoretical work underlying the electronic and magnetic structure of transition-metal ions in solids and complexes.
Why is pairing energy treated as a property of the metal ion rather than the whole complex?

Pairing energy arises from electron-electron repulsion and exchange interactions purely within the metal's dd-orbitals, quantified through Racah parameters BB and CC that are extracted from the free ion's or complex's optical spectrum. These repulsion integrals depend on how contracted and how many electrons occupy the dd-shell — properties of the metal and its oxidation state — much more than on which ligands are attached. Ligands do modestly reduce PP from its bare free-ion value through covalent delocalization of dd-density onto ligand orbitals (the nephelauxetic effect), but this is a secondary correction. To first order, chemists tabulate one PP value per metal ion and treat it as fixed when scanning across different ligands, exactly as done when comparing [FeF6]4−\text{[FeF}_6\text{]}^{4-} and [Fe(CN)6]4−\text{[Fe(CN)}_6\text{]}^{4-}.

Does the spin-only formula ever fail badly, not just by a small correction?

Yes, particularly for second- and third-row transition metals (4d, 5d series) and for lanthanides, where spin–orbit coupling is large enough that orbital angular momentum is not a small perturbation but a dominant contributor to the total magnetic moment. For most first-row (3d) octahedral complexes with orbitally non-degenerate (AA or EE) ground terms, the spin-only formula is accurate to within a few percent. For first-row ions with orbitally degenerate (TT) ground terms, deviations of a few tenths of a μB\mu_B are typical but the qualitative story (paramagnetic vs diamagnetic, roughly how many unpaired electrons) survives. For heavier metals the formula should be used only as a rough starting estimate, with full Russell-Saunders coupling or even relativistic treatments needed for real quantitative work.

How is Δₒ actually measured, given that P is needed to predict spin state before you even know Δₒ?

Δo\Delta_o is measured independently of the high-spin/low-spin question, primarily from the position of dd–dd absorption bands in the UV-visible spectrum of the complex — the lowest-energy spin-allowed dd–dd transition directly reports Δo\Delta_o (with some caveats for multi-electron configurations where more than one Racah-parameter-dependent term is involved). This spectroscopic measurement does not require prior knowledge of the spin state; rather, once Δo\Delta_o is measured this way, it is compared against the independently tabulated free-ion PP to predict (and cross-check against separately measured magnetic moments) which spin state the complex actually adopts.

Why do second- and third-row transition metals almost never show high-spin configurations?

Two effects compound in the same direction going down a group. First, 4d4d and 5d5d orbitals are more radially extended and overlap more effectively with ligand orbitals than 3d3d orbitals, producing substantially larger Δo\Delta_o values for chemically similar ligands — often 50% or more larger than the 3d analogue. Second, the same radial expansion of 4d4d/5d5d orbitals reduces electron-electron repulsion within the metal dd-shell, lowering PP. Both effects independently push the Δo>P\Delta_o > P inequality toward low spin, which is why essentially all well-characterized octahedral 4d and 5d complexes, even with comparatively weak-field ligands, are low-spin.

Can a single complex switch between high-spin and low-spin under normal laboratory conditions?

Yes — these are called spin-crossover complexes, and they are deliberately designed so that Δo\Delta_o and PP are very close in magnitude, making the balance sensitive to small perturbations. Changing temperature shifts the populated spin state because the high-spin state, despite costing electronic energy, often gains enough vibrational entropy (weaker, longer average metal-ligand bonds allow more low-frequency vibrational modes) to become thermodynamically favored at higher temperature even when the low-spin state is the electronic ground state at 0 K. Pressure, and in some cases light irradiation (the LIESST effect, Light-Induced Excited Spin-State Trapping), can also drive the crossover, which is why such complexes are studied intensively for molecular switches and memory materials.

Is diamagnetism ever observed for a reason other than a low-spin d⁶ (or similarly fully-paired) configuration?

Yes — diamagnetism is the default expectation whenever every electron in a molecule is spin-paired, which includes the vast majority of main-group closed-shell molecules and any d0d^0 or d10d^{10} transition-metal complex, regardless of spin-state considerations (there is no high-spin/low-spin ambiguity for those counts, as shown in the unpaired-electron table). Low-spin d6d^6, d4d^4, and d8d^8 (in square-planar geometry, where the dx2−y2d_{x^2-y^2} orbital is pushed high enough that d8d^8 becomes diamagnetic even though it is paramagnetic in octahedral or tetrahedral fields) are the classic ligand-field-driven routes to diamagnetism specifically discussed in this article, but plenty of diamagnetic complexes simply have no unpaired-electron question to answer in the first place.