Born Repulsion and the Total Lattice Potential
Squeeze two Na⁺ and Cl⁻ ions together. At first, energy drops steeply as opposite charges approach. This is pure Coulomb attraction, rewarding closeness without limit. Yet real NaCl has a fixed interionic distance of 2.82 Å, not zero. The crystal does not collapse into a point. Something must switch on at short range. It must rise even more steeply than the Coulomb term falls. That something stops the collapse. That something is Born repulsion. It is the energy cost of forcing two closed-shell electron clouds to overlap. This is a direct consequence of the Pauli exclusion principle. This matters because the entire quantitative edifice of ionic bonding rests on one thing. Lattice energies, Born-Haber cycles, compressibility, even the choice of crystal structure — all depend on it. They require some short-range repulsive term to balance the long-range Coulombic Attraction and the Ion-Pair Potential. Without repulsion, the lattice energy expression has no minimum. It is a monotonically decreasing function of the ion separation. No equilibrium bond length could ever be predicted. Born repulsion converts an unbounded attractive potential into a proper energy well. That well has a minimum at a finite, measurable, physically sensible distance. The big picture is a competition of exponents. Coulomb attraction falls off gently, as . So it "reaches" over long distances. It dominates the energetics of the crystal at ordinary bond lengths. Electron-cloud repulsion, by contrast, is a steep, short-ranged effect. It was historically modeled as , with between 5 and 12. Later it was refined to an exponential . This better reflects the physics of overlapping wavefunctions decaying exponentially into space. The interplay of these two terms fixes two things. One term is gentle and long-ranged; the other is violent and short-ranged. Together they fix the equilibrium separation . They also fix the depth of the energy well at that separation — the lattice energy itself. This article builds the total pair potential from scratch. It combines the Coulomb term plus the repulsive term. It differentiates this sum to find the equilibrium separation. It then shows how the curvature of the well at the minimum matters. This curvature is what lets you extract the repulsion parameters from experimental data. Such data includes compressibility, or the Born exponent from ionic electron configurations. It sets up directly for the The Born-Lande Equation and The Born-Mayer Equation. Both of these are just this same total-potential machinery. They simply scale it up from an ion pair to a full lattice sum.
- Coulomb attraction alone has no energy minimum — it decreases monotonically as ions approach, so a repulsive term is mandatory for a stable bond length.
- Born repulsion arises from Pauli-exclusion-driven overlap of filled electron shells: cost rises very steeply as ion separation shrinks below the sum of ionic radii.
- Two standard functional forms are used: the power law (Born model, from compressibility or ionic structure) and the exponential (Born–Mayer model, physically better since real electron density decays exponentially).
- Setting at links the repulsion coefficient (or ) to the attractive Madelung/Coulomb term, eliminating the unknown constant from the final lattice-energy formula.
- The curvature at the minimum is measurable via bulk compressibility, giving an independent experimental route to the Born exponent .
- Key idea: stable ionic bond lengths exist only because a steep, short-range repulsive energy (from Pauli exclusion between overlapping electron clouds) exactly balances the long-range Coulomb attraction at one particular separation.
The equilibrium ionic bond length is the distance at which the outward push of overlapping electron clouds (Born repulsion, steep and short-ranged) exactly cancels the inward pull of Coulomb attraction (gentle and long-ranged); this balance point is a genuine energy minimum only because repulsion falls off faster with distance than attraction does.
Where this lives today
Born repulsion is not a historical curiosity — it is load-bearing machinery in modern computational chemistry and materials science. Every classical molecular dynamics or lattice-energy-minimization force field used to model ionic solids, ceramics, minerals, or battery electrolyte materials includes a short-range repulsive term of exactly this Born or Born–Mayer form (often combined with a van der Waals attractive dispersion term into what is called a Buckingham potential, , widely used in mineralogy and solid-state ionics simulations). Predicting whether a candidate solid-state battery electrolyte (e.g. Li-ion conducting garnets or NASICON-type materials) will have the right lattice parameters and ionic mobility relies on getting these repulsive parameters right, since they set the size of the "bottleneck" channels through which ions must hop. In geochemistry and mineral physics, Born-type repulsive potentials underlie predictions of how silicate and oxide minerals respond to the immense pressures inside planetary interiors — the same curvature-at-the-minimum argument developed here (Step 2 of the second derivation) is the conceptual ancestor of the equations of state used to model Earth's mantle and cores of other rocky planets. In pharmaceutical crystal engineering, repulsive-term parametrization feeds into polymorph prediction software that determines which crystal packing of a drug molecule is thermodynamically favored — a problem of enormous practical importance since different polymorphs can have different solubility and bioavailability. Finally, in the classroom and in the Born-Haber cycle analyses used throughout inorganic chemistry to rationalize thermochemical stability, reactivity trends, and the existence (or non-existence) of compounds like "MgCl" or "NaCl₂," the Born repulsion term is the quiet, unglamorous partner to the Madelung sum that makes the whole quantitative lattice-energy framework work at all.
Ask the tutor: How does adding the Madelung constant turn this single ion-pair potential into the full lattice energy used in Born–Haber cycles?
The physical picture
Picture a single Na⁺–Cl⁻ ion pair as the two ions are pushed together from a large separation. At large , each ion looks to the other like a point charge; the energy is the familiar Coulomb term,
which is negative (attractive, since and have opposite sign) and becomes more negative — i.e., the system gets more stable — as decreases, all the way to . If this were the only term in the potential, the ions would collapse into each other; there is no finite equilibrium distance predicted by Coulomb attraction alone. Physically, that collapse cannot happen because each ion is not a point charge — it is a nucleus surrounded by a full complement of core electrons (Cl⁻ is -like, Na⁺ is -like, both closed-shell configurations with electron density spread over a finite ionic radius). As the ions approach, their electron clouds begin to overlap once becomes comparable to the sum of ionic radii . Overlapping closed shells cannot simply superpose their electrons into the same states: the Pauli exclusion principle forces some electrons into higher-energy orbitals (formally, into antibonding combinations of the atomic orbitals, or equivalently the electron density must be "pushed out" of the overlap region and raised in kinetic energy by the uncertainty principle). This costs energy, and the cost rises extremely steeply as the clouds are forced to interpenetrate further — far more steeply than the Coulomb term falls. The net potential is the sum of a gentle, long-range attractive term and a violent, short-range repulsive term. At large the attractive term dominates (repulsion is exponentially or power-law suppressed at large distances, decaying to zero faster than ), so pulling the ions together lowers the energy. At small the repulsive term dominates and blows up, so pushing the ions together further costs enormous energy. Somewhere in between, the two effects exactly balance: this is the equilibrium separation , and it is a true minimum (not just a balance point) precisely because repulsion is more steeply varying than attraction — the second derivative of the total potential is positive there.
The steepness contrast is the entire story. In the historical Born model the repulsive energy is written as a power law with typically between 5 and 12 (larger for more compressible, more polarizable ions with more diffuse outer shells; smaller — meaning steeper in relative terms at the relevant — for "harder," less compressible ions like small, highly-charged cations). Because , this term is essentially negligible until drops within roughly the sum of ionic radii, at which point it rises almost vertically. Later refinement, due to Born and Mayer, replaced the power law with an exponential form , which is physically preferable because atomic and ionic electron density genuinely falls off exponentially with distance from the nucleus (a feature of the radial solutions of the Schrödinger equation for many-electron atoms), so the overlap of two such clouds — and hence the repulsive energy it generates — also decays exponentially.
The core ideas
The total potential energy of an ion pair separated by distance is the sum of the attractive Coulomb term and a short-range repulsive term:
where:
- are the ionic charges (with negative, so the product is negative and the first term is attractive),
- is the elementary charge, the vacuum permittivity,
- is the center-to-center ion separation,
- is a positive, steeply decreasing function of representing electron-cloud overlap repulsion.
Reading: the first term alone has no stationary point in ; it is monotonic. Stability requires , and the shape of (how fast it falls with ) sets both the equilibrium distance and the curvature of the well there. Two standard choices for are used throughout ionic-bonding theory:
where:
- is an empirical repulsion coefficient (units chosen so comes out in energy),
- is the Born exponent, typically 5–12, obtained from ionic electronic configuration or from compressibility data (larger for ions with more electron shells, i.e. more "incompressible" cores such as noble-gas-like heavy ions).
where:
- is an empirical pre-exponential repulsion constant,
- (units of length, typically ≈ 0.3 Å) is a "softness" parameter describing how rapidly the repulsion decays — smaller means a harder, steeper repulsive wall.
Reading: both functions share the essential qualitative behavior — positive, rapidly vanishing at large , diverging as — but the exponential form is the physically motivated one, since it mirrors the actual exponential decay of atomic orbital wavefunctions at large distance from the nucleus, -type behavior, whose overlap integral between two centers separated by also decays exponentially. The full pair potential (Born model) is therefore
and this is the expression whose minimum defines the observed equilibrium bond length and whose depth (once summed over the whole lattice with the Madelung constant) becomes the lattice energy — the subject of the The Born-Lande Equation.
Goal. Starting from the total pair potential with a Born (power-law) repulsive term, find the equilibrium separation and express the repulsion constant in terms of and , so that never needs to be measured independently.
Step 1 — write the total potential.
Here is written explicitly as a positive number multiplying an overall minus sign, since itself is negative for an oppositely charged pair; this keeps every subsequent sign transparent.
Step 2 — differentiate with respect to r. Equilibrium occurs where the net force is zero, i.e. where the slope of vanishes:
The first term is because differentiating gives (the attractive term produces an inward-pulling force that grows as ions approach — consistent with attraction). The second term is because decreases with increasing , so its derivative is negative; equivalently, the repulsive term produces an outward-pushing force.
Step 3 — set the derivative to zero at r = r₀.
This states that at equilibrium, the attractive force per unit "handle" exactly equals the repulsive force — the ions sit where inward and outward forces cancel.
Step 4 — solve for B in terms of r₀. Multiply both sides by and divide by :
This is the crucial result: the empirical, hard-to-measure repulsion coefficient is now written entirely in terms of the experimentally known equilibrium separation (from X-ray diffraction) and the Born exponent (from tabulated values based on electronic configuration). No independent measurement of is ever required.
Step 5 — substitute back to get U(r₀), the well depth.
Factor the common term:
This is exactly the Born correction factor that appears (scaled up by the Madelung constant) in the The Born-Lande Equation for full lattice energies. Note the check: as (an infinitely hard, infinitely steep repulsive wall — repulsion switches on like a hard sphere exactly at and is zero for all ), the correction factor , and reduces to the pure Coulomb energy at . This is the correct limiting case: an infinitely hard repulsive wall contributes no energy at the equilibrium point itself (it only prevents approach closer than ), so all the binding energy at equilibrium is Coulombic, exactly as physical intuition demands.
Go deeper · Derivation B · 1 minCurvature at the minimum and the compressibility route to n
Goal. Show how the curvature of at — an experimentally accessible quantity via the bulk modulus / compressibility of the crystal — determines the Born exponent independently of any spectroscopic argument about electron configuration.
Step 1 — second derivative of the total potential. Differentiate once more:
The first term is negative (curvature contribution from the attractive Coulomb term, which by itself would make concave, consistent with having no minimum). The second term is positive and, near , large because is a big prefactor — this is what turns the total curvature positive and creates a true minimum rather than an inflection.
Step 2 — evaluate at r = r₀ using the Step 4 result for B. Substitute from the first derivation into the repulsive curvature term:
so the total curvature at the minimum collapses to
Step 3 — interpret physically. This curvature is (up to lattice geometry factors) proportional to the crystal's bulk modulus — a stiffer, less compressible crystal has larger curvature at its potential minimum, meaning a larger . Because curvature is measurable directly from the pressure-dependence of crystal volume (compressibility experiments), this equation can be inverted:
giving an experimental value of that can be cross-checked against the value estimated from the ions' electronic configurations (the two independent routes to agreeing is one of the classic validations of the Born model).
Step 4 — limiting case check. As , the curvature : the well becomes almost flat at the bottom, meaning a very soft, compressible crystal — physically sensible, since would make the repulsive term have the same dependence as the Coulomb term itself, degenerate with attraction and unable to produce any localized minimum at all. This confirms must exceed 1 for a genuine bound minimum to exist, consistent with the tabulated range – used for real ions, all comfortably clear of this degenerate limit.
Worked examples
Example 1 — Foundational: locate the minimum for a model ion pair with round-number . Take a hypothetical 1:1 ion pair with , equilibrium separation Å (chosen off the real NaCl value of 2.82 Å to keep the arithmetic transparent and non-suggestive of a "special" real salt), and Born exponent (a mid-range value typical of ions with argon-like cores). Using Step 4 of the first derivation,
Compute . First (since , , , ), and , so . Numerator: ; multiplied by gives . Denominator: .
Check the well depth via the Step 5 result:
The bare Coulomb term at : numerator , denominator , giving J. Multiplying by :
Converting to a molar quantity (×Avogadro's number) gives kJ/mol for this single ion-pair interaction — smaller in magnitude than a real Madelung-summed lattice energy (which includes attraction/repulsion from all neighboring ions, not just the nearest pair), exactly as expected, since this toy calculation deliberately omits the lattice sum that the The Born-Lande Equation adds on top.
Example 2 — Applied: comparing vs for the same , and why softer ions bind slightly less tightly at fixed bond length. Suppose two different hypothetical salts happen to share exactly the same equilibrium separation Å and the same , but one has Born exponent (softer, more polarizable ions, e.g. involving larger anions like I⁻) and the other (harder, more incompressible ions, e.g. small F⁻ paired with a small, high-charge-density cation). The bare Coulomb energy at Å is the same for both (it doesn't depend on ):
(dividing the earlier denominator-scaling: , so J.) For : correction factor , giving
For : correction factor , giving
The harder-ion salt () binds about 8% more strongly at the same bond length than the softer one (), because a steeper (larger-) repulsive wall "gives back" less of the Coulomb attraction — repulsion only switches on right at the wall, leaving more of the pure Coulomb well depth intact. This is exactly why, in real Born-Landé calculations, ions built from more electrons (bigger, softer, more diffuse clouds — smaller effective is not generally true; conventionally larger ions get larger , and the sign of this trend is worth checking against tables rather than memorized as "always"). The essential physical lesson survives regardless: the correction factor is always a fraction less than 1, always shaves some magnitude off the bare Coulomb energy, and the amount shaved depends on how steep the repulsive wall is.
Example 3 — Exam/competition level: extracting the Born exponent from a measured compressibility-derived curvature. A hypothetical rock-salt-structure crystal MX (1:1 charges, ) has measured equilibrium nearest-neighbor separation Å. An independent compressibility experiment yields a second-derivative (curvature) of the pair potential at of
Find the Born exponent implied by this measurement, and compare with the Coulomb curvature term alone. Using the inverted relation from the second derivation,
First compute . , so . Numerator of the fraction: (using ). Multiply stepwise: . Then . Divide by :
This is puzzlingly small — the numbers imply , essentially , which would be unphysical (no true minimum). This flags an important dimensional/scale check worth doing explicitly: real ionic-crystal curvature values, when properly extracted from bulk moduli (which involve the full lattice sum, the Madelung constant, and the number of nearest neighbors, not a bare single-pair potential), are enormously larger in magnitude than a bare single-pair estimate — typically of order – N/m in force-constant terms once lattice geometry is folded in. The arithmetic pipeline above is correct as a method; the lesson of this worked example is that must be the correctly scaled single-pair curvature (stripped of lattice geometry factors such as the coordination number and Madelung constant) before this formula can be applied — exactly the bookkeeping problem that the The Born-Lande Equation and its lattice sums are built to handle properly. A student who plugs in a macroscopic compressibility number without first converting it to a single-pair curvature will get exactly this kind of nonsensical near-unity , which is itself a useful diagnostic that a unit or lattice-factor conversion has been skipped.
Limiting cases, scope & common traps
| Regime | Behavior | Interpretation |
|---|---|---|
| (Coulomb dominates, repulsion exponentially/power-law) | Free, non-interacting ions; correct asymptotic limit | |
| Repulsion diverges faster than Coulomb attraction diverges to ; physically forbids total collapse | ||
| Correction factor | Infinitely hard-sphere repulsion; well depth equals bare Coulomb energy at | |
| Curvature at minimum | Degenerate case; repulsion has the same form as attraction, no true localized minimum | |
| Exponential (Born–Mayer) vs power-law (Born) form | Both reproduce a minimum; exponential is physically better motivated | Exponential decay matches real atomic orbital tails; power law is a convenient empirical fit |
| Only nearest-neighbor pair considered here | Real lattice energy needs sum over all ion pairs (Madelung constant) | This article is the pairwise building block; full lattice energy is the next stage |
The chemist behind it
Max Born (1882–1970) was a German theoretical physicist whose name is more famous today for the Born interpretation of the quantum wavefunction (probability density ) than for ionic crystals, but his early career, in Göttingen before quantum mechanics existed in its later form, was deeply concerned with the mechanics of crystal lattices. Working alongside Alfred Landé around 1918, Born sought a classical-mechanical (pre-quantum-mechanical, in the modern sense) model that could reproduce measured lattice energies and, crucially, the compressibility of ionic crystals — a property utterly unexplained by Coulomb attraction alone. Introducing a short-range repulsive term of the form , calibrated against measured compressibilities, gave the first quantitatively successful model of an ionic crystal's cohesive energy, decades before the full quantum-mechanical justification (Pauli exclusion, exchange interactions) was available. Joseph E. Mayer, working with Born considerably later (the Born–Mayer refinement dates to the early 1930s, after the Pauli principle and modern quantum mechanics were established), replaced the power-law repulsion with the physically motivated exponential form, better matching the true exponential decay of atomic electron density predicted by quantum theory.
Origins · 1 minMax Born and how this was discovered
Why isn't the equilibrium bond length just the sum of the ionic radii?
The sum of ionic radii is in fact very close to the observed equilibrium separation for many simple salts, because ionic radii are themselves defined (empirically, from crystal structure data) so as to approximately reproduce measured bond lengths when added together. But the underlying physical reason the bond length settles where it does is the energy-minimization argument in this article: attraction pulls ions together until the steeply rising repulsive term stops them. Ionic radii are a convenient bookkeeping tool built from many such measured values, not an independent physical explanation in themselves — the true explanation is the balance of Coulomb attraction against Pauli-exclusion-driven repulsion.
Does Born repulsion depend on the charges of the ions, the way the Coulomb term does?
Not directly through charge in the same explicit way. The Coulomb term contains explicitly because it comes from Coulomb's law for point charges. The repulsive term or instead depends on the sizes and electron configurations of the ions — how diffuse their outer electron shells are — which is only indirectly related to formal ionic charge (higher charge typically pulls electron density in and shrinks the ion, which affects and indirectly the repulsion parameters, but there is no explicit factor multiplying or the way there is in the Coulomb term).
Why do textbooks quote Born exponents n in the range 5 to 12 specifically?
The Born exponent is tied empirically to the electronic configuration of the ions involved — ions isoelectronic with He (n≈5), Ne (n≈7), Ar/Cu⁺ (n≈9), Kr/Ag⁺ (n≈10), and Xe/Au⁺ (n≈12) are the traditional assignments, with the exponent for a pair typically taken as the arithmetic mean of the two ions' individual values. Physically, more electron shells make an ion's electron cloud "harder" and more incompressible at short range (core electrons resist overlap more strongly than a single diffuse valence shell would), which shows up mathematically as needing a steeper power law, i.e. larger n, to fit the same compressibility data.
Is the Born repulsive term the same thing as van der Waals repulsion in the Lennard-Jones potential?
Conceptually yes — both represent short-range Pauli-exclusion-driven repulsion from overlapping electron clouds, and both are steep, short-ranged terms added to a longer-range attractive term to produce a stable energy minimum. The difference is context and the attractive partner term: the Lennard-Jones potential pairs a repulsive term with a dispersion (van der Waals) attractive term appropriate for neutral, non-bonded atoms or molecules, whereas the Born model pairs its repulsive term with a Coulomb attractive term appropriate for charged ions. The repulsive physics is the same family of phenomenon; the attractive physics differs completely.
Can Born repulsion ever be attractive, or become negative?
No — by construction or is always positive for and ; it represents a pure energy cost, never a stabilization. This is essential to the whole picture: the potential well exists only because a purely destabilizing, steeply rising term is added to a purely stabilizing, gently falling term. If the repulsive term could itself become attractive at some distance, it would not serve its physical role of preventing lattice collapse, and the entire justification for a finite equilibrium bond length would break down.
How does Born repulsion connect to why compounds like "NaCl₂" or "MgCl" don't exist?
Indirectly but importantly: the Born repulsion terms (through the ionic radii and the compressibility-derived curvature) set the equilibrium bond lengths that go into the full lattice energy (Born–Landé/Born–Haber) calculations used to test the stability of hypothetical compounds. A hypothetical "NaCl₂" would require Na²⁺, whose second ionization energy is enormous; the lattice energy gained (which depends on the ionic radii and hence indirectly on the repulsive-term-determined bond lengths) is nowhere near large enough to repay that ionization cost, so the compound is thermodynamically unstable relative to NaCl + Cl. The repulsive term itself doesn't cause this instability, but it is one of the necessary ingredients in the full energetic bookkeeping that reveals it.
Why does this article stop at a single ion pair instead of summing over the whole crystal?
Because the pairwise potential — Coulomb attraction plus Born repulsion between two ions — is the fundamental building block, and understanding its minimum, its curvature, and the meaning of the Born exponent is a prerequisite for the next step, which is summing this pairwise interaction over every ion in an infinite lattice using the Madelung constant. That summation, and the resulting closed-form lattice energy expression, is precisely the subject of the The Born-Lande Equation and its exponential refinement, The Born-Mayer Equation; both simply take the machinery built here and apply it lattice-wide.