Bond-dissociation energy 2026-10-13
A bond-dissociation energy specifies the energy needed for a stated dissociation into separated fragments. An energy from the lowest vibrational state, an energy from the bottom of a potential energy well, and a finite-temperature molar dissociation enthalpy require different conventions; do not silently mix them in an electronegativity formula.
Which fragments, in which quantum states, and at which temperature? For a neutral gaseous molecule with a specified two-electron covalent bond, the usual thermochemical convention is homolysis,
Each fragment receives one of the two bonding Electrons; the dots denote unpaired Electrons. The final fragments are isolated from each other, with their own relaxed molecular geometry and specified electronic quantum states. The energy cost includes this relaxation, rather than merely stretching the initial chemical bond while freezing everything else. For a neutral parent, heterolysis instead produces , or the opposite assignment of electric charges; those are different final states and different energies. A value for gaseous neutral fragments cannot be transferred to ions, a chemical solution, or a solid without accounting for those changed conditions.[ref]
The distinction is useful beyond terminology. Pauling electronegativity compares consistently defined bond-dissociation energies; photodissociation can reveal a specified ground-state threshold; a thermal chemical reaction balance requires compatible enthalpies. A threshold is also different from an activation energy: it compares initial and final quantum states, whereas a barrier can obstruct the path between them.
Born-Haber cycle 2026-10-14
A Born-Haber cycle uses Hess's law to infer a lattice energy from measurable enthalpy differences and isolated-species data. The motivating difficulty is that separating a mole of an ionic crystal into mutually separated gaseous ions is not a convenient direct calorimetry experiment. Instead, compare two accounting routes between the same elemental reference states and the same solid. Because enthalpy is a state function, the signed differences close exactly when all inputs describe compatible states. These routes do not assert a reaction mechanism or a temporal sequence of reaction intermediates.[ref]
For one mole of sodium chloride formula units, the overall formation reaction is
The stoichiometry requires half a mole of diatomic chlorine molecules, supplying one mole of chlorine chemical atoms. A half coefficient counts an amount of substance; it does not describe half of an individual molecule. Write each auxiliary chemical reaction with its own sign:
Here is the sublimation enthalpy, the enthalpy of atomization of chlorine per mole of chemical atoms, and the molar ionization enthalpy represented by the ionization energy input in elementary treatments. If the bond-dissociation energy table gives the compatible molar enthalpy for , use half that number for . Both ions in the last step are gaseous, and no aqueous hydration of ions belongs in that step.
Adding these equations cancels the gaseous chemical atoms, the gaseous ions and the free Electron, leaving precisely the overall formation reaction. Thus
The closed traversal returns from the solid to the elemental reference states, adding ; therefore . Notice that the signed attachment term is negative. Substituting a positive spectroscopic electron affinity for would reverse the attachment contribution.
Figure 1.
A closed Born-Haber cycle for sodium chloride using explicitly synthetic molar enthalpies: levels represent complete material inventories, and horizontal position is bookkeeping rather than a reaction coordinate
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The diagram deliberately uses invented, internally consistent inputs in : , , , and . Preparation of separated gaseous ions raises the enthalpy by , so and . The closure check is . These numbers are not measured sodium chloride data and do not replace the source's example in lattice energy. Every level retains one sodium nucleus, one chlorine nucleus and zero total electric charge; the ionization level explicitly retains the free Electron.
A tabulated electronegativity is useful because it compresses many comparisons, but one number per chemical element suppresses chemical context. Changing the bonded partners, bond length or electron configuration changes the conditions under which a chemical atom attracts electron density. The bond-dissociation energy can change for reasons beyond bond polarization, so attributing every extra unit of energy solely to an electronegativity difference is an approximation.[ref]
An oxidation state labels a formal allocation of Electrons; it is not a measured partial atomic charge. State-sensitive electronegativity models may give different values for different oxidation states or electron configurations, while a simple chemical element table intentionally provides a common comparison convention. Likewise, replacing an isolated chemical atom by a site in an ionic crystal introduces a surrounding electric field and many neighbours. Applying the same tabulated electronegativity without adjustment becomes an additional assumption.[ref]
For the ground-state Mulliken scale, the state dependence is visible directly in the formula. Replacing by replaces with as the removal cost, and replaces with as the attachment release. These are different ionization energies and electron affinities. This isolated-ion arithmetic does not claim that a bonded chemical atom with the same formal oxidation state is an isolated ion. In a molecule, the actual electron density and dipole evidence for bond polarization supply complementary information about that environment.
Enthalpy of atomization 2026-10-13
An enthalpy of atomization is the enthalpy change for making one mole of separated gaseous chemical atoms from a specified starting chemical substance. For sodium, the relevant step is sublimation to monatomic gas; for diatomic chlorine, it is half the compatible molar bond-dissociation energy expressed as an enthalpy.
The contrast between Pauling electronegativity and Mulliken electronegativity becomes clearer by following the measurements into the formulas. A Pauling bond-energy excess compares three compatible bond-dissociation energies; Mulliken electronegativity takes the arithmetic mean of an ionization energy and an electron affinity. The former asks how much stronger an unlike-atom chemical bond is than a stipulated baseline; the latter combines two different isolated-species energy gaps.
Actual readouts precede those model choices. In the nitrogen dissociation threshold from fragment images, fitted squared image radii versus assigned excitation energies reveal a threshold after accounting for the product quantum states. In the chlorine photodetachment threshold experiment, mass-selected anions overlap a tunable laser, and neutral-atom counts reveal the onset of Electron detachment. Opposite laser directions control the Doppler shift. That second threshold supplies an electron affinity, not an electronegativity; the Mulliken scale still needs an independent ionization energy.[ref][ref]
For an original arithmetic comparison, stipulate isolated-species and positive attachment-release for fictitious species . Their Mulliken electronegativities are . The largest ionization energy belongs to , while the largest Mulliken electronegativity belongs to : accepting an Electron matters as well as retaining one. Using signed attachment energies in gives exactly the same results.
Figure 1.
Stipulated inputs to Mulliken electronegativity and arithmetic-baseline Pauling electronegativity: different energies, units and orderings
. Details.
Independently stipulate and for , with unlike-atom values
Thus , and the Pauling scale differences from are . If all three fictitious species are placed above on that scale, their ordering is , whereas the stipulated Mulliken scale gives . The bond-dissociation energies and isolated-species energies were invented independently: this demonstrates what the formulas do, not a measured disagreement for actual chemical elements. A unit conversion cannot force these two input models to agree.
A Pauling bond-energy excess subtracts a chosen like-atom baseline from the unlike-atom bond-dissociation energy. For an unequal-input arithmetic example, stipulate , and , all with one dissociation convention. The arithmetic mean baseline and excess are
The arithmetic-baseline Pauling scale model therefore gives . The bond-dissociation energy is not itself the excess: subtracting the baseline is essential. All three numbers are stipulated, not experimental values for named chemical elements.
Changing the baseline changes the model. For the same stipulated inputs, a geometric mean baseline would be , yielding an excess of and a difference of approximately . It is a different construction, even though both start from the same bond-dissociation energies. State which baseline is used before comparing electronegativity differences.
The arithmetic-baseline Pauling scale also has a useful inverse: a difference of corresponds to an excess of , and a difference of corresponds to . Doubling the electronegativity difference quadruples the modeled excess. Interchanging the endpoint labels changes neither quantity; the square root alone cannot choose the direction of bond polarization.
In The Nature of the Chemical Bond. IV. The Energy of Single Bonds and the Relative Electronegativity of Atoms (printed pp. 3576–3578, Table II and equation (1)), Linus Pauling organized excess energies for chemical bonds into an approximately additive map of their square roots. He also identified a limitation: his H–F map separation of predicted an excess of , exceeding his table's value by . Those are historical values and a historical model discrepancy, not modern recommended inputs.[ref]
Pauling electronegativity 2026-10-13
Pauling electronegativity is a relative, dimensionless scale motivated by bond-dissociation energies. The interesting observation is that a chemical bond between unlike chemical atoms can be stronger than a simple baseline inferred from the corresponding like-atom chemical bonds. An empirical excess energy can then be associated with an electronegativity difference. The 1932 paper The Nature of the Chemical Bond. IV. The Energy of Single Bonds and the Relative Electronegativity of Atoms built such a map; its original coordinates used hydrogen as zero, so those coordinates should not be mistaken for the modern tabulated Pauling electronegativities.[ref]
One arithmetic-baseline version of the Pauling scale relation is
Here , and are consistently defined bond-dissociation energies per molecule, and the arithmetic mean is the chosen baseline. With molar energies instead, write , approximately . The denominator makes the result dimensionless; the factor is not a unit-independent magic constant. This is an empirical relation with a specified baseline, not a definition valid for every chemical bond.[ref]
For an explicitly synthetic example, suppose and with the same temperature and dissociation convention. Then and the model gives an electronegativity difference of . Replacing by gives zero; a negative excess would make this real square-root model inapplicable, not produce a negative electronegativity difference. These invented inputs illustrate the formula and are not measurements of named chemical substances.
Only differences appear, so adding the same constant to every Pauling electronegativity leaves this relation unchanged. A reference value must fix the origin. The bond-dissociation energies alone also do not tell which endpoint attracts electron density more strongly, because interchanging and leaves the formula unchanged. Chemical comparisons fix that direction. Thus Pauling electronegativity is useful as a compact ordering, while the underlying measured energies and approximations remain essential.