Pauling electronegativity Pauling first proposed later revised to 2.20 by Allred. It is also necessary to decide which of the two elements is the more electronegative (equivalent to choosing one of the two possible signs for the square root). This is usually done using "chemical intuition": in the above example,
hydrogen bromide dissolves in water to form H+ and Br− ions, so it may be assumed that bromine is more electronegative than hydrogen. However, in principle, since the same electronegativities should be obtained for any two bonding compounds, the data are overdetermined, and the signs are unique once a reference point has been fixed (usually, for H or F). To calculate Pauling electronegativity for an element, it is necessary to have data on the dissociation energies of at least two types of covalent bonds formed by that element. A. L. Allred updated Pauling's original values in 1961 to take account of the greater availability of thermodynamic data, with the units of
kilojoules per mole or
electronvolts. However, it is more usual to use a linear transformation to transform these absolute values into values that resemble the more familiar Pauling values. For ionization energies and electron affinities in electronvolts, \chi = 0.187(E_{\rm i} + E_{\rm ea}) + 0.17 \, and for energies in kilojoules per mole, \chi = (1.97\times 10^{-3})(E_{\rm i} + E_{\rm ea}) + 0.19. The Mulliken electronegativity can only be calculated for an element whose electron affinity is known.
Measured values are available for 72 elements, while approximate values have been
estimated or calculated for the remaining elements. The Mulliken electronegativity of an atom is sometimes said to be the negative of the
chemical potential. By inserting the energetic definitions of the ionization potential and electron affinity into the Mulliken electronegativity, it is possible to show that the Mulliken chemical potential is a finite difference approximation of the electronic energy with respect to the number of electrons., i.e., \mu(\rm Mulliken) = -\chi(\rm Mulliken) = {}-\frac{E_{\rm i} + E_{\rm ea}} 2
Allred–Rochow electronegativity A. Louis Allred and
Eugene G. Rochow considered that electronegativity should be related to the charge experienced by an electron on the "surface" of an atom: The higher the charge per unit area of atomic surface the greater the tendency of that atom to attract electrons. The
effective nuclear charge,
Zeff, experienced by
valence electrons can be estimated using
Slater's rules, while the surface area of an atom in a molecule can be taken to be proportional to the square of the
covalent radius,
rcov. When
rcov is expressed in
picometres, \chi = 3590{{Z_{\rm eff}}\over{r^2_{\rm cov}}} + 0.744
Sanderson electronegativity equalization R.T. Sanderson has also noted the relationship between Mulliken electronegativity and atomic size and has proposed a method of calculation based on the reciprocal of the atomic volume. With a knowledge of bond lengths, Sanderson's model allows the estimation of bond energies in a wide range of compounds. Sanderson's model has also been used to calculate molecular geometry,
s-electron energy,
NMR spin-spin coupling constants and other parameters for organic compounds. This work underlies the concept of
electronegativity equalization, which suggests that electrons distribute themselves around a molecule to minimize or equalize the Mulliken electronegativity. This behavior is analogous to the equalization of chemical potential in macroscopic thermodynamics.
Allen electronegativity Perhaps the simplest definition of electronegativity is that of Leland C. Allen, who has proposed that it is related to the average energy of the
valence electrons in a free atom, \chi = {n_{\rm s}\varepsilon_{\rm s} + n_{\rm p}\varepsilon_{\rm p} \over n_{\rm s} + n_{\rm p}} where
εs,p are the one-electron energies of s- and p-electrons in the free atom and
ns,p are the number of s- and p-electrons in the valence shell. The one-electron energies can be determined directly from
spectroscopic data, and so electronegativities calculated by this method are sometimes referred to as
spectroscopic electronegativities. The necessary data are available for almost all elements, and this method allows the estimation of electronegativities for elements that cannot be treated by the other methods, e.g.
francium, which has an Allen electronegativity of 0.67. However, it is not clear what should be considered to be valence electrons for the d- and f-block elements, which leads to an ambiguity regarding their electronegativities calculated by the Allen method. On this scale,
neon has the highest electronegativity of all elements, followed by
fluorine,
helium, and
oxygen. ==Correlation of electronegativity with other properties==