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General Chemistry Principles, Patterns, and Applications, 2011

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could therefore be described quantitatively by the average of the values of its first ionization energy <strong>and</strong><br />

the absolute value of its electron affinity. Using our definition of electron affinity, we can write Mulliken’s<br />

original expression for electronegativity as follows: [1]<br />

Equation 7.15<br />

X =I+|EA|/2<br />

Elements with a large first ionization energy <strong>and</strong> a very negative electron affinity have a large positive<br />

value in the numerator of Equation 7.15, so their electronegativity is high. Elements with a small first<br />

ionization energy <strong>and</strong> a small electron affinity have a small positive value for the numerator in Equation<br />

7.15, so they have a low electronegativity. [2]<br />

As noted previously, all electronegativity scales give essentially the same results for one element relative<br />

to another. Even though the Mulliken scale is based on the properties of individual atoms <strong>and</strong> the Pauling<br />

scale is based on the properties of atoms inmolecules, they both apparently measure the same basic<br />

property of an element. In the following discussion, we will focus on the relationship between<br />

electronegativity <strong>and</strong> the tendency of atoms to form positive or negative ions. We will therefore be<br />

implicitly using the Mulliken definition of electronegativity. Because of the parallels between the Mulliken<br />

<strong>and</strong> Pauling definitions, however, the conclusions are likely to apply to atoms in molecules as well.<br />

Electronegativity Differences between Metals <strong>and</strong> Nonmetals<br />

An element’s electronegativity provides us with a single value that we can use to characterize the<br />

chemistry of an element. Elements with a high electronegativity (χ ≥ 2.2 in Figure 7.15 "Pauling<br />

Electronegativity Values of the ") have very negative affinities <strong>and</strong> large ionization potentials, so they are<br />

generally nonmetals <strong>and</strong> electrical insulators that tend to gain electrons in chemical reactions (i.e., they<br />

are oxidants). In contrast, elements with a low electronegativity (χ ≤ 1.8) have electron affinities that have<br />

either positive or small negative values <strong>and</strong> small ionization potentials, so they are generally metals <strong>and</strong><br />

good electrical conductors that tend to lose their valence electrons in chemical reactions (i.e., they<br />

are reductants). In between the metals <strong>and</strong> nonmetals, along the heavy diagonal line running from B to At<br />

in Figure 1.24 "The Periodic Table Showing the Elements in Order of Increasing ", is a group of elements<br />

with intermediate electronegativities (χ ~ 2.0). These are the semimetals, elements that have some of<br />

the chemical properties of both nonmetals <strong>and</strong> metals. The distinction between metals <strong>and</strong> nonmetals is<br />

Saylor URL: http://www.saylor.org/books<br />

Saylor.org<br />

633

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