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The electron-deficient compound diborane, B2H6, as noted earlier, can be regarded as a cluster of atoms held together by pairs of delocalized electrons that extend their binding influence over all electrons in the molecule. The unusual feature of diborane is the existence of B―H―B bridges as part of the cluster. Although an MO treatment of the molecule deals with it as a whole, chemists find it helpful to focus on this novel feature and to consider each B―H―B moiety as an example of a three-centre, two-electron bond (a 3c,2e bond, as shown in Figure 19). They regard diborane as three atoms held together by a pair of electrons delocalized over three atoms but are aware that this semilocalized picture is only a part of the true picture.

The usefulness of the concept of a 3c,2e bond stems from two observations. The first is that diborane is in fact only one of a large class of compounds of boron and hydrogen, the boranes and the borohydride anions, in which the same feature is found. The second observation is that a 3c,2e bond can be formed by three boron atoms. Intricate networks of atoms can be formed in this way—for example, some having the form of closed frameworks (the closo-boranes), some looking like untidy birds’ nests (the nido-boranes), and some resembling spiderwebs (the arachno-boranes). Which type of structure is obtained correlates with the number of valence electrons in the molecule, and the correlation is expressed by Wade’s rules. These rules are empirical, but they can be justified by a consideration of the numbers of 3c,2e and ordinary 2c,2e bonds that are needed in each type of structure. They constitute an excellent example of how chemists utilize the concept of bond formation and deploy a mixture of valence bond and molecular orbital concepts to establish or rationalize helpful correlations between the number of electrons present and the structure of the species.

Metal cluster compounds

A metal cluster compound is one in which metal atoms are linked directly to one another (Figure 20). A simple example is the ion Hg22+, in which two mercury (Hg) ions are linked together. A slightly more elaborate version is the ion [Re2Cl8]2−, in which there is a direct link between two rhenium (Re) atoms. Some metal cluster compounds have more than two metal atoms; an example is [Re3Cl12]3−, in which there are three rhenium atoms bonded together. It is sometimes difficult to determine whether the metal atoms are indeed directly linked or merely held quite close together by a framework of bridging ligands.

Metal cluster compounds warrant a special mention here because they provide the only examples of quadruple bonds in chemistry. Apart from that, their bonding can be treated as a straightforward exercise in MO or VB theory. Indeed, a metal cluster can be regarded as an exceedingly tiny sample of metal, with insufficient atoms present for the molecular orbitals to form a continuous band. The structure of [Re2Cl8]2− is shown in Figure 20. The clue to the existence of unusual bonding is the arrangement of the two sets of chloride ligands: to minimize repulsions between the atoms, each ReCl4 group might be expected to be twisted 45° relative to the next rather than being in the orientation shown. There appears to be a bonding feature between the two rhenium atoms that holds the groups as illustrated. This feature is taken to be a quadruple bond arising from the overlap of d orbitals on the two rhenium atoms.

One component in the structure of a quadruple bond is a σ bond formed by the cylindrically symmetrical overlap of two d orbitals. There are also two π bonds formed by the overlap of two appropriately orientated d orbitals. The new feature is the δ bond, which is formed by the face-to-face overlap of two parallel d orbitals and has a distinctly different symmetry with respect to the internuclear axis than the other two types of bond. A quadruple bond therefore consists of a σ bond, two π bonds, and one δ bond. The reduction in bond strength that would occur if one d orbital were rotated away from its partner so that overlap is lessened accounts for the torsional rigidity of the bond and the observed shape of the species.

Computational approaches to molecular structure

In conclusion, a brief introduction to the manner in which these qualitative ideas are implemented computationally follows. The computation of molecular structures by numerical solution of the Schrödinger equation is a highly developed discipline. The principal difficulty is the large number of interactions between electrons that must be taken into account; this fact makes computational quantum chemists some of the most demanding users of computers and, increasingly, of supercomputers.

There are two strands of approach to the computation of molecular structure. In the semiempirical approach, the calculation draws on a number of experimentally determined characteristics to help in the overall calculation. In the ab initio approach, the calculation proceeds from first principles (the Schrödinger equation) and makes no use of imported information. The former approach was dominant in the 1970s, but increases in computing power have led to an ascendancy of ab initio techniques since then. The latter are intrinsically more reliable because there can be no certainty that a quantity determined in one context is appropriate to a particular molecule.

The central aim of computations is to identify the lowest-energy arrangement of a given set of atoms and to identify that arrangement as the structure of the molecule. The calculational strategy adopted is to seek self-consistency in the calculation, and, for that reason, the computations are referred to as self-consistent field (SCF) procedures. Thus, a particular electronic distribution is proposed, and the distribution of the electrons is recalculated on the basis of this first approximation. The distribution is then calculated again on the basis of that improved description, and the process is continued until there is negligible change—i.e., until the electron distribution has achieved self-consistency.

The implementation of this basic strategy can take a number of forms, and rival techniques have given rise to a large number of acronyms, such as AM1 (Austin Method 1) and MINDO (Modified Intermediate Neglect of Differential Overlap), which are two popular semiempirical procedures.

With self-consistency established, the wave functions are available for detailed scrutiny. One illustration must suffice. There is certain evidence that carcinogenic or pharmacological activity correlates with certain aspects of the charge distribution in molecules. Instead of dealing with the primitive concept of partial charges, numerical wave functions can be used to map the details of the charge distribution and hence to screen molecules for possible activity. This approach is potentially of considerable utility for pharmaceutical products as it can help to reduce the amount of in vivo screening of novel products.

Computational procedures have advanced to the stage where the role of the environment (for example, the water around enzyme molecules) can be incorporated. They are also being applied to the demanding calculations that are needed to describe the replacement of one grouping of chemical bonds into another that takes place in the course of chemical reactions. Thus, as well as dealing with the static considerations of structure, modern treatments of the chemical bond are now confronting the dynamic problems of reactions.

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covalent bond

chemistry
Also known as: covalency, electron-pair bond, nonpolar bond

covalent bond, in chemistry, the interatomic linkage that results from the sharing of an electron pair between two atoms. The binding arises from the electrostatic attraction of their nuclei for the same electrons. A covalent bond forms when the bonded atoms have a lower total energy than that of widely separated atoms.

A brief treatment of covalent bonds follows. For full treatment, see chemical bonding: Covalent bonds.

Molecules that have covalent linkages include the inorganic substances hydrogen, nitrogen, chlorine, water, and ammonia (H2, N2, Cl2, H2O, NH3) together with all organic compounds. In structural representations of molecules, covalent bonds are indicated by solid lines connecting pairs of atoms; e.g.,

Structural formula.

A single line indicates a bond between two atoms (i.e., involving one electron pair), double lines (=) indicate a double bond between two atoms (i.e., involving two electron pairs), and triple lines (≡) represent a triple bond, as found, for example, in carbon monoxide (C≡O). Single bonds consist of one sigma (σ) bond, double bonds have one σ and one pi (π) bond, and triple bonds have one σ and two π bonds.

Covalent bonds are directional, meaning that atoms so bonded prefer specific orientations relative to one another; this in turn gives molecules definite shapes, as in the angular (bent) structure of the H2O molecule. Covalent bonds between identical atoms (as in H2) are nonpolar—i.e., electrically uniform—while those between unlike atoms are polar—i.e., one atom is slightly negatively charged and the other is slightly positively charged. This partial ionic character of covalent bonds increases with the difference in the electronegativities of the two atoms. See also ionic bond.

When none of the elements in a compound is a metal, no atoms in the compound have an ionization energy low enough for electron loss to be likely. In such a case, covalence prevails. As a general rule, covalent bonds are formed between elements lying toward the right in the periodic table (i.e., the nonmetals). Molecules of identical atoms, such as H2 and buckminsterfullerene (C60), are also held together by covalent bonds.

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Lewis formulation of a covalent bond

The idea that two electrons can be shared between two atoms and serve as the link between them was first introduced in 1916 by the American chemist G.N. Lewis, who described the formation of such bonds as resulting from the tendencies of certain atoms to combine with one another in order for both to have the electronic structure of a corresponding noble-gas atom.

In Lewis terms a covalent bond is a shared electron pair. The bond between a hydrogen atom and a chlorine atom in hydrogen chloride is formulated as follows:

The bond between a hydrogen atom and a chlorine atom in hydrogen chloride is formulated as per this process. (Lewis formulation of a covalent bond.)

In a Lewis structure of a covalent compound, the shared electron pair between the hydrogen and chlorine ions is represented by a line. The electron pair is called a bonding pair; the three other pairs of electrons on the chlorine atom are called lone pairs and play no direct role in holding the two atoms together.

Each atom in the hydrogen chloride molecule attains a closed-shell octet of electrons by sharing and hence achieves a maximum lowering of energy. In general, an incomplete shell means that some attracting power of a nucleus may be wasted, and adding electrons beyond a closed shell would entail the energetic disadvantage of beginning the next shell of the atom concerned. Lewis’s octet rule is again applicable and is seen to represent the extreme means of achieving lower energy rather than being a goal in itself.

A covalent bond forms if the bonded atoms have a lower total energy than the widely separated atoms. The simplest interpretation of the decrease in energy that occurs when electrons are shared is that both electrons lie between two attracting centres (the nuclei of the two atoms linked by the bond) and hence lie lower in energy than when they experience the attraction of a single centre.

Lewis structures of more complex molecules can be constructed quite simply by extending the process that has been described for hydrogen chloride. First, the valence electrons that are available for bonding are counted (2 × 1 + 6 = 8 in H2O, for example, and 4 + 4 × 7 = 32 in carbon tetrachloride, CCl4), and the chemical symbols for the elements are placed in the arrangement that reflects which are neighbours:

Step 1 in the construction of a Lewis structure for hydrogen chloride.

Next, one bonding pair is added between each linked pair of atoms:

Step 2 in the construction of a Lewis structure for hydrogen chloride.

The remaining electrons are then added to the atoms in such a way that each atom has a share in an octet of electrons (this is the octet-rule part of the procedure):

Step 3 in the construction of a Lewis structure for hydrogen chloride.

Finally, each bonding pair is represented by a dash:

Step 4 in the construction of a Lewis structure for hydrogen chloride.

(Note that Lewis structures do not necessarily show the actual shape of the molecule, only the topological pattern of their bonds.)

In some older formulations of Lewis structures, a distinction was made between bonds formed by electrons that have been supplied by both atoms (as in H―Cl, where one shared electron can be regarded as supplied by the hydrogen atom and the other by the chlorine atom) and covalent bonds formed when both electrons can be regarded as supplied by one atom, as in the formation of OH from O2− and H+. Such a bond was called a coordinate covalent bond or a dative bond and symbolized O → H. However, the difficulties encountered in the attempt to keep track of the origin of bonding electrons and the suggestion that a coordinate covalent bond differs somehow from a covalent bond (it does not) have led to this usage falling into disfavour.

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