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H3
                  MOLECULAR ORBITAL THEORY OF
                         DIATOMIC MOLECULES I



        Key Notes
                                Direct calculation of the molecular orbitals is possible only in the
                                       +
                                case of H 2 . For more complex molecules, a range of
                                approximations must be made in order to predict the nature of the
                                molecular orbitals. In all cases, it is necessary to assume that the
                                nuclei are stationary relative to the motion of the electrons. This
                                is known as the Born-Oppenheimer approximation, and allows
                                the internuclear geometry and motion to be treated completely
                                separately from that of the electrons.
                                                       +
                                In all cases other than that of H 2 , the molecular orbitals may be
                                approximately derived from a linear combination of atomic
                                orbitals. The atomic wavefunctions are combined in a linear
                                combination to give a molecular orbital,   ,
                                where c m  is the mixing coefficient. c m  may be varied for all the
                                atomic orbitals so as to minimize the energy of the resulting
                                molecular orbital. The variation principle states that the lowest
                                energy calculated orbital most accurately describes the actual
                                molecular wavefunction.
                                A molecular bonding orbital differs from the atomic orbitals from
                                which it is derived as it increases the probability of finding an
                                electron in the internuclear region. This reduces the free energy
                                of the electrons, and that of the molecule as a whole. Antibonding
                                molecular orbitals are derived by subtraction of one or more
                                atomic wavefunction from the others. The energy of the resulting
                                antibonding molecular orbital is greater than that of the atomic
                                orbitals, since a node in the internuclear electron density causes
                                an increase in the internuclear repulsion.
                                The stability of a molecule is heavily dependent upon the extent
                                to which the orbitals are allowed to overlap. The extent of the
                                orbital overlap is determined by the internuclear distance. At
                                relatively large separations, the energy decreases as the nuclei are
                                brought together, and the atomic orbital overlap increases,
                                whereas at low internuclear distances a repulsion term is
                                dominant. There is a point at which these two opposing effects
                                balance, and the molecule adopts its lowest free energy state. For
                                the antibonding orbital, there is a fully repulsive interaction
                                between the nuclei at any distance.
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