NASA NTRS · 20020080725
Accurate In Bond Energies
Abstract
InXn atomization energies are computed for n = 1-3 and X = H, Cl, and CH3. The geometries and frequencies are determined using density functional theory. The atomization energies are computed at the coupled cluster level of theory. The complete basis set limit is obtained by extrapolation. The scalar relativistic effect is computed using the Douglas-Kroll approach. While the heats of formation for InH, InCl and InCl3 are in good agreement with experiment, the current results show that the experimental value for In(CH3)3 must be wrong.
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Bauschlicher, Charles W., Jr., Arnold, James O.. 1999-01-01. Accurate In Bond Energies. https://ntrs.nasa.gov/citations/20020080725
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