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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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BibTeXRIS

Bauschlicher, Charles W., Jr., Arnold, James O.. 1999-01-01. Accurate In Bond Energies. https://ntrs.nasa.gov/citations/20020080725

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