Abstract
Ab initio calculations of RgFn (Rg = Xe, Rn, and Element 118; n = 2, 4) were performed using relativistic effective core potentials and two-component HF, MP2, CCSD, and CCSD(T) methods. Geometries were optimized at the HF level with and without effective spin-orbit operators. The D4h, structures of all tetrafluorides and the linear difluorides are local minima with and without spin-orbit interactions. Spin-orbit contributions makes the Td form of (118)F4 another local minimum with the energy comparable to that of the D4h one. The spin-orbit interactions stabilize the (118) fluorides by a significant margin (∼2.0 eV) and the Rn fluorides by 40-60% (0.2∼ 0.4 eV) of the stabilization energy obtained at the corresponding scalar relativistic level. For (118)F4, the vibrational frequency of the B2u mode of the D4h form decreases from 143 to 20 cm-1 upon inclusion of the spin-orbit interactions, and a doubly degenerate mode of the Td structure, which is stable only with the inclusion of spin-orbit interactions, has the frequency of 34 cm-1, indicating that the (118)F4 molecule is very flexible due to spin-orbit effects.
| Original language | English |
|---|---|
| Pages (from-to) | 1104-1108 |
| Number of pages | 5 |
| Journal | Journal of Physical Chemistry A |
| Volume | 103 |
| Issue number | 8 |
| DOIs | |
| State | Published - 1999 |
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