1978
DOI: 10.1063/1.436650
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A bi n i t i o effective core potentials including relativistic effects. II. Potential energy curves for Xe2, Xe+2, and Xe*2

Abstract: Articles you may be interested inA b i n i t i o effective core potentials including relativistic effects. V. SCF calculations with ω-ω coupling including results for Au2 +, TlH, PbS, and PbSe Relativistic effects in a b i n i t i o effective core potential studies of heavy metal compounds. Application to HgCl2, AuCl, and PtH A b i n i t i o effective core potentials including relativistic effects. IV. Potential energy curves for the ground and several excited states of Au2 A b i n i t i o effective core poten… Show more

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Cited by 145 publications
(34 citation statements)
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“…24,25 At large internuclear distances the results from those studies were in qualitative agreement. For the 1 g state some bound character was predicted with a minimum in the potential at about 8 bohr, whereas for the 0 g ϩ state a fully dissociative potential was obtained as long as the state is described as an ion core with a 6s g Rydberg electron.…”
Section: Assignmentssupporting
confidence: 77%
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“…24,25 At large internuclear distances the results from those studies were in qualitative agreement. For the 1 g state some bound character was predicted with a minimum in the potential at about 8 bohr, whereas for the 0 g ϩ state a fully dissociative potential was obtained as long as the state is described as an ion core with a 6s g Rydberg electron.…”
Section: Assignmentssupporting
confidence: 77%
“…The Rydberg electron of these molecular excited states is of 6s g symmetry. 24,25 In Fig. 5 a diagram is presented in which molecular states derived from dimer electronic configurations are correlated to molecular states derived from the appropriate dissociation limits.…”
Section: Assignmentsmentioning
confidence: 99%
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“…Зачастую такой подход является вынуж денным, поскольку сведения о дипольных моментах переходов в димерах инер тных газов практически отсутствуют. Для интересующих нас переходов с учетом спин орбитального взаимодействия) нам известны данные только для Хе 2 [21] и Кr 2 [22].…”
Section: 2unclassified