1999
DOI: 10.1088/0953-4075/32/23/301
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Configuration interaction calculations of miscellaneous properties of the X2Pirground state, the C´2Delta excited state and related C´2Delta-X2Pirtransition bands of PO: I. X2Pirground state

Abstract: Extended basis set configuration interaction calculations on the ground state (X 2 r ) of PO have been performed. A wide variety of molecular properties are reported, including: (i) spectroscopic constants; (ii) vibrational energies and anharmonicity effects; (iii) pure rotational transitions for several (J , J ) sets and the first 11 vibrational quantum numbers; (iv) one-electron properties such as the electric dipole/quadrupole moments, nuclear quadrupole ( 17 O) coupling, anisotropic hyperfine parameters, e… Show more

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Cited by 11 publications
(8 citation statements)
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“…By comparison with the experiments, it is easy to find that their accuracy is inferior to the presents expect for ω e of b 4 Σ − and C 2 Σ − with respect to PO. The same MRCI+Q method was adopted by de Brouckère52 to calculate the ground state properties of PO with aug‐cc‐pVQZ basis set. From Table I, it is not difficult to find that the values of B e and α e are still smaller than the experiments11.…”
Section: Resultsmentioning
confidence: 99%
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“…By comparison with the experiments, it is easy to find that their accuracy is inferior to the presents expect for ω e of b 4 Σ − and C 2 Σ − with respect to PO. The same MRCI+Q method was adopted by de Brouckère52 to calculate the ground state properties of PO with aug‐cc‐pVQZ basis set. From Table I, it is not difficult to find that the values of B e and α e are still smaller than the experiments11.…”
Section: Resultsmentioning
confidence: 99%
“…In theory, a number of ab initio calculations were performed on the low‐lying electronic states of PO and PO + 39–56. However, the extracted spectroscopic properties from the theoretical work mainly focus on the spectroscopic parameters ( D e , R e , ω e , ω e χ e , α e , B e ).…”
Section: Introductionmentioning
confidence: 99%
“…A brief history of the experimental work on PO is given by de Brouckère. 65 It is worth noting that PO is believed to exist in dense interstellar clouds although evidence of its presence there is not yet conclusive. 48 In contrast to the experimental work, the theoretical investigation of these species has not been extensive.…”
Section: Introductionmentioning
confidence: 99%
“…48 In contrast to the experimental work, the theoretical investigation of these species has not been extensive. [52][53][54][55][56][57][58][59][60][61][62][63][64][65][66] The first calculations on PO and its anion were done as early as 1966 by Boyd and Lipscomb 52 at the self-consistent field/ Slater type orbitals ͑SCF/STO͒ level, and their results for the PO Ϫ were the only ones available for some time. In 1971 Mulliken and Liu 53 repeated the calculations on PO at the SCF/STO level with a larger basis set as part of their investigation of the importance of the d and f functions in the chemical bond.…”
Section: Introductionmentioning
confidence: 99%
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