The pure rotational spectrum of HPS ((X)over-tilde1A′): Chemical bonding in second-row elements

被引:19
|
作者
Halfen, D. T. [1 ,2 ,3 ]
Clouthier, D. J. [4 ]
Ziurys, L. M. [1 ,2 ,3 ]
Lattanzi, V. [5 ,6 ]
McCarthy, M. C. [5 ,6 ]
Thaddeus, P. [5 ,6 ]
Thorwirth, S. [7 ,8 ]
机构
[1] Univ Arizona, Dept Chem, Arizona Radio Observ, Tucson, AZ 85721 USA
[2] Univ Arizona, Dept Astron, Arizona Radio Observ, Tucson, AZ 85721 USA
[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[4] Univ Kentucky, Dept Chem, Lexington, KY 40506 USA
[5] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02318 USA
[6] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02318 USA
[7] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[8] Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany
来源
JOURNAL OF CHEMICAL PHYSICS | 2011年 / 134卷 / 13期
基金
美国国家科学基金会;
关键词
CORRELATED MOLECULAR CALCULATIONS; MATRIX IR INVESTIGATIONS; AB-INITIO CALCULATIONS; GAUSSIAN-BASIS SETS; CIRCUMSTELLAR ENVELOPES; EQUILIBRIUM STRUCTURE; PHOSPHORUS CHEMISTRY; MICROWAVE-SPECTRA; INFRARED-SPECTRUM; INTERSTELLAR PN;
D O I
10.1063/1.3562374
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
The pure rotational spectrum of HPS, as well as its S-34 and D isotopologues, has been recorded at microwave, millimeter, and submillimeter wavelengths, the first observation of this molecule in the gas phase. The data were obtained using a combination of millimeter direct absorption, Fourier transform microwave (FTMW), and microwave-microwave double-resonance techniques, which cover the total frequency range from 15 to 419 GHz. Quantum chemical calculations at the B3LYP and CCSD(T) levels were also performed to aid in spectral identification. HPS was created in the direct absorption experiment from a mixture of elemental phosphorus, H2S, and Ar carrier gas; DPS was produced by adding D-2. In the FTMW study, these species were generated in a pulsed discharge nozzle from PH3 and H2S or D2S, diluted in neon. The spectra recorded for HPS and its isotopologues exhibit clear asymmetric top patterns indicating bent structures; phosphorus hyperfine splittings were also observed in HPS, but not DPS. Analysis of the data yielded rotation, centrifugal distortion, and phosphorus nuclear spin-rotation parameters for the individual species. The r(m)((1)) structure for HPS, calculated from the rotational constants, is r(H-P) = 1.438(1) angstrom, r(P-S) = 1.9320(1) angstrom, and theta(H-P-S) = 101.85(9)degrees. Empirically correcting for zero-point vibrational effects yields the geometry r(e)(H-P) = 1.4321(2) angstrom, r(e)(P-S) = 1.9287(1) angstrom, and theta(e)(H-P-S) = 101.78(1)degrees, in close agreement with the r(m)((1)) structure. A small inertial defect was found for HPS indicating a relatively rigid molecule. Based on these data, the bonding in this species is best represented as H-P=S, similar to the first-row analog HNO, as well as HNS and HPO. Therefore, substitution of phosphorus and sulfur for nitrogen and oxygen does not result in a dramatic structural change. (C) 2011 American Institute of Physics. [doi: 10.1063/1.3562374]
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页数:9
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