2001
DOI: 10.1006/jmsp.2000.8234
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Submillimeter-Wave Spectroscopy of Phosphaalkynes: HCCCP, NCCP, HCP, and DCP

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Cited by 35 publications
(25 citation statements)
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“…We have fit only the diagonal elements of v, the nuclear quadrupole coupling constant tensor of 14 N, and C, the spin-rotation tensor of 31 P. The rotational constants, the centrifugal distortion constants, and the hyperfine constants of H 2 PCN are given in Table 2. Also presented in Table 2 are the results of the B3LYP ab initio calculation with the scaled rotational constants for the normal isotopomer as discussed previously.…”
Section: Assignment and Analysismentioning
confidence: 99%
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“…We have fit only the diagonal elements of v, the nuclear quadrupole coupling constant tensor of 14 N, and C, the spin-rotation tensor of 31 P. The rotational constants, the centrifugal distortion constants, and the hyperfine constants of H 2 PCN are given in Table 2. Also presented in Table 2 are the results of the B3LYP ab initio calculation with the scaled rotational constants for the normal isotopomer as discussed previously.…”
Section: Assignment and Analysismentioning
confidence: 99%
“…Ab initio B3LYP calculations of the nuclear spinrotation hyperfine constants for the 1 H, 14 N, and 31 P nuclei in H 2 PCN were performed and the results are given in Table 4 [32]. The calculated constants for the phosphorus nuclei are approximately an order of mag- nitude larger than those of hydrogen and nitrogen.…”
Section: Nuclear Spin-molecular Rotation Constants Of 31 Pmentioning
confidence: 99%
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“…Considering of the product distribution of CN with CH 2 CO, we think that some important and interesting carbon-phosphorusbearing molecules, such as HCP [19][20][21]22], HCCP [23][24][25][26][27], HOCP [28][29][30][31][32][33][34], CH 2 CP [35][36][37], and HCCCP [38][39][40], may be possible products in the reactions of carbon monophosphide (CP), the phosphorus analogue of CN, with CH 2 CO. The CP radical is a well-known interstellar molecule [41,42].…”
Section: Introductionmentioning
confidence: 99%
“…[35][36][37][38][39] Because of the real existence of the CP radical in interstellar cloud, it may react with possible hydrocarbons to form some important and interesting carbon-phosphorus-bearing products, such as HCP, [40][41][42] HCCP, 8,[43][44][45][46] and HCCCP, [47][48][49] which have received considerable attention in previous studies as possible candidates in interstellar observations. Therefore, those reactions should be attended, at least in laboratory studies.…”
Section: Introductionmentioning
confidence: 99%