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1.
The high-resolution infrared spectrum of HCF3 was studied in the ν6 fundamental (near 500 cm−1) and in the 2ν6 overtones (near 1000 cm−1) regions. The present study reports on the analysis of the hot bands in the ν6 region, as well as the first observation and assignment of the 2ν62 perpendicular band. Using ν6, 2ν6±2ν6±1 and 2ν62 experimental wavenumbers, accurate coefficients C0 and DK0 of the K-dependent ground-state energy terms were obtained, using the so-called “loop method.” Ground-state energy differences Δ(K,J)=E0(K,J)−E0(K−3,J) were obtained for K=3–30. A least-squares fit of 81 such differences gave the following results (in cm−1): C0=0.1892550(15); DK0=2.779(26) × 10−7.  相似文献   

2.
First measurements of line intensities for ν1 and ν3 bands of D232S are reported. About 300 intensities of D232S vibration–rotation lines were obtained from experimental high-resolution spectra recorded in the 1810–2051 cm−1 region with the Fourier Transform Spectrometer built in Reims. Empirical values of transition moment parameters for ν1 and ν3 bands of D232S were determined for the first time using a least-square fit to the observed intensities. Experimental D232S intensities were compared with recent global variational predictions [Vl.G. Tyuterev, L. Régalia-Jarlot, D.W. Schwenke, S.A. Tashkun, Y.G. Borkov, C. R. Phys. 5 (2004) 189–199] computed from isotopically invariant potential and dipole moment functions of the hydrogen sulphide molecule. Average discrepancy between these calculations and our observed data was 0.03 cm−1 for line positions of this spectral range. The discrepancy between these calculations and our measurements for the sum of line intensities was 5.5% and 3.5% for the ν1 and ν3 bands, correspondingly.  相似文献   

3.
The infrared (IR) spectrum of PD3 has been recorded in the 1580–1800 cm−1 range at a resolution of 0.0027 cm−1. About 2400 rovibrational transitions with J=K22 have been measured and assigned to the ν1 (A1) and ν3 (E) stretching fundamentals. These include 506 “perturbation-allowed” transitions with selection rules Δ(kl)=±3. Splittings of the K′′=3 lines have been observed. Effects of strong perturbations are evident in the spectrum. Therefore the rovibrational Hamiltonian adopted for the analysis explicitly takes into account the Coriolis and k-type interactions between the v1=1 and v3=1 states, and includes also several essential resonances within these states. The rotational structure in the v1=1 and v3=1 vibrational states up to J=K=18 was reproduced by fitting simultaneously all experimental data. Thirty-four parameters reproduced 1950 transitions retained in the final cycle with a standard deviation of the fit equal to 4.9 × 10−4 cm−1 (about the precision of the experimental measurements).  相似文献   

4.
The rotational structure of the ν3 fundamental of 14N16O2 has been recorded by employing a vacuum grating infrared spectrograph. The analysis has led to the assignment of over 500 R- and P-branch transitions in the spectral region 1562–1650 cm−1. Molecular constants for the upper state, 001, have been presented. No Q-branch transitions were used in the evaluation of these constants. The presently obtained and the band center ν0 = 1616.846 cm−1 differ significantly from previous determinations. Spin splitting was observed but no information was extracted about upper state spin splitting parameters.  相似文献   

5.
We present the high resolution absorption measurements of gaseous HONO at room temperature using continuous-wave cavity ring-down spectroscopy in the near-infrared region between 6017 and 6067 cm−1 at a resolution of 1 pm (0.037 cm−1). For the trans-HONO isomer an extensive analysis of the ν1+2ν3 combination band 6045.8089 cm–1 was performed starting from the results of a previous study for the 11 and 31 vibrational states [Guilmot J-M, Godefroid M, Herman M. Rovibrational parameters for trans-nitrous acid. J Mol Spectrosc 1993;160:387–400]. The present combination band is perturbed because of the existence of several dark states of HONO which could not be identified unambiguously. The rotational constants achieved for the 1132 state deviate slightly from the values which are predicted from the rotational constants achieved in the previous studies for the 11 and 31 vibrational states of trans-HONO.  相似文献   

6.
The Coriolis-coupled band system of ν5, ν2, and 2ν3 of CD3I was analyzed by making use of all of the experimental data now available. These data included the high-resolution infrared spectra, microwave spectra, and laser Stark spectra. The analysis gave values, more precise than before, of the spectroscopic constants for ν5, ν2, and 2ν3 and the interaction constants. The determination of the rotational constant A for 2ν3 gave a value for , with which all of the αA constants for CD3I have been completed. These αA values were incorporated with the known value of A6 to give a value for A0.  相似文献   

7.
Using 0.002 cm−1 resolution Fourier transform absorption spectra of an 17O-enriched ozone sample, an extensive analysis of the ν3 band together with a partial identification of the ν1 band of the 17O16O17O isotopomer of ozone has been performed for the first time. As for other C2v-type ozone isotopomers [J.-M. Flaud and R. Bacis, Spectrochim. Acta, Part A 54, 3–16 (1998)], the (001) rotational levels are involved in a Coriolis-type resonance with the levels of the (100) vibrational state. The experimental rotational levels of the (001) and (100) vibrational states have been satisfactorily reproduced using a Hamiltonian matrix which takes into account the observed rovibrational resonances. In this way precise vibrational energies and rotational and coupling constants were deduced and the following band centers ν03) = 1030.0946 cm−1 and ν01) = 1086.7490 cm−1 were obtained for the ν3 and ν1 bands, respectively.  相似文献   

8.
An updated analysis of the full NOMAD data corresponding to 1.35 × 106 charged current interactions has been performed to search for neutrino oscillations through ντ appearance. This document updates the recently published results on the νμ → ντ and νμ → νe oscillations search in NOMAD [1] with a unified analysis of the hadronic channels.  相似文献   

9.
New measurements are reported for the infrared spectrum of sulfur trioxide, 32S16O3, with resolutions ranging from 0.0015 cm−1 to 0.0025 cm−1. Rovibrational constants have been measured for the fundamentals ν2, ν3, and ν4 and the overtone band 2ν3. Comparisons are made with the earlier high-resolution measurements on SO3, and the high correlation among some of the constants related to the Coriolis coupling of the ν2 and ν4 levels is discussed in order to understand the areas of disagreement with the earlier work. Splittings of some of the levels are observed and the splitting constant for K=3 of the ground state is determined for the first time. Other observed splittings include the K=1 levels of 2ν3 (l=2), the K=2 levels of ν3 and ν4, and the K=3 levels of ν2. The analysis shows that there are level crossings between the l=0 and l=2 states of 2ν3 that allow one to determine the separation of the subband centers for these two states even though access to the l=0 state from the ground state is electric-dipole forbidden. This is a generalized phenomenon that should be found for many other molecules with the same symmetry. The l-type resonance constant, q3, that causes the splitting of the l3=±1, k=±1 levels of ν3 also couples the l3=0 and 2 states of 2ν3.  相似文献   

10.
This paper is devoted to the third part of the analysis of the very weak absorption spectrum of the 18O3 isotopologue of ozone recorded by CW-Cavity Ring Down Spectroscopy between 5930 and 6900 cm−1. In the two first parts [A. Campargue, A. Liu, S. Kassi, D. Romanini, M.-R. De Backer-Barilly, A. Barbe, E. Starikova, S.A. Tashkun, Vl.G. Tyuterev, J. Mol. Spectrosc. (2009), doi: 10.1016/j.jms.2009.02.012 and E. Starikova, M.-R. De Backer-Barilly, A. Barbe, Vl.G. Tyuterev, A. Campargue, A.W.Liu, S. Kassi, J. Mol. Spectrosc. (2009) doi: 10.1016/j.jms.2009.03.013], the effective operators approach was used to model the spectrum in the 6200–6400 and 5930–6080 cm−1 regions, respectively. The analysis of the whole investigated region is completed by the present investigation of the 6490–6900 cm−1 upper range. Three sets of interacting states have been treated separately. The first one falls in the 6490–6700 cm−1 region, where 1555 rovibrational transitions were assigned to three A-type bands: 3ν2 + 5ν3, 5ν1 + ν2 + ν3 and 2ν1 + 3ν2 + 3ν3 and one B-type band: ν1 + 3ν2 + 4ν3. The corresponding line positions were reproduced with an rms deviation of 18.4 × 10−3 cm−1 by using an effective Hamiltonian (EH) model involving eight vibrational states coupled by resonance interactions. In the highest spectral region – 6700–6900 cm−1 – 389 and 183 transitions have been assigned to the ν1 + 2ν2 + 5ν3 and 4ν1 + 3ν2 + ν3 A-type bands, respectively. These very weak bands correspond to the most excited upper vibrational states observed so far in ozone. The line positions of the ν1 + 2ν2 + 5ν3 band were reproduced with an rms deviation of 7.3 × 10−3 cm−1 by using an EH involving the {(054), (026), (125)} interacting states. The coupling of the (431) upper state with the (502) dark state was needed to account for the observed line positions of the 4ν1 + 3ν2 + ν3 band (rms = 5.7 × 10−3 cm−1).The dipole transition moment parameters were determined for the different observed bands. The obtained set of parameters and the experimentally determined energy levels were used to generate a complete line list provided as Supplementary Materials.The results of the analyses of the whole 5930–6900 cm−1 spectral region were gathered and used for a comparison of the band centres to their calculated values. The agreement achieved for both 18O3 and 16O3 (average difference on the order of 1 cm−1) indicates that the used potential energy surface provides accurate predictions up to a vibrational excitation approaching 80% of the dissociation energy. The comparison of the 18O3 and 16O3 band intensities is also discussed, opening a field of questions concerning the variation of the dipole moments and resonance intensity borrowing by isotopic substitution.  相似文献   

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