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1.
Using a Fourier transform spectrometer, we have recorded the spectra of ozone in the region of 4600 cm−1, with a resolution of 0.008 cm−1. The strongest absorption in this region is due to the ν1+ ν2+ 3ν3band which is in Coriolis interaction with the ν2+ 4ν3band. We have been able to assign more than 1700 transitions for these two bands. To correctly reproduce the calculation of energy levels, it has been necessary to introduce the (320) state which strongly perturbs the (113) and (014) states through Coriolis- and Fermi-type resonances. Seventy transitions of the 3ν1+ 2ν2band have also been observed. The final fit on 926 energy levels withJmax= 50 andKmax= 16 gives rms = 3.1 × 10−3cm−1and provides a satisfactory agreement of calculated and observed upper levels for most of the transitions. The following values for band centers are derived: ν01+ ν2+ 3ν3) = 4658.950 cm−1, ν0(3ν1+ 2ν2) = 4643.821 cm−1, and ν02+ 4ν3) = 4632.888 cm−1. Line intensities have been measured and fitted, leading to the determination of transition moment parameters for the two bands ν1+ ν2+ 3ν3and ν2+ 4ν3. Using these parameters we have obtained the following estimations for the integrated band intensities,SV1+ ν2+ 3ν3) = 8.84 × 10−22,SV2+ 4ν3) = 1.70 × 10−22, andSV(3ν1+ 2ν2) = 0.49 × 10−22cm−1/molecule cm−2at 296 K, which correspond to a cutoff of 10−26cm−1/molecule cm−2.  相似文献   

2.
Raman spectroscopy has been used to study the rare‐earth mineral churchite‐(Y) of formula (Y,REE)(PO4) ·2H2O, where rare‐earth element (REE) is a rare‐earth element. The mineral contains yttrium and, depending on the locality, a range of rare‐earth metals. The Raman spectra of two churchite‐(Y) mineral samples from Jáchymov and Medvědín in the Czech Republic were compared with the Raman spectra of churchite‐(Y) downloaded from the RRUFF data base. The Raman spectra of churchite‐(Y) are characterized by an intense sharp band at 975 cm−1 assigned to the ν1 (PO43−) symmetric stretching mode. A lower intensity band observed at around 1065 cm−1 is attributed to the ν3 (PO43−) antisymmetric stretching mode. The (PO43−) bending modes are observed at 497 cm−12) and 563 cm−14). Some small differences in the band positions between the four churchite‐(Y) samples from four different localities were found. These differences may be ascribed to the different compositions of the churchite‐(Y) minerals. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

3.
The bending vibration-rotation band ν4 of DCCF was studied. The measurements were carried out with a Fourier spectrometer at a resolution of about 0.03 cm?1. The constants B0=0.29141(1)cm?1, α4=?5.02(2)×10?4cm?1, q4=4.52(3)×10?4cm?1, and D0=9.2(4)×10?8cm?1 were derived. The rotational analysis of the “hot” bands 2ν4(Δ) ← ν4(II) and 2ν4+) ← ν4(II) was performed. In addition, the “hot” bands ν4 + ν5 ← ν5 were assigned. A set of vibrational constants involved was derived.  相似文献   

4.
The water vapour line-broadening (γ) and shift (δ) coefficients for 310 lines of 10 vibrational bands ν1, ν3, 2ν2, ν1+ ν2, ν2+ ν3,23, 2ν1, ν1+ ν3, 2ν3 and ν1 +2ν2 induced by argon pressure were measured with a Bruker IFS HR 125 spectrometer. The measurements were performed at room temperature, at the spectral resolution of 0.01 cm1 and over a wide pressure range of Ar. The calculations of the broadening coefficients γ and δ were performed in the framework of the semi-classical method. The intermolecular potential was taken as the sum of the atom–atom potential and the vibrationally and rotationally dependent isotropic induction+dispersion potential. The measured γ and δ were combined with literature data for the ν2 and 3ν13, 2ν1+2ν23 vibrational bands, and the optimal sets of potential parameters that gave the best agreement with the measured broadening coefficients for each vibrational band separately were found. Then, combined experimental data of 13 vibrational bands of H2O perturbed by Ar were used to determine the analytical dependence of some potential parameters on vibrational quantum numbers.  相似文献   

5.
We measured 305 absolute line intensities in the ν13+u)-0(Σ+g) band of 12C2H2 and 13C12CH2 and the ν12+(ν14−15)0+u)-0(Σ+g), ν1314g)-ν14g), and ν1351u)-ν51u) bands of the main isotopomer, all observed near 1.5 μm. The absolute intensity of these bands are respectively 6.4882 (34), 0.12337 (10), 0.083746 (71), 0.58771 (28), and 0.32126 (11) cm−2 atm−1 at 296 K. In addition, we also determined Herman-Wallis factors for the first time in this spectral region.  相似文献   

6.
The structures of LiTiPO5 and LiTi2(PO4)3, as well as the possibility of oxygen vacancies formation in the systems are studied by first-principles calculations. It is found that oxygen vacancies can be formed in LiTiPO5 and LiTi2(PO4)3 under oxygen poor condition. The formation of oxygen vacancies introduce a defect band within their band gaps, which is expected to improve the electronic conductivity of LiTiPO5 and LiTi2(PO4)3 significantly. Meanwhile, a great concentration of oxygen vacancies may increase the discharge voltage of LiTiPO5 and LiTi2(PO4)3.  相似文献   

7.
Li1.3Al0.15Y0.15Ti1.7(PO4)3 compound was synthesized by solid-state reaction, and ceramics were sintered. The surfaces of the ceramics were investigated by scanning electron microscopy and X-ray photoelectron spectroscopy. Li1.3Al0.15Y0.15Ti1.7(PO4)3 samples were tested in solid galvanic cells Ag|O2+CO2|Li2CO3|Li1.3Al0.15Y0.15Ti1.7(PO4)3|LiMnO2+Mn2O3|O2|Ag. The electromotive force measurements of this cell indicated that investigated samples are practically pure Li-ion conductors. Impedance spectroscopy studies have been performed in the frequency range 10?2–3·109 Hz and temperatures from ?57 °C to 334 °C. Three dispersion regions related to Li+ ionic transport in bulk, grain boundaries of the ceramics and to polarization of electrodes have been found. Total conductivity changes according to Arrhenius law in the studied temperature range, but an anomalous behavior was observed for the bulk conductivity of the ceramics.  相似文献   

8.
Solid electrolyte Li1.3Al0.3Ti1.7(PO4)3 was prepared by sol-gel method under different sintering conditions. The structural identification, surface morphology, electrochemical window, ionic conductivity, and activation energy of the Li1.3Al0.3Ti1.7(PO4)3 sintered pellets were investigated by X-ray diffraction, scanning electron microscopy, cyclic voltammetry, and electrochemical impedance spectroscopy. It is found that the sintering temperature and time have considerable effect on the properties of the Li1.3Al0.3Ti1.7(PO4)3 sintered pellets. The Li1.3Al0.3Ti1.7(PO4)3 pellet sintered at 900 °C for 2 h is denser than the pellets sintered at other conditions. Different sintering conditions result in the sintered pellet with different porosity. However, the sintering conditions have little effect on the electrochemical window of Li1.3Al0.3Ti1.7(PO4)3. Among the Li1.3Al0.3Ti1.7(PO4)3 pellets sintered at various conditions, the pellet sintered at 900 °C for 2 h shows the highest ionic conductivity of 3.46 × 10−4 S cm−1 and the lowest activation energy of 0.2821 eV.  相似文献   

9.
The spectral characteristics of the SiF4 molecule in the range 3100–700 cm?1, including the absorption range of the band ν3, are studied in the gas phase at P = 0.4–7 bar and in solutions in liquefied Ar and Kr. In the cryogenic solutions, the relative intensities of the vibrational bands, including the bands of the isotopically substituted molecules, are determined. The absorption coefficients of the combination bands 2ν3, ν3 + ν1, ν3 + ν4, and 3ν4 are measured in the solution in Kr. In the gas phase of the one-component system at an elevated pressure of SiF4, the integrated absorption coefficient of the absorption band ν3 of the 28SiF4 molecule was measured to be A3) = 700 ± 30 km/mol. Within the limits of experimental error, this absorption coefficient is consistent with estimates obtained from independent measurements and virtually coincides with the coefficient A3) = 691 km/mol calculated in this study by the quantum-chemical method MP2(full) with the basis set cc-pVQZ.  相似文献   

10.
The structures of the naturally occurring sulfite‐bearing minerals scotlandite, hannebachite and orschallite have been studied by Raman spectroscopy. Raman bands are observed for scotlandite PbSO3 at 935, 880, 622 and 474 cm−1 and are assigned to the (SO3)2−ν1(A1), ν3(E), ν2(A1) and ν4(E) vibrational modes, respectively. For hannebachite (CaSO3)2·H2O these bands are observed at 1005, 969 and 655 cm−1 with multiple bands for the ν4(E) mode at 444, 492 and 520 cm−1. The Raman spectrum of hannebachite is very different from that of the compound CaSO3·2H2O. It is proposed, on the basis of Raman spectroscopy, that in the mineral hannebachite, the sulfite anion bonds to Ca through the sulfur atom. The Raman spectrum of the mineral orschallite Ca3[SO4](SO3)2·12H2O is complex resulting from the overlap of sulfate and sulfite bands. Raman bands at 1005 cm−1, 1096 and 1215 cm−1 are assigned to the (SO4)2−ν1 symmetric and ν3 asymmetric stretching modes. The two Raman bands at 971 and 984 cm−1 are attributed to the (SO3)2−ν3(E) and ν1(A1) stretching vibrations. The formation of sulfite compounds in nature offers a potential mechanism for the removal of sulfates and sulfites from soils. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

11.
Raman spectroscopy, complemented with infrared spectroscopy, was used to study the uranyl carbonate mineral voglite. The mineral has the formula Ca2Cu2+ [(UO2)(CO3)3](CO3)6H2O, and bands attributed to these vibrating units are readily identified in the Raman spectrum. Symmetric stretching modes at 836 and 1094 cm−1 are assigned to ν1(UO2)2+ and ν1(CO3)2− units, respectively. The ν3 antisymmetric stretching modes of (UO2)2+ are not observed in the Raman spectrum but may be readily observed in the infrared spectrum at 898 cm−1. The ν3 antisymmetric stretching mode of (CO3)2− is observed in the Raman spectrum at 1369 cm−1 as a low intensity band as is also the ν3(CO3)2− infrared modes at 1362, 1425, 1509 and 1566 cm−1. No ν2(CO3)2− Raman bending modes are observed for voglite. The Raman band at 749 cm−1 and the two infrared bands at 747 and 709 cm−1 are assigned to the ν4(CO3)2− bending modes. U O bond and O H…O bond lengths in the structure of voglite were inferred from the infrared and Raman spectra. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

12.
The Fourier transform infrared spectrum of H3SiI has been recorded in the ν14region from 2075 to 2315 cm−1at an optical resolution of 2.3 × 10−3cm−1. The ν14fundamental bands and the (ν1+ ν3) − ν3/(ν4+ ν3) − ν3hot bands have been rotationally investigated. Numerous local perturbations have been observed in the ν1and ν4bands and in the hot bands. Without the lines involved in perturbations, more than 2900 transitions of the ν14bands were used to determine the band origins and the vibration–rotation parameters of the ν1= 1 and νv4= 1 states. A least-squares fit of 766 apparently unperturbed transitions of the hot bands gave the parameters of the ν1= ν3= 1 and ν4= ν3= 1 states. Thel(2, 2) resonance in ν4and theA1–E Coriolis coupling between ν1and ν4have been investigated. Most of the local perturbations have been studied individually using a simple model by which the main perturber for each resonance was identified.  相似文献   

13.
In pursuing the systematic study of ozone high-resolution infrared spectra, we present here the analysis of line positions of the 16O18O16O isotopomer. The recorded spectra cover the range 900-5000 cm−1, that has allowed 13 bands to be observed: ν1, ν3, 2ν2, ν23, ν12, ν13, ν123, 3ν3, 2ν13, ν2+3ν3, ν1+3ν3, ν12+3ν3, and 5ν3. The analysis of these bands has been performed using effective rovibrational Hamiltonians for 10 polyads of interacting upper vibrational states. To correctly reproduce all observed transitions, it has been necessary to account for resonance perturbations due to “dark” states: (002), (200), (012), (210), (102), (310), (004), (014), (320), (104), and (311). We present the results for spectroscopic parameters (vibrational energy levels, rotational and centrifugal distortion constants, and resonance coupling parameters), as well as the statistics for rovibrational energy levels, range of observed transitions, and typical example of wavefunction mixing coefficients. A comparison of observed band centers with those predicted from an isotopically invariant potential function is discussed. The R.M.S. deviation between predicted and directly observed band centers is ≈0.2 cm−1 up to 2800 cm−1 and ≈0.5 cm−1 for all 13 bands up to 4800 cm−1.  相似文献   

14.
15.
Experimental line intensities of 1727 transitions arising from nine hot bands in the pentad–dyad system of methane are fitted to first and second order using the effective dipole moment expansion in the polyad scheme. The observed bands are ν3− ν2, ν3− ν4, ν1− ν2, ν1− ν4, 2ν4− ν4, ν2+ ν4− ν2, ν2+ ν4− ν4, 2ν2− ν2, and 2ν2− ν4, and the intensities are obtained from long-path spectra recorded with the Fourier transform spectrometer located at Kitt Peak National Observatory. For the second order model, some of the 27 intensity parameters are not linearly independent, and so two methods (extrapolation and effective parameters) are proposed to model the intensities of the hot bands. In order to obtain stable values for three of these parameters, 1206 dyad (ν4, ν2) intensities are refitted simultaneously with the hot band lines. The simultaneous fits to first and second order lead to rms values respectively of 21.5% and 5.0% for the 1727 hot band lines and 6.5% and 3.0% for the 1206 dyad lines. The band intensities of all 10 pentad–dyad hot bands are predicted in units of cm−2atm−1at 296 K to range from 0.931 (for 2ν4− ν4) to 7.67 × 10−5(for 2ν4− ν2). The total intensities are also estimated to first order for two other hot band systems (octad–pentad and tetradecad–octad) that give rise to weak transitions between 5 and 10 μm.  相似文献   

16.
ABSTRACT

The Fourier transform infrared (FTIR) spectrum of vinyl fluoride, H2C=CHF, has been widely investigated in the region of the ν47 combination band around 2800 cm?1 at a resolution of 0.005 cm?1. This vibration of A' symmetry gives rise to an a/b-hybrid band with a predominant a-type component. The rovibrational structure is strongly perturbed and the analysis has been rather complicated since this combination band is involved at least in a seven-level interacting polyad, including the ν8+2ν10, 2ν810, 2ν79, ν7812, ν5910 and ν71012 vibrational states. The study has been further complicated by the absence of transitions coming from the perturbers that were considered as dark states. The spectral analysis resulted in the identification of 936 transitions with J" ≤ 46 and Ka" ≤ 11, all belonging to the a-type component. Most of the assigned data have been fitted using the Watson's A-reduction Hamiltonian in the Ir representation and proper Coriolis perturbation operators. The model employed includes seven different resonances within a complex polyad resonant system and a set of spectroscopic constants for the ν47 combination band, for the dark states, and Coriolis coupling coefficients have been determined.  相似文献   

17.
As part of the simultaneous analysis of line positions and intensities of the first two polyads of monodeuterated methane, the results achieved for the region 3-5 μm are reported. It involves the three highest fundamentals, (ν1, ν2, ν4), overlapped by overtone (2ν3, 2ν5, 2ν6) and combination (ν36, ν35, ν56) bands. The theoretical model was based on the global tensorial model implemented in the MIRS package. Some 10 000 line positions and 2400 line intensities have been modeled to ±0.000 88 cm−1 and ±3.6% respectively, using measurements obtained at 0.0056 and 0.011 cm−1 resolution with the Fourier transform spectrometer at National Solar Observatory located at Kitt Peak. The strongest band in this polyad is ν4(E) at 3016.7 cm−1 with a strength of 6.3×10−18 cm−1/(molecule cm−2) at 296 K; the weakest band is 2ν3(E) at 2597.7 cm−1 with a strength of 1.9×10−20 cm−1/(molecule cm−2) at 296 K. The total calculated absorption arising from the CH3D nonad is 8.95×10−18 cm−1/(molecule cm−2) at 296 K.  相似文献   

18.
The Q branch of the 2ν2 ← ν2 band of 13C2D2 has been recorded with an instrumental resolution of about 0.003 cm?1 using inverse Raman spectroscopy combined with stimulated Raman pumping in order to populate the ν2=1 state. A weak local perturbation evident in the spectrum has been attributed to the effect of an anharmonic resonance between the ν2=2 and ν345=1 Σ+ g, states. To study this interaction, the components of the latter vibrational manifold (Σ+ g, ? g and Δg), together with all the bending states up to (ν4 + ν5)=2 associated with ν3=1, have been characterized through the analysis of their infrared spectra. Both cold and hot bands from states thermally populated at room temperature, ν4, ν5, 2ν4, 2ν5 and ν4 + ν5, have been recorded in the region between 2300 and 3000 cm?1 at an effective resolution of about 0.009 cm?1. A simultaneous analysis of all the assigned transitions has been performed on the basis of a theoretical model which takes into account the rotational and vibrational ?-type resonances within each vibrational manifold, the Darling-Dennison anharmonic resonance between the ν3 + 2ν4 and ν3 + 2ν5 states, and the anharmonic interaction between the 2ν2 and ν3 + ν4 + ν5 states.  相似文献   

19.
Raman spectroscopy has been used to characterise four natural halotrichites: halotrichite FeSO4.Al2(SO4)3. 22H2O, apjohnite MnSO4.Al2(SO4)3.22H2O, pickingerite MgSO4.Al2(SO4)3.22H2O and wupatkiite CoSO4.Al2(SO4)3.22H2O. A comparison of the Raman spectra is made with the spectra of the equivalent synthetic pseudo‐alums. Energy dispersive X‐ray analysis (EDX) was used to determine the exact composition of the minerals. The Raman spectrum of apjohnite and halotrichite display intense symmetric bands at ∼985 cm−1 assigned to the ν1(SO4)2− symmetric stretching mode. For pickingerite and wupatkiite, an intense band at ∼995 cm−1 is observed. A second band is observed for these minerals at 976 cm−1 attributed to a water librational mode The series of bands for apjohnite at 1104, 1078 and 1054 cm−1, for halotrichite at 1106, 1072 and 1049 cm−1, for pickingerite at 1106, 1070 and 1049 cm−1 and for wupatkiite at 1106, 1075 and 1049 cm−1 are attributed to the ν3(SO4)2− antisymmetric stretching modes of ν3(Bg) SO4. Raman bands at around 474, 460 and 423 cm−1 are attributed to the ν2(Ag) SO4 mode. The band at 618 cm−1 is assigned to the ν4(Bg) SO4 mode. The splitting of the ν2, ν3 and ν4 modes is attributed to the reduction of symmetry of the SO4 and it is proposed that the sulphate coordinates to water in the hydrated aluminium in bidentate chelation. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

20.
The IR absorption spectra of solutions of SF6 in liquid argon are studied at a temperature of 93 K in the concentration interval 10?5–10?7 mole fractions. A sample with a natural abundance of isotopes and a monoisotope 34SF6 sample are studied. The frequencies, half-widths, and relative intensities of bands in the vibrational spectrum of all isotopomers of the molecule are determined. For the 34SF6 molecule, the ratio of integral absorption coefficients of fundamental bands A4)/A3)=0.07(6) is larger than 32SF6:A4)/A3)=0.66(4) for the 32SF6 molecule, which corresponds to the same signs of P3 and P4. The change in the intensity of the ν26 and ν56 bands upon isotopic substitution is explained by the change in the resonance contributions of due to the isotope shift of the ν3 band.  相似文献   

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