Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Overtone spectra

As in the infrared spectrum, overtone bands with Ac > 1 are possible, but have much weaker intensity and are usually not observed.) The A/= -2, 0, and +2 branches of a vibration-rotation Raman band are called O, Q, and S branches, respectively, in an extension of the P, Q, R notation used in infrared spectra. [Pg.99]

Weak bands in the high-frequency region, resulting from the fundamental absorption of functional groups, such as S—H and C=C, are extremely valuable in the determination of structure. Such weak bands would be of little value in the more complicated regions of the spectrum. Overtones and combination tones of lower... [Pg.80]

The infrared spectra of polyatomic molecules contain one fundamental band for each normal mode whose motion modulates the dipole moment of the molecule. Normal modes that do not modulate the dipole moment of the molecule are not seen in the infrared spectrum. Overtone bands occur as with diatomic molecules, along with combination bands, which are produced when two normal modes make simultaneous transitions. [Pg.997]

Marquardt R, Sanches Gongalves N and Sala O 1995 Overtone spectrum of the CH chromophore In CHI3 J. Chem. Phys. 103 8391-403... [Pg.1091]

Figure 9.40 Cavity ring-down absorption spectrum of HCN showing the overtone/combination band. (Reproduced, with permission, from Romanini, D. and Lehmann, K. K., J. Chem. Phys., 99, 6H1, 1993)... Figure 9.40 Cavity ring-down absorption spectrum of HCN showing the overtone/combination band. (Reproduced, with permission, from Romanini, D. and Lehmann, K. K., J. Chem. Phys., 99, 6H1, 1993)...
Fig. 1. Model Spectra re-binned to CRIRES Resolution To demonstrate the potential for precise isotopic abundance determination two representative sample absorption spectra, normalized to unity, are shown. They result from a radiative transfer calculation using a hydrostatic MARCS model atmosphere for 3400 K. MARCS stands for Model Atmosphere in a Radiative Convective Scheme the methodology is described in detail e.g. in [1] and references therein. The models are calculated with a spectral bin size corresponding to a Doppler velocity of 1 They are re-binned to the nominal CRIRES resolution (3 p), which even for the slowest rotators is sufficient to resolve absorption lines. The spectral range covers ss of the CRIRES detector-array and has been centered at the band-head of a 29 Si16 O overtone transition at 4029 nm. In both spectra the band-head is clearly visible between the forest of well-separated low- and high-j transitions of the common isotope. The lower spectrum is based on the telluric ratio of the isotopes 28Si/29Si/30Si (92.23 4.67 3.10) whereas the upper spectrum, offset by 0.4 in y-direction, has been calculated for a ratio of 96.00 2.00 2.00. Fig. 1. Model Spectra re-binned to CRIRES Resolution To demonstrate the potential for precise isotopic abundance determination two representative sample absorption spectra, normalized to unity, are shown. They result from a radiative transfer calculation using a hydrostatic MARCS model atmosphere for 3400 K. MARCS stands for Model Atmosphere in a Radiative Convective Scheme the methodology is described in detail e.g. in [1] and references therein. The models are calculated with a spectral bin size corresponding to a Doppler velocity of 1 They are re-binned to the nominal CRIRES resolution (3 p), which even for the slowest rotators is sufficient to resolve absorption lines. The spectral range covers ss of the CRIRES detector-array and has been centered at the band-head of a 29 Si16 O overtone transition at 4029 nm. In both spectra the band-head is clearly visible between the forest of well-separated low- and high-j transitions of the common isotope. The lower spectrum is based on the telluric ratio of the isotopes 28Si/29Si/30Si (92.23 4.67 3.10) whereas the upper spectrum, offset by 0.4 in y-direction, has been calculated for a ratio of 96.00 2.00 2.00.
The number of fundamental vibrational modes of a molecule is equal to the number of degrees of vibrational freedom. For a nonlinear molecule of N atoms, 3N - 6 degrees of vibrational freedom exist. Hence, 3N - 6 fundamental vibrational modes. Six degrees of freedom are subtracted from a nonlinear molecule since (1) three coordinates are required to locate the molecule in space, and (2) an additional three coordinates are required to describe the orientation of the molecule based upon the three coordinates defining the position of the molecule in space. For a linear molecule, 3N - 5 fundamental vibrational modes are possible since only two degrees of rotational freedom exist. Thus, in a total vibrational analysis of a molecule by complementary IR and Raman techniques, 31V - 6 or 3N - 5 vibrational frequencies should be observed. It must be kept in mind that the fundamental modes of vibration of a molecule are described as transitions from one vibration state (energy level) to another (n = 1 in Eq. (2), Fig. 2). Sometimes, additional vibrational frequencies are detected in an IR and/or Raman spectrum. These additional absorption bands are due to forbidden transitions that occur and are described in the section on near-IR theory. Additionally, not all vibrational bands may be observed since some fundamental vibrations may be too weak to observe or give rise to overtone and/or combination bands (discussed later in the chapter). [Pg.63]

Based on empirical observation, a general statement about overtones and combination bands might be Overtones do occur, but they are very weak. Combination bands are seldom observed. Kirtley, for example, says that overtones are about a factor of 200 weaker than fundamentals in the case of the benzoate ion [47, 53]. Ramsier, Henriksen, and Gent identify a single clear overtone in the tunneling spectrum of the phosphite ion (HPO3 2) [54], The fundamental associated with... [Pg.197]

Near-infrared Spectroscopy. Near-infrared spectroscopy (NIRS) uses that part of the electromagnetic spectrum between the visible and the infrared. This region has the advantage that the instrumentation is nearest to visible instrumentation. Signals in the near-infrared come not from the fundamental vibrations of molecules but from overtones. As... [Pg.21]

Whether SnFLt is a symmetric or spherical top was discussed based on the rotational spectrum of the sixth stretching vibrational overtone, obtained by photoacoustic spectroscopy107. The IR band at vgn ]q 1844 cm-1 served to investigate the kinetics and mechanism of chemical vapour deposition of a thin tin layer, by thermolysis of trimethylstannane at 378-503 K108. [Pg.378]

Figure 8.9 Diffuse reflectance infrared spectrum of a silica support, showing silica vibrations at frequencies below 1300 cm1, overtones and combination bands between 1700 and 2050 cm-1, and various hydroxyl groups at frequencies above 3000 cm 1. The sharp peak at 3740 cm"1 is due to isolated OH groups, the band around 3550 cm 1 to paired, H-bonded OH groups, and the band around 3660 cm 1 to hydroxyls inside the silica (courtesy of R.M. van Hardeveld, Eindhoven). Figure 8.9 Diffuse reflectance infrared spectrum of a silica support, showing silica vibrations at frequencies below 1300 cm1, overtones and combination bands between 1700 and 2050 cm-1, and various hydroxyl groups at frequencies above 3000 cm 1. The sharp peak at 3740 cm"1 is due to isolated OH groups, the band around 3550 cm 1 to paired, H-bonded OH groups, and the band around 3660 cm 1 to hydroxyls inside the silica (courtesy of R.M. van Hardeveld, Eindhoven).
As mentioned above, the NIR portion of the electromagnetic spectrum is located between the visible and mid-range infrared sections, roughly 750-2500nm or 13,333-4000cm It mainly consists of overtones and... [Pg.13]

The number of peaks in an IR spectrum may increase due to overtones. Normally, the vibrational level is allowed to change by +1. If the vibrational energy level changes by 2 or more (a forbidden transition), an overtone results. It is also possible for two normal mode vibrations to combine into a third. [Pg.124]

Any unknown (isolated) band may be deduced from first principles unfortunately, there is considerable overlap in the NIR region, but this is where Chemometrics will be discussed. An idealized spectrum of combinations and overtones is seen in Fig. 6.3. [Pg.169]

The two stretching modes are called V and v3 here in order to conform with standard notation (Herzberg, 1950 v2 is the bending mode). Several other cases have been analyzed. Typical root-mean-square deviations for the lowest-order Hamiltonian of Eq. (4.28) are < 5 cm-1 up to the sixth overtone. For example, the calculation of water of Table 4.1 has a root-mean-square deviation of 4.0 cm. In addition to providing a calculation of stretching overtones, one is also able to determine, in a simple way, the nature of the spectrum. If one compares, for example, water, H20, with sulfur dioxide, S02, one observes the situation of Table 4.2. Thus S02 is much closer to the normal limit than H20. We shall... [Pg.79]

Figure 6.9 Observed opto-thermal spectrum of the Avcw = 3 overtone of benzene (points with error bars) and a stick spectrum calculated by means of the algebraic theory. Labels indicate the most important states involved in borrowing intensity from the CH overtone. Adapted from Bassi et al. (1993). Figure 6.9 Observed opto-thermal spectrum of the Avcw = 3 overtone of benzene (points with error bars) and a stick spectrum calculated by means of the algebraic theory. Labels indicate the most important states involved in borrowing intensity from the CH overtone. Adapted from Bassi et al. (1993).

See other pages where Overtone spectra is mentioned: [Pg.79]    [Pg.81]    [Pg.79]    [Pg.79]    [Pg.81]    [Pg.79]    [Pg.1136]    [Pg.381]    [Pg.131]    [Pg.257]    [Pg.18]    [Pg.452]    [Pg.122]    [Pg.69]    [Pg.1136]    [Pg.102]    [Pg.90]    [Pg.28]    [Pg.17]    [Pg.139]    [Pg.65]    [Pg.197]    [Pg.198]    [Pg.351]    [Pg.159]    [Pg.380]    [Pg.381]    [Pg.388]    [Pg.231]    [Pg.627]    [Pg.150]    [Pg.164]    [Pg.326]    [Pg.13]    [Pg.28]    [Pg.45]   
See also in sourсe #XX -- [ Pg.155 ]




SEARCH



Energy overtone spectra

Hamiltonian overtone spectra

Information from overtone spectra

Overton

Overtone

Raman spectrum, overtone

Vibrational overtone spectra

Vibrational overtone spectra interpretation

Vibrational overtone spectra references

© 2024 chempedia.info