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Bands band vibration

Band assignment Vibration frequency [cm- ] Tunneling splitting [cm ] ... [Pg.96]

The UV-visible spectra of Ni and Nia have also been identified in argon matrices (93) Ni absorbed at 377, 529, and 4l0 nm, with vi-bronic structure on the first two bands, and with spacing of—330 cm , and Nis absorbed at 420 and 480 nm, the latter band showing vibrational spacing of -200 cm" . Higher-nuclearity clusters were observed, but not characterized. After prolonged warm-up of these matrices, nickel colloid was formed (93). [Pg.91]

Anti-Stokes picosecond TR spectra were also obtained with pump-probe time delays over the 0 to 10 ps range and selected spectra are shown in Figure 3.33. The anti-Stokes Raman spectrum at Ops indicates that hot, unrelaxed, species are produced. The approximately 1521 cm ethylenic stretch Raman band vibrational frequency also suggests that most of the Ops anti-Stokes TR spectrum is mostly due to the J intermediate. The 1521 cm Raman band s intensity and its bandwidth decrease with a decay time of about 2.5 ps, and this can be attributed the vibrational cooling and conformational relaxation of the chromophore as the J intermediate relaxes to produce the K intermediate.This very fast relaxation of the initially hot J intermediate is believed to be due to strong coupling between the chromophore the protein bath that can enable better energy transfer compared to typical solute-solvent interactions. ... [Pg.170]

A 9 cm-1 upshift of the tangential mode (G band) vibrational frequency as well as a 90% decrease in intensity was observed by applying 1.0 V between an individual nanotube and a silver reference electrode in a dilute sulfuric acid solution. [Pg.507]

It is usually easier, mathematically, not to think in terms of wavelength X (which is inversely proportional to energy) but to employ variables that are directly proportional to energy. Most spectroscopists use co, which is the frequency of the vibration normalized to the speed of light c, so co = v + c, where v is the frequency. In the context of infrared spectroscopy, we usually call co the wavenumber of the band vibration. [Pg.465]

Optical spectroscopy has merits in identifying radical cations, particularly when their spectra are known independently. For example, the radiolysis of quadricyclane led to the observation of the known spectrum of norbornadiene radical cation. In another study, irradiation of cyclooctatetraene radical cation caused the color of the sample to change from bright red to royal blue, suggesting the conversion to a different species, the previously identified semibullvalene radical cation. Further irradiation of the latter led to a characteristic banded (vibrationally resolved) spectrum the nature of this spectrum suggested that the rearranged species may be a linear conjugated radical cation and helped in its identification as 1,4-dihydropen-talene radical cation. ... [Pg.269]

Despite the fact that a full assignment of all the observed absorptions to the respective macromolecule s natural frequencies is not possible in all cases - in particular for complex co- and terpolymers, stereoregular polymers, crosslinked systems, composites, compounds or blends this is very difficult - there are many bands caused by local group vibrations of a few atoms which can be interpreted very nicely. As an example, the C=0 band (stretching vibration) is usually observed as an intense absorption between v = 1850-1650 cm. Because of the coupling with other vibrations of the molecule its frequency is characteristic for the constitution and the neighborhood of the observed atom group. [Pg.82]

As was mentioned previously, the first absorption band (I) of 4a,4b-dihydrophen-anthrene is usually structureless and rather broad, having a half height width (AXiy2) of 4700 cm in 1. This band shows vibrational structure (developed to various extents) only in 12,13,15, 37, 38, 40, 43-46, and in 49—53 (see Table 13). The observed vibrational spacings, usually 1200—1400 cm correspond very probably to an excited state-totally symmetric stretching mode (i/j) of the C—C double bonds such as... [Pg.59]

Les spectres sont enregistres par im spectrographe Perkin-Elmer equipe d une optique en fluorure de lithium. Le spectrographe est rempli d air deshy drate afin d eviter les perturbations de lecture par les bandes de vibration-rotation de l eau atmospherique. Notons que la precision relative des lectures est de Fordre du cm 1 pour les bandes OH libre et de Fordre d une dizaine pour les bandes OH associees a cause de la plus grande largeur de ees dernieres bandes. [Pg.164]

Table 4.13. Analytical form (Eqs. 4.39 and 4.40) of the dipole matrix elements for the H2-H2 first overtone band, single vibrational transitions [284]. Table 4.13. Analytical form (Eqs. 4.39 and 4.40) of the dipole matrix elements for the H2-H2 first overtone band, single vibrational transitions [284].
Assign these bands to vibrational transitions use the notation of Problem 6.29. (The lowest and highest frequency fundamentals are v2 and vy respectively.)... [Pg.152]

In molecular spectra, perturbations cause Uie displacement of a band from its regular position in the band system (vibrational perturbation) or the displacement (and/or weakening) of corresponding lines in the different branches of a band (rotational perturbation). A perturbation observed in the spectrum is indicative of the presence of a perturbation (shift) of one of the energy levels involved due to interaction with another level of the same, or nearly the same, energy. [Pg.1240]

It is not so simple that certain ions show no structure in their spectra, whereas other do. The nature of the host lattice plays also an important role. This is illustrated in an impressive way by the Bi3 + (6s2) ion. Depending on the host lattice its spectra may show narrow bands with vibrational structure or very broad and structureless bands, and the Stokes shift of the emission may vary from 1000 to 20000 cm-1 [2]. [Pg.3]

Compositions CsMgj xNixCl3 show Ni2+ emission at about 5000 cm-1 [40]. The emission band shows vibrational structure yielding an S value of about 2.5. From this value Qo—QZ is found to be 0.7 A, which gives dr=0.24 A for the change in the Ni-Cl distance. This emission is due to a transition from one of the crystal-field components of the first excited state 3nt ground state (3d8, Oh notation). The lifetime of the excited state is 5.2 ms. The luminescence is quenched above 200 K. [Pg.18]


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See also in sourсe #XX -- [ Pg.465 , Pg.466 ]




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Vibrational bands

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