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Infrared transitions

Figure C3.3.3. A schematic drawing of tlie Doppler-lineshape profile for a typical infrared transition in a small... Figure C3.3.3. A schematic drawing of tlie Doppler-lineshape profile for a typical infrared transition in a small...
Analogous to Equation (6.47) for an allowed infrared transition is the requirement... [Pg.172]

The Hj ion, recently detected in the interstellar medium via infrared transitions,25 can subsequently react with a variety of neutral atoms present in the gas. The reaction with oxygen leads to a chain of reactions that rapidly produce the hy-dronium ion H30+ via well-studied H atom-transfer reactions ... [Pg.7]

The theoretical studies usually obtained the infrared transition probabilities from the diagonalization of a total Hamiltonian which did not account for relaxational mechanisms. The theoretical spectra are then composed of Dirac delta peaks that are not fully suitable for comparison with experimental spectra. [Pg.247]

Focusing on the 0 ) > 1 ) infrared transition of the fast mode, the dipole... [Pg.265]

Owing to the above remarks, it is clear that the spectral densities resulting from the dynamical study of the two-level system, involving relaxational mechanisms, should not be viewed as the simple broadening of the infrared transitions obtained in the undamped frame. [Pg.283]

Another illustration is Fig. 13, where one can observe the complex modifications of the band structure, owing to the numerous infrared transitions enhanced by a higher temperature T = 300 K. [Pg.283]

Two ingredients are needed to compute the intensities of transitions the wave functions of the initial and final states and the form of the transition operator (Ogilvie and Tipping, 1983). For infrared transitions the appropriate operator is the dipole operator, M(r, 0, (j>). This operator is a vector (tensor of rank 1) and thus can be written as... [Pg.11]

Intensities of transition can be also analyzed by means of fitting formulas. An expansion quite often used for infrared transitions is the Herman-Wallis (1955) form... [Pg.19]

As in the previous case of infrared transitions, one wants to calculate the line strengths S(v,J —> v, J ) defined in Eq. (2.127). For Raman transitions there are two contributions, as discussed in Chapter 1. The so-called trace scattering is induced by the monopole operator... [Pg.54]

In order to find the coefficients a, for infrared transitions (for which the operator is a dipole operator), one returns to the geometric structure of the molecule and introduces a set of Cartesian coordinates (in the plane x, y), shown in Figure 4.4. The operator f has two components, fx and Ty, given by... [Pg.81]

The important point is that the Lamb-dip widths for most visible and near infrared transitions at low pressures are several orders of magnitude smaller than the doppler widths and are therefore well suited for high resolution spectroscopy. When probing with a... [Pg.66]

Different types of chemical reactions involve different types of vibrational modes, e.g. dissociation reactions may be controlled by stretching vibrations, isomerizations by skeletal modes, and so on. The argument that infrared quanta are relatively energy-poor and infrared transitions generally have low absorption cross sections, especially if multiphoton excitation is required, limits the choice of suitable molecular transitions. With respect to these constraints the type of reaction chosen and described below was dissociation, involving molecules with maximal transition dipole moments, comparatively weak bonds to be broken, and vibrational excitation in the mid-infrared spectral range. [Pg.103]

The factor in (6.67) that multiplies the integral (6.73) contains the derivatives of the dipole-moment components with respect to the normal coordinate Qk, evaluated at the equilibrium configuration. We conclude that a radiative infrared transition in which the vibrational quantum number of the A th normal mode changes by one is forbidden unless the Acth mode has a change in dipole moment associated with it. The value of the equilibrium dipole moment de is irrelevant for infrared transitions of a polyatomic molecule. [Pg.134]

Actually, many other infrared transitions occur besides those allowed by the selection rule (6.74). The neglected terms in the expansion (6.66) will give transitions with a change of 2 or more in a given vibrational quantum number and transitions in which more than one vibrational quantum number changes moreover, anharmonicity corrections to the vibrational wave function will add to the probability of such transitions. Generally, the transitions (6.74) are the strongest. [Pg.384]

In any low angular momentum state the radiative decay rate is usually dominated by the high frequency transitions to low lying states, and as a result it is impossible to control completely the decay rate using a millimeter wave cavity. In a circular i = m = n - 1 state the only decay is the far infrared transition to the n — 1 level, and Hulet et al. have observed the suppression of the decay of this level.26 They produced a beam of Cs atoms in the circular n = 22, = m = 21 state by pulsed laser excitation and an adiabatic rapid passage technique.27 The beam of circular state atoms then passed between a pair of plates 6.4 cm wide, 12.7 cm long, spaced by 230.1 jum, and held at 6 K. The 0 K radiative lifetime is 460ps, and... [Pg.63]

Hydrides of the fullerene C60 have also been investigated as potential DIB carriers (Webster 1992, 1993b). No specific identification has been suggested but it should be noted that the conjugated systems of -electrons are predicted to have transitions in the visible range. The predicted optical and near-infrared transitions of fullerene based molecules may offer a potential explanation for the long-standing problem of the diffuse interstellar bands and other interstellar and circumstellar features. [Pg.15]

FIGURE 1 Near-infrared transition metal PL in GaN samples grown (a) on p-SiC substrate by the sublimation sandwich technique, and (b) on sapphire substrate bv HVPE. [Pg.323]

The infrared transitions obey the following selection rules Ap — 1, and A./ = 1 or 0. The wave functions for the initial and final states obtained by solving the Schrodinger equation with the Hamiltonian of Eq. (1-261) or (1-265) can be used to compute the infrared absorption intensities for the complex. The infrared absorption coefficient J(J" ->./ ) for the transition J" J is proportional to,... [Pg.91]


See other pages where Infrared transitions is mentioned: [Pg.2439]    [Pg.2447]    [Pg.3000]    [Pg.515]    [Pg.515]    [Pg.204]    [Pg.232]    [Pg.41]    [Pg.48]    [Pg.49]    [Pg.145]    [Pg.145]    [Pg.252]    [Pg.111]    [Pg.162]    [Pg.134]    [Pg.309]    [Pg.353]    [Pg.217]    [Pg.224]    [Pg.533]    [Pg.533]    [Pg.533]    [Pg.217]    [Pg.236]    [Pg.675]    [Pg.88]    [Pg.90]   
See also in sourсe #XX -- [ Pg.11 , Pg.81 , Pg.145 ]




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Infrared active transition

Infrared intensities transition moments

Infrared rotational transitions

Infrared spectra of transition-metal

Infrared spectroscopy transition temperatures

Infrared transition dipole

Stretching vibrations infrared transitions

Symmetry infrared transitions

Transition metal clusters infrared spectra

Transition metal complexes infrared spectra

Transition metal complexes infrared spectroscopy

Transition metal hydrides infrared studies

Transition metal ions infrared emissions

Transition metals infrared spectroscopy

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