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Spectral Transitions

NMR arises from transitions between energy levels, just as in other branches of spectroscopy, with transitions induced by the absorption of energy from an applied electromagnetic field with a magnetic amplitude of 2B,.The interaction [Pg.18]

From the well-established results of time-dependent perturbation theory, we find that the probability of transition per unit time between levels m and m is [Pg.18]

is the magnitude of the radio frequency field applied in the x direction, with B0 in the z direction (m lx m ) is the quantum mechanical matrix element of the [Pg.18]


Atomic spectra are much simpler than the corresponding molecular spectra, because there are no vibrational and rotational states. Moreover, spectral transitions in absorption or emission are not possible between all the numerous energy levels of an atom, but only according to selection rules. As a result, emission spectra are rather simple, with up to a few hundred lines. For example, absorption and emission spectra for sodium consist of some 40 peaks for elements with several outer electrons, absorption spectra may be much more complex and consist of hundreds of peaks. [Pg.605]

Figure 6.2. (I) Conventional phosphorescence spectrum of 2,3-dichloroquinoxa-line in durene at 1.6°K. (II) am-PMDR spectrum, obtained by amplitude modulation of microwave radiation that pumps the tv-t, (1.055 GHz) zf transition with the detection at the modulation frequency. Only bands whose intensities change upon microwave radiation (1.055 GHz) and thus originate from tv or rz appear in the am-PMDR spectrum. Transitions from r and rv appear with opposite sign (phase-shifted by 180°). (Hb, lie ) Polarization of the am-PMDR spectral transitions, relative to the crystal axes. The band at 0,0-490 cm-1 originates from both the r and t spin states its intensity does not change upon the 1.055-GHz saturation (no band in II) however, its polarization does rhanp. (bands in Hb and IIc ). (Reproduced with permission from M. A. El-Sayed.tt7W)... Figure 6.2. (I) Conventional phosphorescence spectrum of 2,3-dichloroquinoxa-line in durene at 1.6°K. (II) am-PMDR spectrum, obtained by amplitude modulation of microwave radiation that pumps the tv-t, (1.055 GHz) zf transition with the detection at the modulation frequency. Only bands whose intensities change upon microwave radiation (1.055 GHz) and thus originate from tv or rz appear in the am-PMDR spectrum. Transitions from r and rv appear with opposite sign (phase-shifted by 180°). (Hb, lie ) Polarization of the am-PMDR spectral transitions, relative to the crystal axes. The band at 0,0-490 cm-1 originates from both the r and t spin states its intensity does not change upon the 1.055-GHz saturation (no band in II) however, its polarization does rhanp. (bands in Hb and IIc ). (Reproduced with permission from M. A. El-Sayed.tt7W)...
Abstract. We discuss new observations of 3He towards planetary nebulae (PNe) using the Very Large Array (VLA), the 305 m Arecibo telescope, which is now capable of observing the 3He+ spectral transition, and the recently commissioned 100 m Green Bank Telescope (GBT). [Pg.37]

For metal ions having d2, d3, d7, and d8 configurations, the ground state is an F state, but there is an excited P state that has the same multiplicity. For d1 and d7 ions in an octahedral field, the spectroscopic states are the same (except for the multiplicity) as they are for d3 and d8 ions in tetrahedral fields. Therefore, the expected spectral transitions will also be the same for the two types of complexes. The three spectral bands are assigned as follows (Tlg(F) means the Tis state arising from the F spectroscopic state) ... [Pg.654]

The corresponding energies for the spectral transitions that occur for d3 and d8 ions in octahedral fields (or d2 and d7 ions in tetrahedral fields) are as follows ... [Pg.654]

The fact that quantum observables are represented by matrices immediately suggests problems of non-commutation. For instance, the observables can be measured at the same time only if they have a complete orthogonal set of eigenvectors in common. This happens only when they commute, i.e. XY = YX, or the commutator [X, Y] = XY — YX = 0. This is a central feature of the matrix formulation of quantum theory discovered by Heisenberg, Born and Jordan while trying to explain the observed spectral transitions of the hydrogen atom in a more fundamental way than the quantization... [Pg.189]

Figure 27. Polymer effect on isothermal spectral transition induced by moisture treatment of polyion complex films, (relative humidity = 62%)... Figure 27. Polymer effect on isothermal spectral transition induced by moisture treatment of polyion complex films, (relative humidity = 62%)...
An example of an application to actual spectroscopy is shown in Figure 6.9. This shows the states computed in the range of the 0 —> 3 CH spectral transition. The intensities were computed as a Franck-Condon overlap of the optically bright CH overtone state (Holme and Levine, 1989 Levine and Berry, 1989) with the relevant eigenstate. [Pg.155]

Dispersion interactions have been shown in the absence of other effects to be responsible for gas-to-liquid changes of chemical shifts 1>2). The dispersion contribution to the electric field effect on infrared and ultraviolet spectral transitions has been shown to be proportional to McRae term 10 n)... [Pg.126]

Bearing in mind that the primary ohjective of spectral analysis in its two stages combined is to evaluate parameters of minimal number that serve to reproduce archetypal characteristics of spectral lines in related sets, we consider how to apply formulae presented above for analysis of data of type wave number or frequency of spectral transitions. On a purely empirical basis for spectra of each separate isotopic species, one might simply apply formulae 2 and 3 in combination,... [Pg.269]

The application of resonance Raman spectroscopy to the study of metalloprotelns has led to the Identification of metal-llgated groups based on the appearance of characteristic metal-llgand and Intrallgand vibrational modes. Electronic spectral transitions due... [Pg.63]

The scope of the quantum chemistry is manifold. It provides numerical solutions obtained by the use of equations of the quantum mechanical theory. It enables to calculate bond and dissociation energies, characteristics of spectral transitions, force constants, electron and spin densities, polarizabilities. The properties referring to atoms, molecules and other systems can be theoretically determined without knowledge of empirical data of these systems (ab initio level). [Pg.41]

The term symbol summarizes the properties of any state and also permits a concise representation of spectral transitions. It consists of an upper case letter (S, P, D. ..) to represent the net orbital angular momentum (L) and a number written as a superscript on the upper left to indicate spin multiplicity (i. e. the number of possible orientations of total spin of the atom). L is zero for Fe " (no angular momentum) and 2 for Fe ". The spin multiplicity is defined as (2S -i- 1) S = 5/2 and 2 for Fe " and Fe ", respectively. The ground state term symbol for Fe " is, therefore, 85 2 and for Fe " it is 04. The subscript on the right is the value J. [Pg.112]

The most extensive and systematic study of the chemistry of lignin with theoretical methods has been performed by Remko and co-workers. Their work has involved the nature of intramolecular (40-43) and inter-molecular (44-48) hydrogen bonding of lignin model compounds, spectral transitions (49-52), and conformational analysis (53). The methods used have included CNDO/2 and PCILO (Perturbative Configuration Interaction using Localized Orbitals) (54). [Pg.273]

Less symmetric molecules require a considerably more complicated treatment, but in the end their spectral transitions arc functions of their three moments of inertia (see Section 10.3.5). From a computational standpoint, then, prediction of rotational spectral lines depends only on the moments of inertia, and hence only on the molecular geometry. Thus, any method which provides good geometries will permit an accurate prediction of rotational spectra within the regime where tlie rigid-rotor approximation is valid. [Pg.334]

In the future, analysis of this problem at the SCRF level will necessarily have to focus on molecular properties other than the solvation free energy to assess the greater accuracy of one cavity compared to another. Thus, differences in the gas-phase and solvated wave functions, and their corresponding effects on such properties as NMR, IR, and UV spectral transitions, may prove useful in identifying optimal methods for handling the electrostatics. [Pg.411]

Both the semiquantitative and quantitative types of calculation yield energy-level schemes from which, in principle, spectral transition energies may be calculated. Comparison of these schemes with observed electronic spectra should enable an assessment of their relative values to be made however, the spectral data on organometallic molecules are very limited and often qualitative. There are few accurate studies involving polarization data and solvent shifts from which the nature of the observed bands can be classified and since, in most cases, the theoretical schemes of bond levels yield an embarrassing number of transitions, this lack of assignment is serious. [Pg.22]


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Balhausen, C. J., Intensities of Spectral Bands in Transition Metal Complexes

Electronic transition dipole moment spectral overlap

Electronic transitions, forbidden spectral strength

Optical spectral transitions

Solvated electron spectral transitions

Spectral lines transition probability

Spectral properties of transition-metal

Spectral properties of transition-metal complexes

Spectral transition assignments

Spectral transitions, intermediate coupling

Transitions spectral shifts

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