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Transition integrals

The first term in this expansion, when substituted into the integral over the vibrational eoordinates, gives ifj(Re) , whieh has the form of the eleetronie transition dipole multiplied by the "overlap integral" between the initial and final vibrational wavefunetions. The if i(Rg) faetor was diseussed above it is the eleetronie El transition integral evaluated at the equilibrium geometry of the absorbing state. Symmetry ean often be used to determine whether this integral vanishes, as a result of whieh the El transition will be "forbidden". [Pg.411]

An example of an El forbidden but "vibronically allowed" transition is provided by the singlet n ==> ti transition of H2CO that was discussed earlier in this section. As detailed there, the ground electronic state has Ai symmetry, and the n ==> 71 state is of 1A2 symmetry, so the El transition integral... [Pg.414]

Xvf (Ra - Ra,e) Xvi> will be non-zero and probably quite substantial (because, for harmonic oscillator functions these "fundamental" transition integrals are dominant- see earlier) ... [Pg.414]

Frosch(84,133) have explained the external heavy-atom effect in intersystem crossing by postulating that the singlet and triplet states of the solute, which cannot interact directly, couple with the solvent singlet and triplet states, which themselves are strongly coupled through spin-orbit interaction. Thus the transition integral becomes<134)... [Pg.134]

The term III scattering (equation 8) is the weakest in the three scattering mechanisms, as shown by two derivative terms (M ) in the electronic transition integrals. Clearly, for a dipole forbidden transition (M° = 0) the only non-zero term is term III. The term in scattering results in binary overtone and combination transitions of vibronically active modes. It is noted that no fundamental transition survives. [Pg.153]

The relativistic version (RQDO) of the quantum defect orbital formalism has been employed to obtain the wavefunctions required to calculate the radial transition integral. The relativistic quantum defect orbitals corresponding to a state characterized by its experimental energy are the analytical solutions of the quasirelativistic second-order Dirac-like equation [8]... [Pg.265]

The relativistic quantum defect orbitals lead to closed-form analytical expressions for the transition integrals. This allows us to calculate transition probabilities and oscillator strengths by simple algebra and with little computational effort. [Pg.265]

In Eq. (14), /max is the maximum of the orbital angular momentum quantum numbers of the active electron in either the initial or final states, I nl, n l ) is the radial transition integral, that contains only the radial part of both initial and final wavefunctions of the jumping electron and a transition operator. Two different forms for this have been employed, the standard dipole-length operator, P(r) = r, and another derived from the former in such a way that it accounts explicitly for the polarization induced in the atomic core by the active electron [9],... [Pg.276]

As in the case of LS coupling, when there are N equivalent electrons in the outer shell, both the line strength and the oscillator strength should be multiplied by N as well as by the corresponding CFP [ 10,12]. As in the LS scheme the two forms of the electric dipole length transition operator have been employed here in the calculation of the radial transition integral, I nl, n l ). [Pg.277]

Theoretical calculations of the rotatory dispersion curves for molecules require knowledge of the magnetic-dipole transition integral M between two states, tpi and tpz This integral is M = -i/3 x... [Pg.135]

The transition integrals derived from the above wavefunctions are closed-form analytical expressions and, thus, their calculation is free from convergence problems. Another advantage is that the computational cost does not increase with the size ofthe atomic system. [Pg.53]

Figure 2 Systematic trends of the oscillator strengths of the 3s2 S0- 3s3p P 0 transitions in the magnesium isoelectronic sequence. RQDO (pol) are the core-polarisation-corrected RQDO f-values. Both CIV3 and GRASP f-values correspond to the length form of the transition integral... Figure 2 Systematic trends of the oscillator strengths of the 3s2 S0- 3s3p P 0 transitions in the magnesium isoelectronic sequence. RQDO (pol) are the core-polarisation-corrected RQDO f-values. Both CIV3 and GRASP f-values correspond to the length form of the transition integral...
Keywords Colloidal dispersion Flow curve Glass transition Integration through transients approach Linear viscoelasticity Mode coupling theory Nonlinear rheology Non-equilibrium stationary state Shear modulus Steady shear... [Pg.59]

Permanent dipole moments may not occur in molecules with a certain symmetry. For example, p-dichlorobenzene should not have a dipole moment, whereas m-dichlorobenzene should have a dipole moment. This plays a role in spectroscopy. The intensity of light absorption, when a system moves from the state A to the state B with wave functions and can be characterized by the transition integral... [Pg.424]

Let us consider a molecule having a fixed position in a Cartesian coordinate system. To excite the molecule, the IR light (because the separation of the vibrational levels corresponds to the infrared region) is used that is polarized along the x-axis. The electromagnetic theory says that what decides the intensity of the absorption is the square of the transition integral ... [Pg.1113]


See other pages where Transition integrals is mentioned: [Pg.326]    [Pg.633]    [Pg.194]    [Pg.33]    [Pg.135]    [Pg.343]    [Pg.144]    [Pg.52]    [Pg.59]    [Pg.234]    [Pg.151]    [Pg.209]    [Pg.343]    [Pg.204]    [Pg.204]    [Pg.186]    [Pg.283]    [Pg.46]    [Pg.170]    [Pg.787]    [Pg.135]   
See also in sourсe #XX -- [ Pg.109 , Pg.110 ]




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