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Angular momentum integral operator

This term describes a shift in energy by Acim rn, for an orbital with quantum numbers I — 2, mi and that is proportional to the average orbital angular momentum (/z) for the TOj-spin subsystem and the so-called Racah parameters Bm, that in turn can be represented by the Coulomb integrals and The operator that corresponds to this energy shift is given by... [Pg.458]

Without essential limitation of generality it may be assumed that the orientation of the molecule and its angular momentum are changed by collision independently, therefore F(JU Ji+, gt) = f (Jt, Ji+i)ip(gi). At the same time the functions /(/ , Ji+ ) and xp(gi) have common variables. There are two reasons for this. First, it may be due to the fact that the angle between / and u must be conserved for linear rotators for any transformation. Second, a transformation T includes rotation of the reference system by an angle sufficient to combine axis z with vector /. After substitution of (A7.16) and (A7.14) into (A7.13), one has to integrate over those variables from the set g , which are not common with the arguments of the function / (/ , /j+i). As a result, in the MF operator T becomes the same for all i and depends on the moments of tp as parameters. [Pg.270]

The orbital angular momentum operations needed to calculate integrals for other orbitals are summarized in Table 4.2. [Pg.59]

Schrodinger s equation has solutions characterized by three quantum numbers only, whereas electron spin appears naturally as a solution of Dirac s relativistic equation. As a consequence it is often stated that spin is a relativistic effect. However, the fact that half-integral angular momentum states, predicted by the ladder-operator method, are compatible with non-relativistic systems, refutes this conclusion. The non-appearance of electron... [Pg.237]

The long but straightforward integration[65] produces the expression for the angular momentum in terms of a new vector operator, s, in the form... [Pg.254]

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]

It was shown in Section 1.7 that when the operators Px, PY, Pz °t>ey general angular-momentum commutation relations, as in (5.41), then the eigenvalues of P2 and Pz are J(J+ )h2 and Mh, respectively, where M ranges from — J to J, and J is integral or half-integral. However, we exclude the half-integral values of the rotational quantum number, since these occur only when spin is involved. [Pg.109]

The SH Hs acts only on the spin kets S,Ms) yielding eigenvalues that are identical with those produced by the perturbation operator H acting on the full set of spin-orbit variables a,L,Mi,S,M ). This situation is explained in Table 1 the truncated SH matrix involves integrals over the angular momentum via the perturbation theory. [Pg.7]

Symmetry dictates that the representations of the direct product of the factors in the integral (3 /T Hso 1 l/s2) transform under the group operations according to the totally symmetric representation, Aj. The spin part of the Hso spin-orbit operator converts triplet spin to singlet spin wavefunctions and singlet functions to triplet wavefunctions. As such, the spin function does not have a bearing on the symmetry properties of Hso- Rather, the control is embedded in the orbital part. The components of the orbital angular momentum, (Lx, Ly, and Lz) of Hso have symmetry properties of rotations about the x, y, and z symmetry axes, Rx, Ry, and Rz. Thus, from Table 2.1, the possible symmetry... [Pg.48]

The frozen-core (fc) approach is not restricted to spin-independent electronic interactions the spin-orbit (SO) interaction between core and valence electrons can be expressed by a sum of Coulomb- and exchange-type operators. The matrix element formulas can be derived in a similar way as the Sla-ter-Condon rules.27 Here, it is not important whether the Breit-Pauli spin-orbit operators or their no-pair analogs are employed as these are structurally equivalent. Differences with respect to the Slater-Condon rules occur due to the symmetry properties of the angular momentum operators and because of the presence of the spin-other-orbit interaction. It is easily shown by partial integration that the linear momentum operator p is antisymmetric with respect to orbital exchange, and the same applies to t = r x p. Therefore, spin-orbit... [Pg.129]

Given a molecule that possesses C2p symmetry, let us try to figure out how to calculate ( Ai ffsol Bi) from wave functions with Ms = 1. The coupling of an Ai and a B state requires a spatial angular momentum operator of B2 symmetry. From Table 11, we read that this is just the x component of It. A direct computation of (3A2, Ms = 1 t x spin-orbit Hamiltonian with x symmetry and So correspondingly for the zero-component of the spin tensor. This is the only nonzero matrix element for the given wave functions. [Pg.151]

We recall from section 5.2.4 that, from the general theory of angular momentum, j can take half-integral (more strictly half-odd) values as well as integral ones. The particular case of j = 1 /2 deserves special mention because of its importance in the discussion of electron or proton spin. For j = 1/2, there are two possible states l/2, 1/2) and 11/2, -1/2) which are often denoted a) and /3) respectively. The spin operators which define these states are particularly simple. For example,... [Pg.150]

The simplest example of the Wigner—Eckart theorem is given by the Gaunt integral over three spherical harmonics, which is the matrix element for the transition between eigenstates m) and fm ) of a single orbital angular momentum observable due to a tensor operator Tj. We prefer to use the renormalised tensor operator C, which simplifies the expression. [Pg.69]


See other pages where Angular momentum integral operator is mentioned: [Pg.280]    [Pg.142]    [Pg.441]    [Pg.161]    [Pg.59]    [Pg.284]    [Pg.388]    [Pg.212]    [Pg.153]    [Pg.106]    [Pg.14]    [Pg.213]    [Pg.145]    [Pg.82]    [Pg.506]    [Pg.31]    [Pg.3]    [Pg.314]    [Pg.111]    [Pg.119]    [Pg.84]    [Pg.85]    [Pg.90]    [Pg.155]    [Pg.218]    [Pg.26]    [Pg.31]    [Pg.15]    [Pg.145]    [Pg.142]    [Pg.284]    [Pg.76]    [Pg.331]   
See also in sourсe #XX -- [ Pg.586 ]




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