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Angular moment

A+B L -fl/2) have also been used. The theoretical assumption underlying an inverse power dependence is that the basis set is saturated in the radial part (e.g. the cc-pVTZ ba.sis is complete in the s-, p-, d- and f-function spaces). This is not the case for the correlation consistent basis sets, even for the cc-pV6Z basis the errors due to insuficient numbers of s- to i-functions is comparable to that from neglect of functions with angular moment higher than i-functions. [Pg.163]

The dipole moment m depends on the total angular momentum, which may be written in terms of the orbital angular moment operator L and the total eleetron spin S. [Pg.237]

Angular moments along the main magnetic axes. [Pg.161]

Figure 6.2 Formation of the solar system (a) unstable molecular cloud possessing some angular momentum (b) angular moment conservation produces the disc shape under collapse (c) matter accretion forms the planets (d) the mature system of planets seen today evolves after 4 Myr... Figure 6.2 Formation of the solar system (a) unstable molecular cloud possessing some angular momentum (b) angular moment conservation produces the disc shape under collapse (c) matter accretion forms the planets (d) the mature system of planets seen today evolves after 4 Myr...
The mean angular moment (in units of %) is fit = dqjdv and the mean dipole-dipole energy is ED — — dq/dp. In the limit of high temperatures we may expand the exponential and retain only the linear terms, v and /9 may then be considered as the coefficients of the expansion of p in orthogonal operators, since Tr(VmMa) — 0. In this limiting case it then becomes evident that v and / are independent. It is easily shown that the thermodynamical temperature, defined by... [Pg.298]

In these expressions, e and N refer to electron and nucleus, respectively, Lg is the orbital angular moment operator, rg is the distance between the electron and nnclens. In and Sg are the corresponding spins, and reN) is the Dirac delta fnnction (eqnal to 1 at rgN = 0 and 0 otherwise). The other constants are well known in NMR. It is worth mentioning that eqs. 3.8 and 3.9 show the interaction of nnclear spins with orbital and dipole electron moments. It is important that they not reqnire the presence of electron density directly on the nuclei, in contrast to Fermi contact interaction, where it is necessary. [Pg.45]

In an earlier paper (S 044], anomalies in the angular moments of the monomer-monomer distribution function for flexible polymers are established. It is shown here how these anomalies arise from the tetrahedral symmetry of the three-state RIS model and how they disappear in the continuum limit of torsional conformations. It is concluded that the eighth and higher radial moments contain spurious contributions when calculated within the usual three-state model. [Pg.44]

Nuclear magnetic resonance (NMR) is based on a phenomenon that nuclei which possess both magnetic and angular moments (i.e. have odd mass number or odd atomic number) interact with an applied magnetic field B0 yielding 21 + 1 (where 1 is the nuclear spin quantum number) energy levels with separation AE ... [Pg.9]

These are derived frum a. lensui force resulting from a coupling between individual pairs of nucleons and from the coupling between spin and orbital angular moments of the individual nucleus, as described by the shell model of the nucleus. [Pg.1097]

Both v tit) and Aj t) depend on changes in both the direction and magnitude of the linear and angular moments. Therefore, it is important to determine which of these changes contributes the most to the overall time dependence of f(t) and Aj(t). In order to investigate this problem we have also computed the normalized linear and angular speed autocorrelation functions, c(t) and Oj(t) ... [Pg.92]

For example, the singlet-triplet transitions in ethylenic compounds generally have tmax <3C 1. The fact that spin-forbidden transitions can be observed at all shows that the transition moment, f electric dipole operator. This operator also contains small terms such as quadrupole operators and spin-orbit operators. The latter is the part of any dynamical operator which couples orbital and spin angular moments this term is responsible for the appearance of weak triplet — singlet absorption spectra. [Pg.15]

Auzinsh, M.P. (1984). On the solution of rate equations for polarization momenta in case of large angular moments, Izv. Akad. Nauk Latv. SSR Ser. Fiz. Tekh. Nauk, 1, 9-15. [Pg.267]

Jeyes, S.R., McCaffery, A.J. and Rowe, M.D. (1978). Energy and angular moment transfer in atom-diatom collisions from polarized laser fluorescence, Mol. Phys., 36, 1865-1891. [Pg.281]

Both the orbital and the effective spinning motions of the electron have associated angular moments quantized in units of ii = 1.055 x 10-34 Js. It is an elementary exercise in physics to show that the relationship between the magnetic dipole moment /< and the angular momentum L for a moving particle of mass m and charge Q is... [Pg.470]

FIG. 12.1 Precession of a nuclear angular moment in a magnetic field. [Pg.363]

Restricted to an individual bond the definition of a g function is a function cylinder symmetrical round the bond axis (angular moment zero), a tz function has a component of unity along this axis comp, s and p states with values for the subsidiary or azimuthal quantum number l equal to o and i, respectively (P. 11). [Pg.184]

In a free multielectron atom or ion, the spin and orbital angular moments of the electrons couple to give a total angular momentum represented in the Russell-Saunders scheme by the quantum number J. Since J arises from vectorial addition of L (the total orbital quantum number) and 5 (total spin quantum number), it may take integral (or half-integral... [Pg.88]


See other pages where Angular moment is mentioned: [Pg.101]    [Pg.151]    [Pg.209]    [Pg.249]    [Pg.251]    [Pg.252]    [Pg.506]    [Pg.77]    [Pg.153]    [Pg.62]    [Pg.524]    [Pg.539]    [Pg.539]    [Pg.432]    [Pg.65]    [Pg.15]    [Pg.93]    [Pg.15]    [Pg.63]    [Pg.185]    [Pg.314]    [Pg.71]    [Pg.104]    [Pg.328]    [Pg.363]    [Pg.153]    [Pg.358]    [Pg.342]    [Pg.30]    [Pg.31]    [Pg.40]    [Pg.263]    [Pg.65]   
See also in sourсe #XX -- [ Pg.51 ]




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