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Electromagnetic transition

To understand the parity of electromagnetic transitions, we need to recall that each of the initial and final states of the nucleus undergoing the transition can be... [Pg.224]

Conventional spherical shell model calculations have been undertaken to describe 90 88zr and 90 88y in these large scale calculations valence orbitals included If5/2 2P3/2 2Pl/2 and 199/2 The d5/2 orbital was included for 98Y and for high-spin calculations in 98Zr. Restrictions were placed on orbital occupancy so that the basis set amounted to less than 2b,000 Slater determinants. Calculations were done with a local, state independent, two-body interaction with single Yukawa form factor. Predicted excitation energies and electromagnetic transition rates are compared with recent experimental results. [Pg.87]

Selected electromagnetic moments are presented in Tables III. Agreement for the electric quadrupole moment and magnetic moment for the 8]+ state is not very good for 88Zr(8 +). There are several electromagnetic transitions rates that can be compared The calculated value B(E2 8]+... [Pg.90]

For a space of eigenvectors of matrices of the gaussian orthogonal ensemble (k = N) the distribution of values of matrix elements of electromagnetic transition operators is gaussian, as follows from the central limit theorem. The ensemble averaging of hamiltonians guarantees that no correlations exist between the hamiltonian structure and the particular transition operator that is considered. [Pg.123]

In fig. la-c the distribution function (14) is compared for isoscalar Ml-, E2- and E4-electromagnetic transition amplitudes with shell-model results for 20Ne(T s0,T2 0), calculated in the sd-conf iguration space. A surface delta interaction was used with strength parameters [BRU77] Aq Aj ... [Pg.125]

Fig. 3. X-ray spectrum in the energy range of the pH(np — Is) transitions as measured with MOS CCDs. The pure electromagnetic transition energies for the 2p — Is transitions of the hydrogen isotopes are 9405.7 keV and 12.505 keV... Fig. 3. X-ray spectrum in the energy range of the pH(np — Is) transitions as measured with MOS CCDs. The pure electromagnetic transition energies for the 2p — Is transitions of the hydrogen isotopes are 9405.7 keV and 12.505 keV...
Metastable muonium atoms in the 2s state have been produced with a beam foil technique at LAMPF and at the Tri University Meson Physics Facility (TRI-UMF) at Vancouver, Canada. Only moderate numbers of atoms could be obtained. The velocity resonance nature of the electron transfer reaction results in a muonium beam at keV energies. Very difficult and challenging experiments using electromagnetic transitions in excited states, particularly the 2 Si/2 2 Pi/2 classical Lamb shift and 2 Si/2-2 P3/2 splitting could be induced with microwaves. However, the achieved experimental accuracy at the 1.5 % level [18,19,20], does not represent a severe test of theory yet. [Pg.84]

The values of Z and 7 values belong to a class of solvent parameters based on various standard physical processes (electromagnetic transition, dielectric constant, NMR chemical shift, etc.. In the context of similarity these parameters are not directly useful for mechanistic studies because the reference process is a physical property rather than a chemical reaction. The parameters Z and are often linearly related to the Grunwald-Winstein Y value (Figure 14) and provide a secondary definition of Y values which are inaccessible via the chemical definition of those parameters. [Pg.39]

Mass Scaling Laws and Lowering of Symmetry Electromagnetic Transition Intensities Anharmonic Couplings... [Pg.455]

Linear Triatomic Molecules Anharmonic (Fermi) Interactions Rotational Spectroscopy Electromagnetic Transition Intensities... [Pg.455]

The nuclear reactions are described as taking place in two steps (1) the formation of a compound nucleus in a highly excited virtual level, and (2) the dissociation of this compound nucleus leading to a state of high excitation of the product nucleus. The product nucleus, which decays promptly by electromagnetic transitions, ends up in the ground state or in some low-lying metastable level called an isomer. [Pg.358]


See other pages where Electromagnetic transition is mentioned: [Pg.322]    [Pg.225]    [Pg.226]    [Pg.227]    [Pg.229]    [Pg.231]    [Pg.236]    [Pg.241]    [Pg.88]    [Pg.122]    [Pg.123]    [Pg.124]    [Pg.126]    [Pg.84]    [Pg.105]    [Pg.556]    [Pg.610]    [Pg.222]    [Pg.1001]   
See also in sourсe #XX -- [ Pg.56 , Pg.73 , Pg.75 , Pg.76 , Pg.79 , Pg.80 , Pg.81 , Pg.96 , Pg.103 ]




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