Walsh's rules, closed shells, and localized electron models

1971 ◽  
Vol 93 (18) ◽  
pp. 4609-4610 ◽  
Author(s):  
H. Bradford Thompson
2016 ◽  
Vol 2016 ◽  
pp. 1-30 ◽  
Author(s):  
Dongyan Shi ◽  
Yunke Zhao ◽  
Qingshan Wang ◽  
Xiaoyan Teng ◽  
Fuzhen Pang

This paper presents free vibration analysis of open and closed shells with arbitrary boundary conditions using a spectro-geometric-Ritz method. In this method, regardless of the boundary conditions, each of the displacement components of open and closed shells is represented simultaneously as a standard Fourier cosine series and several auxiliary functions. The auxiliary functions are introduced to accelerate the convergence of the series expansion and eliminate all the relevant discontinuities with the displacement and its derivatives at the boundaries. The boundary conditions are modeled using the spring stiffness technique. All the expansion coefficients are treated equally and independently as the generalized coordinates and determined using Rayleigh-Ritz method. By using this method, a unified vibration analysis model for the open and closed shells with arbitrary boundary conditions can be established without the need of changing either the equations of motion or the expression of the displacement components. The reliability and accuracy of the proposed method are validated with the FEM results and those from the literature.


1972 ◽  
Vol 27 (4) ◽  
pp. 545-552 ◽  
Author(s):  
R. Albat

Abstract An Approximation of Löwdin's Natural Orbitals for Molecules with a Green's Function Method The many-body-pertubation theorie of the single-particle Green's function is used to get an approximate first-order density matrix. Slightly modified SCF-orbitals form the basis for the expansion. The mass-operator in Dyson's equation is considered up to second order in the Perturbation. In the present form the method is only applicable to ground states with closed shells. The ground states of the molecules LiH and NH3 serve as examples to demonstrate the usefulness of the directly calculated natural orbitals for application in the C I-method. The natural orbitals give a much better convergence of the C I-expansion than the SCF-orbitals do.


2020 ◽  
Vol 15 ◽  
pp. 57
Author(s):  
G. S. Anagnostatos

The significant features of exchange symmetry are displayed by simple systems such as two identical, spinless fermions in a one-dimensional well with infinite walls. The conclusion is that the maxima of probability of the antisymmetrized wave function of these two fermions lie at the same positions as if a repulsive force (of unknown nature) was applied between these two fermions. This conclusion is combined with the solution of a mathematical problem dealing with the equilibrium of identical repulsive particles (of one or two kinds) on one or more spheres like neutrons and protons on nuclear shells. Such particles are at equilibrium only for specific numbers of particles and, in addition, if these particles lie on the vertices of regular polyhedra or their derivative polyhedra. Finally, this result leads to a pictorial representation of the structure of all closed shell nuclei. This representation could be used as a laboratory for determining nuclear properties and corresponding wave functions.


1961 ◽  
Vol 16 (10) ◽  
pp. 1083-1089
Author(s):  
Hans Hackenbroich

The interplay of the quantum mechanical rotation of a core consisting of closed shells and nucleons outside the closed shells is considered. The core is characterized by its moment of inertia and its deformation is taken to be the same as the deformation of the one particle potential. Energies and wave functions of the system are calculated with the help of a variation method. The distortion of the wave function of the outer nucleons due to the rotation is considerably smaller than computed from first order perturbation theory. The INGLIS formula for rotational energies is a limiting case of our energy equation.The core moment of inertia enters the model as a parameter. This parameter can be estimated from the vibrational energies of spherical nuclei and from the rotational-vibrational interaction, but the two values obtained are not in good agreement. In our example (158Gd) only the second value gives the correct moment of inertia of the whole nucleus.


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