Interaction Matrix Element in a Shell Model

1963 ◽  
Vol 129 (6) ◽  
pp. 2643-2652 ◽  
Author(s):  
U. Fano ◽  
F. Prats ◽  
Z. Goldschmidt
2017 ◽  
Vol 26 (01n02) ◽  
pp. 1740021 ◽  
Author(s):  
Wesley Pereira ◽  
Ricardo Garcia ◽  
Larry Zamick ◽  
Alberto Escuderos ◽  
Kai Neergård

We report the discovery of a partial conservation law obeyed by a schematic Hamiltonian of two protons and two neutrons in a [Formula: see text] shell. In our Hamiltonian, the interaction matrix element of two nucleons with combined angular momentum [Formula: see text] is linear in [Formula: see text] for even [Formula: see text] and constant for odd [Formula: see text]. It turns out that in some stationary states, the sum of the angular momenta [Formula: see text] and [Formula: see text] of the proton and neutron pairs is conserved. The energies of these states are given by a linear function of [Formula: see text]. The systematics of their occurrence is described and explained.


1986 ◽  
Vol 41 (5) ◽  
pp. 704-714
Author(s):  
D. Campos ◽  
J. M. Tejeiro ◽  
F. Cristancho

We introduce a multichannel “potential curves hopping” model and obtain the exact quantum mechanical S-matrix by solving the associated set of coupled second-order ordinary differential equations that describes the inelastic collisions between atomic particles. The only assumption is that the interaction matrix element between each pair of channels (say, γ and β) is of the form Uγβ(r) = Uβγ(r) =: Uγβ δ( r - rγβ), where δ (c) is the Dirac deltafunction, and rγβ and Uγβ are parameters which can be chosen freely.Semiclassical techniques can be incorporated directly in the theory if the Schrödinger equations for the uncoupled channels allow this treatment. The formulation is particularized to the two-channel problem and illustrated with a semiclassical example the He+ + Ne problem at 70.9 eV.


1971 ◽  
Vol 49 (9) ◽  
pp. 1205-1210 ◽  
Author(s):  
Charlotte Froese Fischer

Self-consistent field calculations have been performed in three different ways for the average energy of the configurations 3dq−14s2, 3dq4s, and 3dq+1, q = 2,3,..., 9 of the neutral atoms scandium to nickel. The calculations differ in the way the radial functions depend on the configuration. Parameters which enter into the interaction matrix for states of these configurations are reported. It is shown that the lack of orthogonality of an orbital from one configuration with that of another may alter the interaction matrix element significantly, and that the parameters for radial functions independent of the configuration are significantly different from those that depend on the configuration.


2008 ◽  
Author(s):  
L. Kaplan ◽  
Y. Alhassid ◽  
Pawel Danielewicz ◽  
Piotr Piecuch ◽  
Vladimir Zelevinsky

1997 ◽  
Vol 56 (5) ◽  
pp. 2542-2548 ◽  
Author(s):  
P. Navrátil ◽  
B. R. Barrett ◽  
W. E. Ormand

1969 ◽  
Vol 47 (22) ◽  
pp. 2459-2474 ◽  
Author(s):  
M. K. Srivastava ◽  
A. M. Jopko ◽  
Donald W. L. Sprung

A method suggested by Elliott for calculating nuclear interaction matrix elements directly from phase shifts is developed into a practical scheme applicable to all partial waves. Matrix elements are constructed from experimental phase shifts and compared to several other calculations. A shell-model calculation of 58Ni based on these matrix elements gives results comparable to those of Kuo.


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