scholarly journals THE ASYMPTOTIC BEHAVIOUR OF THE S-MATRIX ELEMENT IN HIGHLY SINGULAR POTENTIAL SCATTERING FOR LARGE IMAGINARY VALUES OF ANGULAR MOMENTUM

1966 ◽  
Vol 22 (9) ◽  
pp. 1046
Author(s):  
CHQU LON-SHIANG

1966 ◽  
Vol 22 (9) ◽  
pp. 1038
Author(s):  
CHQU LON-SHIANG


1965 ◽  
Vol 21 (5) ◽  
pp. 983
Author(s):  
DAI YUAN-BEN


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.



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.



1963 ◽  
Vol 23 (2) ◽  
pp. 187-220 ◽  
Author(s):  
Lowell Brown ◽  
Daniel I Fivel ◽  
Benjamin W Lee ◽  
Raymond F Sawyer


Angular momentum in axisymmetric space-times is investigated. The conclusions lead to a general definition suitable for all asymptoticallyflat spaces which is valid both at infinity and on the event horizon of a black hole. This first paper restricts attention to considerations at infinity. Working in terms of the spin coefficient formalism, the field equations are solved asymptotically at large distances and the definition is evaluated. A conservation law is derived and finally the effect on the angular momentum of a supertranslation of the coordinates is discussed.





1974 ◽  
Vol 7 (18) ◽  
pp. 2267-2272
Author(s):  
G Sethia ◽  
M C Gupta ◽  
C S Shastry


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