Elsevier

Nuclear Physics A

Volume 103, Issue 1, 23 October 1967, Pages 71-96
Nuclear Physics A

State dependence of shell-model reaction matrix elements

https://doi.org/10.1016/0375-9474(67)90790-7Get rights and content

Abstract

Shell-model reaction matrix elements are calculated with a combination of the Moszkowski-Scott separation method and the reference-spectrum method of Bethe, Brandow and Petschek. The reaction matrix G is expanded in terms of Gs and VL, where Gs is the reaction matrix for the short-range potential Vs and VL the long-range potential. The contribution from Gs is then calculated with the reference-spectrum method, where the main criterion for choosing the separation distance is that Gs is best approximated by GsR, the reference-spectrum approximation of Gs. The second-order tensor term VTL (Q/e) VTL is calculated with the closure approximation of Kuo and Brown, however the effective energy denominator is now state-dependent, which means that it has a dependence on binding energy, the local density and the centre-of-mass quantum number. The contributions from VTL (Q/e) VTL vary almost linearly with ϱ23, where ϱ is the local density. The reaction matrix elements so calculated have a fairly strong state-dependence which comes in predominantly through Gs and VTL (Q/e) VTL. The state dependence can be approximated quite accurately in a simple way, and thus the application to finite nuclei is convenient. Shell-model applications have been made for nuclei 18O and 18F and we find that the matrix elements are generally weaker than those of Kuo and Brown, especially for those of T = 1, J = 0+ and T = 0, J = 1+. This is desirable, because the Kuo and Brown matrix elements are often somewhat too strong.

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This work was supported in part by the U.S. Atomic Energy Commission and the Higgins Scientific Trust Fund. It made use of the Princeton Computer Facilities supported in part by the National Science Foundation Grant NSF-GP 579.

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