Inelastic scattering E4 transition probabilities in the 0d, 1s shell

B. A. Brown, W. Chung, and B. H. Wildenthal
Phys. Rev. C 21, 2600 – Published 1 June 1980
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Abstract

Theoretical E4 transition matrix elements calculated in the full d52s12d32 shell-model space are presented for excitations of some ground states of stable nuclei for 18A38. These matrix elements have been used to calculate inelastic transition probabilities for electromagnetic and hadronic probes. Available data on the relative magnitudes and energy distributions of E4 excitation strengths are found to be well reproduced theoretically thereby. Based on several experimentally measured transition strengths, the empirical isoscalar E4 effective charge is found to be ep+en=(2.0±0.2)e. This is similar in magnitude to the analogous isoscalar E2 effective charge, but is much larger than existing theoretical estimates.

NUCLEAR STRUCTURE O18, F19, Ne20, Ne22, Mg24, Mg25, Mg26, Si28, Si30, S32, S34, Ar36, Ar38; calculations for the strengths of E4 inelastic scattering transitions and their proton and neutron components; complete 0d521s520d32 shell-model wave functions; Chung-Wildenthal Hamiltonians.

  • Received 25 January 1980

DOI:https://doi.org/10.1103/PhysRevC.21.2600

©1980 American Physical Society

Authors & Affiliations

B. A. Brown

  • Nuclear Physics Laboratory, Oxford University, Oxford OX1 3RH, England

W. Chung

  • Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824

B. H. Wildenthal*

  • Nuclear Physics Laboratory, Oxford University, Oxford OX1 3RH, England and Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824

  • *Permanent address.

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Vol. 21, Iss. 6 — June 1980

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