Magnetic dipole transitions in 32S from electron scattering at 180°

F. Hofmann, P. von Neumann-Cosel, F. Neumeyer, C. Rangacharyulu, B. Reitz, A. Richter, G. Schrieder, D. I. Sober, L. W. Fagg, and B. A. Brown
Phys. Rev. C 65, 024311 – Published 15 January 2002
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Abstract

Magnetic dipole transitions in the self-conjugate nucleus 32S up to an excitation energy of 12 MeV have been investigated in inelastic electron scattering at Θe=180° at the superconducting Darmstadt electron linear accelerator (S-DALINAC). Transition strengths have been determined from a plane-wave Born approximation analysis including Coulomb distortion. For the two strongest M1 transitions, where a discrepancy of a factor of about 2 was observed in previous (e,e) experiments, values intermediate between the two extremes are deduced from the present work. The resulting strength distribution is well described by shell-model calculations using the unified sd-shell interaction and an effective M1 operator. The shell-model wave functions also provide a reasonable description of the form factors. A quasiparticle random phase approximation calculation is less successful. The present results allow for the first time studies of the form factor of extremely weak l-forbidden and isoscalar M1 excitations in 32S. The l-forbidden transition allows a sensitive test of tensor corrections to the M1 operator. A combined analysis with the isospin-analog Gamow-Teller (GT) transitions in the A=32 triplet reveals a situation similar to previous studies in A=39 nuclei: microscopic calculations reasonably account for the GT strengths, but fail in the case of M1 strengths. A possible explanation may be found in the nonrelativistic treatment of the latter. Some examples of the role of relativistic corrections are discussed. A consistent description of the reduced transition strength and the form factor of the isoscalar M1 excitation requires isospin mixing with the close-lying isovector transitions. The extracted Coulomb matrix elements are roughly within the limits set by the approximate constancy of the spreading width derived from the analysis of compound-nucleus reactions.

  • Received 3 September 2001

DOI:https://doi.org/10.1103/PhysRevC.65.024311

©2002 American Physical Society

Authors & Affiliations

F. Hofmann, P. von Neumann-Cosel, F. Neumeyer, C. Rangacharyulu*, B. Reitz, A. Richter, and G. Schrieder

  • Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany

D. I. Sober and L. W. Fagg

  • Department of Physics, Catholic University of America, Washington, D.C. 20064

B. A. Brown

  • Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824

  • *Visitor from the University of Saskatchewan, Saskatoon, Canada S7E 5N2.
  • Present address: Jefferson Laboratory, Newport News, VA 23606.

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Vol. 65, Iss. 2 — February 2002

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