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Role of isobar-hole excitations in the quenching of the K40(β)Ca40 transition

B. Castel, H. Toki, and P. Blunden
Phys. Rev. C 25, 2148(R) – Published 1 April 1982
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Abstract

The quenching effects of nuclear and Δ excitations on the β decay of K40 are examined. It is found that although configuration mixing still provides the largest retardation, the inclusion of isobar-hole excitation is necessary to bring the calculation within calling distance of the experimental decay rate.

RADIOACTIVITY K40(β)Ca40. Shell model calculation including isobar-hole excitations.

  • Received 2 November 1981

DOI:https://doi.org/10.1103/PhysRevC.25.2148

©1982 American Physical Society

Authors & Affiliations

B. Castel*

  • Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830 and Physics Department, Queen's University, Kingston, Canada K7L 3N6

H. Toki

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

P. Blunden

  • Physics Department, Queen's University, Kingston, Canada K7L 3N6

  • *Permanent address.

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Vol. 25, Iss. 4 — April 1982

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