βγ (Circularly Polarized) Correlation Measurements in F20 and Al28

L. G. Mann and S. D. Bloom
Phys. Rev. 139, B540 – Published 9 August 1965
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Abstract

A new measurement of the asymmetry parameter A characterizing the βγ (CP) correlation (CP ≡ circularly polarized) for the decays of F20 and Al28 is reported herein. The spin sequence of F20 was already known to be 2+(β)2+(γ)0+ from the work of Freiburg and Soergel. The purpose of the present experiment was to reduce the error on A in order to get a more accurate value for the isospin impurity coefficient α0(1) characterizing the 1.63-MeV state (2+, T0) in Ne20. Our result is A=0.174±0.014. This agrees with Freiburg and Soergel, but represents an improvement in accuracy of a factor of 5. α0(1) is found to be (1.5±2.9) × 103, using the present value for A. By methods described elsewhere, the effective Coulomb matrix element |Hc| is found to be 14±28 keV. A comparison of this value with the values for four other states in Ne20 (Ex=7.2, 13.7, 14.1, and 14.2 MeV), computed by Wilkinson using the E1 prohibition rule in self-conjugate nuclei, indicates that |Hc| tends to be ≲30 keV regardless of excitation (so long as the state is particle-stable). This result also lends support to the surmise expressed earlier that for mixing of states of the type being observed here this upper limit is independent of atomic weight; the bulk of other similar measurements have been made in the atomic weight range of 40 to 150 (with the single exception of Na24). The result for Al28 is A=0.315±0.024. This establishes the 3+ assignment for the ground state of Al28 and corresponds to a pure Gamow-Teller β decay (3+2+). It also rules out the possibility of a Bouchiat-type comparison of the asymmetry parameters for Al28 and P28 (as has been done for the cases of Na24 and Al24) in order to check the conserved-vector-current hypothesis. In addition, the Al28 measurement was of important practical value in verifying the polarimeter calibration, since the single γ ray of 1.77 MeV in the Al28 decay is so close in energy to the F20 γ energy.

  • Received 15 February 1965

DOI:https://doi.org/10.1103/PhysRev.139.B540

©1965 American Physical Society

Authors & Affiliations

L. G. Mann and S. D. Bloom

  • Lawrence Radiation Laboratory, University of California, Livermore, California

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Issue

Vol. 139, Iss. 3B — August 1965

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