Study of the Isobaric Triplet Mg28Al28Si28

Raymond K. Sheline, Noah R. Johnson, P. R. Bell, R. C. Davis, and F. K. McGowan
Phys. Rev. 94, 1642 – Published 15 June 1954
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Abstract

The nuclide Mg28 has been produced by betatron irradiation and cyclotron bombardments in the following reactions: Si30(γ, 2p)Mg28 and Mg26(α, 2p)Mg28. It is a 21.3±0.2 hour β emitter (Emax=0.418±0.01 Mev, logft=4.30). Mg28 decays to Al28 with which it is in secular equilibrium. Milking experiments indicate that the Al28 daughter has a 2.3-min half-life, and confirm the mass assignment of Mg28. Gamma-ray spectra of the Mg28Al28 secular equilibrium mixture indicate gamma rays of the following energies in Mev (intensities in parentheses): 1.769±0.01 (0.98), 1.346±0.01 (0.70), 0.949±0.01 (0.29), 0.400±0.01 (0.31), 0.0319±0.001 (0.96). The 1.769-Mev gamma results from the decay of Al28. Coincidence measurements show that the 1.346-, the 0.949-, and the 0.400-Mev gammas are each in coincidence with the 0.0319-Mev gamma, and that the 0.949- and 0.400-Mev gammas are in coincidence with each other. Delay coincidence measurements between the 1.346-Mev gamma and the 0.0319-Mev gamma indicate that the half-life of the latter is <2×109 sec. This information together with the αKexp=0.032±0.066 indicates that the 0.0319-Mev gamma is an M1 transition as predicted if the ground-state doublet of Al28 is a jj doublet. A complete decay scheme for the isobaric triplet, Mg28Al28Si28, is proposed. All spins and parities of ground and excited states are assigned. Assuming a mass of 27.985818±0.000043 amu for Si28, the mass of Al28 is 27.990809±0.000045 and the mass of Mg28 is 27.992738±0.000047. On the basis of an empirical scheme of nuclear systematics the energy available for decay and the half-lives of the following nuclei are discussed: Si32, Ne24, O20. A test for jj doublets is proposed. This test indicates that the ground state doublets of Al28 and P32 are true jj doublets, whereas the first excited state doublet of Al28 is not.

  • Received 18 January 1954

DOI:https://doi.org/10.1103/PhysRev.94.1642

©1954 American Physical Society

Authors & Affiliations

Raymond K. Sheline and Noah R. Johnson

  • Chemistry Department, Florida State University, Tallahassee, Florida

P. R. Bell, R. C. Davis, and F. K. McGowan

  • Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee

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Issue

Vol. 94, Iss. 6 — June 1954

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