2019
DOI: 10.1016/j.nuclphysa.2019.03.002
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Large mirror asymmetry in Gamow-Teller β-decay in the A = 26 isobaric multiplet

Abstract: We investigate a striking example of mirror asymmetry in Gamow-Teller (GT) βdecay using the nuclear shell-model including isospin-nonconserving (INC) forces in the sd-shell region. We show that the large mirror asymmetry between 26 P and 26 Na GT β-decay can be accurately reproduced by introducing T = 1, J ̸ = 0 INC forces related to the s 1/2 orbit, while the usual J = 0 INC force, commonly adopted to describe isospin-symmetry breaking, does not work. We further show that the calculated distribution of summed… Show more

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Cited by 5 publications
(9 citation statements)
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“…The difference in the f t values for Gamow-Teller β transitions of mirror nuclei is also one of the observable signatures of isospin-symmetry breaking, which is referred to as mirror asymmetry. This phenomenon has been reported for transitions in the mirror β decays of several sd-shell nuclei, such as 17 Ne → 17 F [7,8] and 17 N → 17 O [9], 20 Mg → 20 Na [10,11] and 20 O → 20 F [12], 22 Si → 22 Al and 22 O → 22 F [13], 24 Si → 24 Al [14] and 24 Ne → 24 Na [15], 26 P → 26 Si [16] and 26 Na → 26 Mg [17]. β-decay spectroscopic study has proved to be a powerful tool to obtain the structure information adjacent to the drip line, as well as an excellent and stringent test of the accuracy of shell-model predictions far from the valley of stability.…”
Section: Introductionsupporting
confidence: 57%
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“…The difference in the f t values for Gamow-Teller β transitions of mirror nuclei is also one of the observable signatures of isospin-symmetry breaking, which is referred to as mirror asymmetry. This phenomenon has been reported for transitions in the mirror β decays of several sd-shell nuclei, such as 17 Ne → 17 F [7,8] and 17 N → 17 O [9], 20 Mg → 20 Na [10,11] and 20 O → 20 F [12], 22 Si → 22 Al and 22 O → 22 F [13], 24 Si → 24 Al [14] and 24 Ne → 24 Na [15], 26 P → 26 Si [16] and 26 Na → 26 Mg [17]. β-decay spectroscopic study has proved to be a powerful tool to obtain the structure information adjacent to the drip line, as well as an excellent and stringent test of the accuracy of shell-model predictions far from the valley of stability.…”
Section: Introductionsupporting
confidence: 57%
“…Reductions of 1.1%, 0.2%, and 3.0% in the β-detection efficiency for 25 Si, 26 P, and 22 Al, respectively, were estimated compared with that for 27 S. These values can be used as the normalization factors to correct the deviation between reference isotopes and 27 S. As shown in Fig. 5, the absolute efficiency for the γ rays emitted in the β decay of 27 S can be deduced from the efficiency curve fixed by the nine known γ -ray lines, with the normalization factors for the 25 Si, 26 P, and 22 Al decays taken into account. One of the 20 HPGe crystals had worse resolutions and two of them were found to exhibit large gain drifts, so the data from these three crystals are discarded from the analysis.…”
Section: γ-Ray Energy and Efficiency Calibrationmentioning
confidence: 98%
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