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0012327591
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note
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For "historical" reasons, these calculations use the KB3 interaction [12], which differs from KB1 in some innocuous nonmonopole changes.
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19
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85088488773
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note
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m it is not essential, and we make it only for simplicity.
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21
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85088491166
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note
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28Si, but the large gaps and the spectroscopic factors for the cs ± 1 states indicate strong magicity.
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22
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85088491664
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note
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80Zr is not a closure, but we can always calculate the monopole properties around a closed pf shell.
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23
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0000814677
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S. Kahana, H. C. Lee, and C. K. Scott, Phys. Rev. 180, 956 (1969); 185, 1378 (1969).
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24
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13844315315
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S. Kahana, H. C. Lee, and C. K. Scott, Phys. Rev. 180, 956 (1969); 185, 1378 (1969).
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Phys. Rev.
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25
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0012327593
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Code made available to A. Z. by H. C. Lee in 1969
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Code made available to A. Z. by H. C. Lee in 1969.
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31
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85088490722
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note
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5/2 orbit.
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33
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85088488426
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note
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56Ni, estimated through truncated calculations, must be viewed as a lower limit.
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34
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18344419459
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S. C. Pieper, V. R. Pandharipande, R. B. Wiringa, and J. Carlson, Phys. Rev. C 64, 014001 (2001).
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Carlson, J.4
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