2002
DOI: 10.1134/1.1471280
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Binding energies and radii of α-cluster-type nuclei from calculations based on the strictly restricted dynamics model

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Cited by 1 publication
(4 citation statements)
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“…The increase is offset slightly because the rms radius is now defined with respect to the centre of mass of the cluster system. Such cluster calculations have been carried out for 44 Ti [14,15] and predict rms radii consistent with the present measurement. However, the accuracy of the calculations is limited and the uncertainties are large compared to the apparent discrepancy between the Ca and Ti (N = 22) isotone radii, which is at the level of 0.01 fm.…”
Section: Discussionsupporting
confidence: 79%
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“…The increase is offset slightly because the rms radius is now defined with respect to the centre of mass of the cluster system. Such cluster calculations have been carried out for 44 Ti [14,15] and predict rms radii consistent with the present measurement. However, the accuracy of the calculations is limited and the uncertainties are large compared to the apparent discrepancy between the Ca and Ti (N = 22) isotone radii, which is at the level of 0.01 fm.…”
Section: Discussionsupporting
confidence: 79%
“…However, the accuracy of the calculations is limited and the uncertainties are large compared to the apparent discrepancy between the Ca and Ti (N = 22) isotone radii, which is at the level of 0.01 fm. The calculations by Krasta et al [14] have an rms deviation with experimental values of at least 0.07 fm (covering nine cluster nuclei below A = 44). For 44 Ti, they predict an rms radius of 3.64 fm, compared to our experimental value of 3.618(4) fm (table 1).…”
Section: Discussionmentioning
confidence: 87%
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