2019
DOI: 10.1007/s13538-019-00681-6
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Existence of 15-21N, 17-23O, and 19-25F Neutron Halo Nuclei via Cluster Decay Process in the Superheavy Region

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Cited by 5 publications
(9 citation statements)
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“…From Figure 1, it is clear that in the case of 29,31 Ne, the (V -Q) is minimum for the 1n + core configuration. Similarly, Figures 2 to 5; shows that for 34 Na, 37 Na, 37 Mg and 55 Ca have also the 1n + core configuration has the deepest minimum corresponding to the most probable configuration. Hence, they can be considered as candidates for 1n-halo nuclei.…”
Section: Resultsmentioning
confidence: 63%
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“…From Figure 1, it is clear that in the case of 29,31 Ne, the (V -Q) is minimum for the 1n + core configuration. Similarly, Figures 2 to 5; shows that for 34 Na, 37 Na, 37 Mg and 55 Ca have also the 1n + core configuration has the deepest minimum corresponding to the most probable configuration. Hence, they can be considered as candidates for 1n-halo nuclei.…”
Section: Resultsmentioning
confidence: 63%
“…These are tabulated and given in table 1. On the basis of our calculation of S(n), the possible 1n-halo candidates in the region Z = 10 -20 are 29 Ne, 31 Ne, 36 Na, 37 Na, 35 Mg, 37 Mg, 46 P and 55 Ca. The isotopes of Z = 10 -20 nuclei showed a lower 2n-separation energy than 1n-separation energy only for 34 Ne and can be considered as a candidate for 2n-halo.…”
Section: Resultsmentioning
confidence: 99%
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