1999
DOI: 10.1016/s1350-4487(99)00086-4
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Use of phosphate glass detectors for study of curium-242 cluster radioactivity

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Cited by 3 publications
(4 citation statements)
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“…In the case of 232-235 U, 236 Pu the maximum preformation is obtained for 28 Mg cluster. For 236 U parent 28,30 [63]) and in the case of 238 Pu parent 28,30 [64]) but the highest peaks in cluster formation probability is obtained for 30 Mg as compared to 28 Mg cluster. i.e.…”
Section: Resultsmentioning
confidence: 89%
See 1 more Smart Citation
“…In the case of 232-235 U, 236 Pu the maximum preformation is obtained for 28 Mg cluster. For 236 U parent 28,30 [63]) and in the case of 238 Pu parent 28,30 [64]) but the highest peaks in cluster formation probability is obtained for 30 Mg as compared to 28 Mg cluster. i.e.…”
Section: Resultsmentioning
confidence: 89%
“…For the case of 234 U parent the cluster radioactivity is observed for 24,26 [62], but the cluster formation probability is maximum for 26 Ne cluster compared to other decays. We have computed the half life for these cluster emissions and it is found that the lowest half life time is for 26 [63] cluster decays are experimentally observed, i.e the 26 Ne cluster emission has the lower half life. As we compared the cluster formation probability of these clusters it is found that the 26 Ne cluster has the larger preformation probability value.…”
Section: Resultsmentioning
confidence: 99%
“…This rare phenomenon was first discussed theoretically in 1980 by Săndulescu, Poenaru and Greiner [1]. Experimental confirmation came four years later with the observation of the 14 C spontaneous emission from 223 Ra, by Rose and Jones [2]. To date, about 35 cluster decay modes have been observed for nuclei in the trans-lead region of 221 < A < 242 and 87 < Z < 96, with daughter nuclei in the neighborhood of 208 Pb.…”
Section: Introductionmentioning
confidence: 95%
“…To date, about 35 cluster decay modes have been observed for nuclei in the trans-lead region of 221 < A < 242 and 87 < Z < 96, with daughter nuclei in the neighborhood of 208 Pb. The observed emitted clusters include 14 C [2], 15 N [3], 18,20 O [4, 5], 22,24,25,26 Ne [6-10], 23 F [11], 28,30 Mg [6,[12][13][14], and 32,34 Si [13,15]. In principle, these decays are characterized with long partial half-lives lying between 10 11 s and 10 28 s, and very small branching ratios relative to α-decay in the range from 10 −9 and 10 −16 [16].…”
Section: Introductionmentioning
confidence: 99%