1990
DOI: 10.1016/0370-2693(90)90092-k
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Detection of radioactive 236Pu decay with emission of 28Mg nuclei

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Cited by 31 publications
(14 citation statements)
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“…Cluster radioactivity is an exotic process. The partial half-lives are very long and vary in a wide range from 10 11 to 10 26 s. Branching ratios to the dominant α decay in these nuclei are very small and fall between 10 −9 and 10 −16 . Moreover, spontaneous fission is also a competing decay channel in some heavy cluster emitters [27].…”
Section: Introductionmentioning
confidence: 94%
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“…Cluster radioactivity is an exotic process. The partial half-lives are very long and vary in a wide range from 10 11 to 10 26 s. Branching ratios to the dominant α decay in these nuclei are very small and fall between 10 −9 and 10 −16 . Moreover, spontaneous fission is also a competing decay channel in some heavy cluster emitters [27].…”
Section: Introductionmentioning
confidence: 94%
“…This discovery represented a milestone in the description of nuclear radioactivity as it bridged the gap between the α emission radioactivity and the standard fission reaction. Since then, cluster radioactivity (CR) has been found in twelve eveneven isotopes [2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19][20][21] and seven odd-even isotopes (see, e.g., references in Refs. [22,23]) in the actinide region.…”
Section: Introductionmentioning
confidence: 99%
“…Already measured are the emission of C, Ne, Mg and Si nuclei. A review of the experimental status up to 1989 is given in [9,10], for the latest results see [11][12][13]26]. Quantitative arguments for the emission of fragments heavier than e-particles have been given for the first time by Sandulescu et al in 1980 [14].…”
Section: Extension To Exotic Decaysmentioning
confidence: 98%
“…Formula (12) indicates that, compared to a-spectroscopic factors S~, the spectroscopic factor for heavier fragments should scale like (S,) "/4. The comparison with our microscopic calculations shows [20] that the scaling is much better described by Sbul k = (Sa)(a-1)/3 (bulk spectroscopic factor).…”
Section: J=lmentioning
confidence: 99%
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