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arXiv 1106.3271nucl-th
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超重核的重粒子放射性

Heavy particle radioactivities of superheavy nuclei

D. N. Poenaru, R. A. Gherghescu, W. Greiner

摘要:

重粒子放射性的概念被改变为允许从Z>110的母体和208 Pb左右的子体发射Z_e>28的粒子。对Z=104-124的超重核(SH)的计算表明,相对于较重的SH的α衰变,其半衰期更短,分支比更大。有可能找到HPR比α衰变更强的区域。新的质量表AME 11和理论KTUY 05和FRDM 95质量用于确定释放的能量。对于124,我们发现了半衰期在ns到ps范围内的同位素。

英文摘要:

The concept of heavy particle radioactivity (HPR) is changed to allow emitted particles with Z_e>28 from parents with Z>110 and daughter around 208Pb. Calculations for superheavy (SH) nuclei with Z=104-124 are showing a trend toward shorter half-lives and larger branching ratio relative to alpha decay for heavier SHs. It is possible to find regions in which HPR is stronger than alpha decay. The new mass table AME11 and the theoretical KTUY05 and FRDM95 masses are used to determine the released energy. For 124 we found isotopes with half-lives in the range of ns to ps.

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