We have made an attempt to parameterize decay energies (Q) during the cluster emissions such as ⁴He, ⁶Li, ⁹Be,^20,22Ne, ²³Na, ²⁴⁻²⁶ Mg, ²⁷Al, ²⁸⁻³⁰Si, ³²⁻³⁴S, ³⁵Cl, ^36,38,40Ar, ^39,41 K and ^{40,42–44,46}Ca from the superheavy nuclei 103 < Z < 126. We have formulated an empirical formula for decay energies of superheavy nuclei during the emission of different clusters of nuclei. To check the predictive power of constructed formula, we have compared the decay energies produced by the present formula with that of the experiments. The constructed empirical formula can reproduce the Q-values during the cluster emissions using simple inputs of mass number of daughter nuclei, atomic number of cluster emission and neutron number of parent nuclei.

我们已尝试对簇发射期间的衰变能量（Q）进行参数化，例如⁴ He，⁶ Li，⁹ Be，^20,22 Ne，²³ Na，²⁴⁻²⁶  Mg，²⁷ Al，²⁸⁻³⁰ Si，^{32− 34} S，³⁵ Cl，^36,38,40 Ar，^39,41  K和^{40,42–44,46}来自超重核103 <Z <126的Ca。我们为不同重核的发射过程中超重核的衰变能量建立了经验公式。为了检查构造公式的预测能力，我们将本公式产生的衰减能量与实验结果进行了比较。所建立的经验公式可以使用子核的质量数，簇发射的原子数和母核的中子数的简单输入来重现簇发射期间的Q值。