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Feasibility of observing the {\alpha} decay chains from isotopes of SHN with Z = 128, Z = 126, Z = 124 and Z = 122

机译:从sHN的同位素观察{\ alpha}衰变链的可行性   Z = 128,Z = 126,Z = 124,Z = 122

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摘要

Taking the Coulomb and proximity potential model for deformed nuclei (CPPMDN)as the interacting potential for the post-scission region, the alpha decayproperties of 34 isotopes of the superheavy nuclei with Z = 128 within therange 306 $\leq$ A $\leq$ 339 have been studied, considering both the parentand daughter nuclei to be deformed. The manuscript also deals with the decayproperties of the isotopes of Z = 126 (within 288 $\leq$ A $\leq$ 339), Z = 124(within 284 $\leq$A $\leq$ 339) and Z = 122 (within 280 $\leq$ A $\leq$ 339).The alpha decay half lives thus evaluated has been compared with the valuesevaluated using other theoretical models and it was seen that, our theoreticalalpha decay half lives matches well with these values. Through the presentstudy, we have underlined and have established the fact that, among the 192isotopes considered in the present study, only those isotopes$^{321-324,328-335}$128, $^{318-320,323-327}$126, $^{305-308,315-322}$124 and$^{298-307,311-314}$122 can be synthesized and detected through alpha decay inlaboratory. As the alpha decay half lives of these superheavy isotopes liewithin the experimental limits, we hope these predictions, on the decay modesof these unknown nuclei, to pave the way for the future experiments. The protonseparation energy calculations on $^{306-339}$128, $^{288-336}$126,$^{284-339}$124 and $^{280-339}$122 superheavy nuclei have also been done andthe study revealed the probable proton emitters among these nuclei.
机译:以变​​形核的库仑和邻近势模型(CPPMDN)作为分裂后区域的相互作用势,Z = 128的超重核的34种同位素的α衰减特性在306 $ \ leq $ A $ \ leq $考虑到父核和子核都发生了变形,对339个进行了研究。该手稿还处理了Z = 126(在288 $ \ leq $ A $ \ leq $ 339之内),Z = 124(在284 $ \ leq $ A $ \ leq $ 339之内)和Z = 122的同位素的衰减特性(在280 $ \ leq $ A $ \ leq $ 339之内)。将这样评估的α衰变半衰期与使用其他理论模型评估的值进行了比较,可以看出,我们的理论α衰变半衰期与这些值非常匹配。通过本研究,我们强调并确定了一个事实,即在本研究中考虑的192个同位素中,只有那些同位素$ ^ {321-324,328-335} $ 128,$ ^ {318-320,323-327} $ 126,$ ^ {305-308,315-322} $ 124和$ ^ {298-307,311-314} $ 122可以通过实验室中的alpha衰减合成和检测。由于这些超重同位素的α衰变半衰期在实验极限之内,我们希望这些关于未知核的衰变模式的预测为将来的实验铺平道路。还完成了对$ ^ {306-339} $ 128,$ ^ {288-336} $ 126,$ ^ {284-339} $ 124和$ ^ {280-339} $ 122超重核的质子分离能的计算,研究发现这些核中可能是质子发射体。

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