“…In this work, using CYE model we have tried to study the half-lives for the predicted SHN 298,310 114, 306,318 122, 308,310 124 and 310,322 126 during the cluster emission such as 4 He, 9 Be, 11 B, 12 C, 14 N, 16 O, 19 F, 20 Ne, 23 Na, 24 Mg, 27 Al, 28 Si, 31 P, 34 S, 35 Cl, 40 Ar, 39 K and 40 Ca. The results of our study have been compared with those of available theoretical values [28][29][30][31][32] and are tabulated in Table 1.…”