Improving the Phenomenological Version of Alpha Decay Energy of Heavy and Super Heavy Nuclei

Abstract

Abstract The nuclear binding energy calculated by the quark model has been used in the current research to quantify alpha decay energy (Qα- value). The research dealt with the odd-even and even - even type of heavy and super-heavy nuclei within the range (78≤ Z ≤ 118). By knowing the number of Z and N for a given nucleus, regardless of its mass, it became possible to calculate the energy of alpha decay. By correlating the experimental nuclear binding energy values of the parent nucleus and its daughters with the theoretically computed values, the quark model was adapted. Graphically extracted calibration equations have been used to produce a modern version of the alpha decay energy by linear and logarithmic matching. As essential statistical instruments, the square root rate and standard deviation were determined to show the utility of adjusted models in testing decay energy and nuclear binding energy. The analyses revealed that the experimental results have been approved.