Nabi, Jameel-UnCakmak, NeclaUllah, AsimUllah Khan, Asad2024-09-292024-09-2920210031-89491402-4896https://doi.org/10.1088/1402-4896/ac13e4https://hdl.handle.net/20.500.14619/5859The beta-decay properties of nuclei with neutron number N = 126 is investigated in this paper. Two different versions of the proton-neutron quasi particle random phase (pn-QRPA) model were employed to compute beta-decay rates and half-lives for the N = 126 isotones. The first set of calculation solves the pn-QRPA equations using the schematic model (SM) approach. The Woods-Saxon potential was employed as a mean-field basis. A spherical shape assigned for each waiting point nuclei throughout all simulations. Both allowed Gamow-Teller (GT) and first-forbidden (FF) transitions were considered in the particle-hole (ph) channel. The second set uses the pn-QRPA model in deformed Nilsson basis to calculate beta-decay rates for allowed GT and unique first-forbidden (U1F) transitions under terrestrial and stellar conditions. Our results are in agreement with shell model findings that first-forbidden transitions lead to a considerable decrement in the calculated half-lives of the isotones. Inclusion of the first-forbidden contribution led to a decent agreement of our computed terrestrial beta-decay half-lives with measured ones, much better than the previous calculations. The possible implication of the waiting point nuclei on r-process nucleosynthesis is discussed briefly.eninfo:eu-repo/semantics/closedAccessGamow-Teller transitionsfirst-forbidden transitionspn-QRPA theorywaiting-point nucleibeta-decay ratesr-processArticle10.1088/1402-4896/ac13e42-s2.0-8511211871111Q296WOS:000675617900001Q2