?-decay of N=126 isotones for the r-process nucleosynthesis
dc.authorid | , Jameel-Un-Nabi/0000-0002-8229-8757 | |
dc.authorid | Cakmak, Necla/0000-0001-5989-6663 | |
dc.contributor.author | Nabi, Jameel-Un | |
dc.contributor.author | Cakmak, Necla | |
dc.contributor.author | Ullah, Asim | |
dc.contributor.author | Ullah Khan, Asad | |
dc.date.accessioned | 2024-09-29T16:03:02Z | |
dc.date.available | 2024-09-29T16:03:02Z | |
dc.date.issued | 2021 | |
dc.department | Karabük Üniversitesi | en_US |
dc.description.abstract | The 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. | en_US |
dc.identifier.doi | 10.1088/1402-4896/ac13e4 | |
dc.identifier.issn | 0031-8949 | |
dc.identifier.issn | 1402-4896 | |
dc.identifier.issue | 11 | en_US |
dc.identifier.scopus | 2-s2.0-85112118711 | en_US |
dc.identifier.scopusquality | Q2 | en_US |
dc.identifier.uri | https://doi.org/10.1088/1402-4896/ac13e4 | |
dc.identifier.uri | https://hdl.handle.net/20.500.14619/5859 | |
dc.identifier.volume | 96 | en_US |
dc.identifier.wos | WOS:000675617900001 | en_US |
dc.identifier.wosquality | Q2 | en_US |
dc.indekslendigikaynak | Web of Science | en_US |
dc.indekslendigikaynak | Scopus | en_US |
dc.language.iso | en | en_US |
dc.publisher | Iop Publishing Ltd | en_US |
dc.relation.ispartof | Physica Scripta | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/closedAccess | en_US |
dc.subject | Gamow-Teller transitions | en_US |
dc.subject | first-forbidden transitions | en_US |
dc.subject | pn-QRPA theory | en_US |
dc.subject | waiting-point nuclei | en_US |
dc.subject | beta-decay rates | en_US |
dc.subject | r-process | en_US |
dc.title | ?-decay of N=126 isotones for the r-process nucleosynthesis | en_US |
dc.type | Article | en_US |