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- W2318795539 abstract "Within the framework of dynamical cluster decay model (DCM), the neutron-evaporation residue cross-sections σ3n, σ4n in the hot fusion reaction 48Ca+248Cm→296116* are calculated over a wide range of compound nucleus excitation energies ECN* = 30-45MeV, within a single parameter description known as neck length parameter ΔR. The calculations are done by taking the superheavy proton magic Z=114, 120 and 126 with neutron magic in each case as N=184. Out of the three choices of magic numbers, the neutron evaporation residue contribution comes out to be largest for Z=126, lowest for the Z=114, clearly suggesting that the Z=126 is the strongest magic number, followed by Z=120 and Z=114 in sequence. Also, at comparable energies i.e. 38.9 MeV for neutron evaporation and 37.3 MeV for fission decay, the fragmentation and preformation paths of decaying fragments are almost independent of decay process. The component of quasi-fission is also analyzed along with fusion-fission and evaporation residues cross-sections." @default.
- W2318795539 created "2016-06-24" @default.
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- W2318795539 date "2013-01-01" @default.
- W2318795539 modified "2023-10-16" @default.
- W2318795539 title "Stability aspect of superheavy nucleus [sup 296]116∗ formed in [sup 48]Ca+[sup 248]Cm reaction" @default.
- W2318795539 doi "https://doi.org/10.1063/1.4801693" @default.
- W2318795539 hasPublicationYear "2013" @default.
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