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- W4256079369 abstract "Coulomb form factors for E0 transition in 18O are discussed taking into account core-polarization effects. These effects are taken into account through the collective model of Tassie and also through a microscopic perturbation theory including excitations up to 2p1f shell. Space wave model functions defined for the orbits 1 and 2125O nucleus has been the subject of extensive theoretical and experimental studies, which received much attention in last decade [Alex Brown et.al.2005]. The 18O system contains two neutrons in addition to the16O core distributed in the sd – shell. d1 are obtained from the diagonalization of the interaction Hamilonian of Wildenthal. The calculations include the 0 2state with excitation energies3.6337MeV. The core – polarization effects which incorporate the ollective model of Tassei describe the data very well for this state." @default.
- W4256079369 created "2022-05-12" @default.
- W4256079369 date "2008-01-01" @default.
- W4256079369 modified "2023-10-18" @default.
- W4256079369 title "O2 State in 18 O by using Core – Polarization effects" @default.
- W4256079369 doi "https://doi.org/10.32792/thi/sc/vol.1.is.1.09" @default.
- W4256079369 hasPublicationYear "2008" @default.
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