O2 State in 18 O by using Core
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 functio...
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| Format: | Article |
| Language: | English |
| Published: |
University of Thi-Qar
2019-05-01
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| Series: | مجلة علوم ذي قار |
| Online Access: | https://mail.jsci.utq.edu.iq/index.php/main/article/view/318 |
| Summary: | 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 |
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| ISSN: | 1991-8690 2709-0256 |