| dc.creator |
Dikmen, Erdal |
|
| dc.date |
2006-06-01T00:00:00Z |
|
| dc.date.accessioned |
2021-12-03T11:31:44Z |
|
| dc.date.available |
2021-12-03T11:31:44Z |
|
| dc.identifier |
889f1814-d63b-4caa-becc-7d4bd49dfc54 |
|
| dc.identifier |
10.1088/0256-307x/23/6/020 |
|
| dc.identifier |
https://avesis.sdu.edu.tr/publication/details/889f1814-d63b-4caa-becc-7d4bd49dfc54/oai |
|
| dc.identifier.uri |
http://acikerisim.sdu.edu.tr/xmlui/handle/123456789/93160 |
|
| dc.description |
The full and reduced shell model calculations have been carried out for the light odd-even Sb-105 and Sb-107 isotopes. The model space has ben chosen as 1d(5/2), 0g(7/2), 1d(3/2), 2s(1/2), and 0h(11/2) for the full calculations and excluded 0h(11/2) for the reduced calculations. The reduced shell model calculations of Sb-105 and Sb-107 isotopes are presented for the first time. We obtain the energy spectra for the Sb-105 and Sb-107 isotopes in the full and reduced model space by using CD-Bonn two-body effective nucleon-nucleon interaction. The resulting energy spectra are compared to the experimental results to understand the effect of the 0h(11/2) level on the shell model calculations. We draw conclusions about the right model space in the shell model calculations for the isotopes around the N = Z = 50 region of the periodic table. |
|
| dc.language |
eng |
|
| dc.rights |
info:eu-repo/semantics/closedAccess |
|
| dc.title |
Effect of 0h (11/2) level on shell model calculations of Sb-105 and Sb-107 |
|
| dc.type |
info:eu-repo/semantics/article |
|