| dc.creator |
Vary, J. P. |
|
| dc.creator |
Maris, P. |
|
| dc.creator |
Barrett, B. R. |
|
| dc.creator |
Lisetskiy, A. F. |
|
| dc.creator |
Dikmen, E. |
|
| dc.creator |
Shirokov, A. M. |
|
| dc.date |
2015-06-02T00:00:00Z |
|
| dc.date.accessioned |
2021-12-03T11:20:48Z |
|
| dc.date.available |
2021-12-03T11:20:48Z |
|
| dc.identifier |
4325d6e4-bdaa-48fe-b5b5-eaac4b7dc705 |
|
| dc.identifier |
10.1103/physrevc.91.064301 |
|
| dc.identifier |
https://avesis.sdu.edu.tr/publication/details/4325d6e4-bdaa-48fe-b5b5-eaac4b7dc705/oai |
|
| dc.identifier.uri |
http://acikerisim.sdu.edu.tr/xmlui/handle/123456789/91179 |
|
| dc.description |
We perform ab initio no-core shell-model calculations for A = 18 and 19 nuclei in a 4 (h) over bar Omega, or N-max = 4, model space by using the effective JISP16 and chiral N3LO nucleon-nucleon potentials and transform the many-body effective Hamiltonians into the 0 (h) over bar Omega model space to construct the A-body effective Hamiltonians in the sd shell. We separate the A-body effective Hamiltonians with A = 18 and A = 19 into inert core, one-, and two-body components. Then we use these core, one-, and two-body components to perform standard shell-model calculations for the A = 18 and A = 19 systems with valence nucleons restricted to the sd shell. Finally, we compare the standard shell-model results in the 0 (h) over bar Omega model space with the exact no-core shell-model results in the 4 (h) over bar Omega model space for the A = 18 and A = 19 systems and find good agreement. |
|
| dc.language |
eng |
|
| dc.rights |
info:eu-repo/semantics/openAccess |
|
| dc.title |
Ab initio effective interactions for sd-shell valence nucleons |
|
| dc.type |
info:eu-repo/semantics/article |
|