Effect of deformation, particle-hole and particle-particle interaction on Gamow-Teller transitions of 76Ge
Abstract
Gamow-Teller (GT) transitions for 76Ge using QRPA methods in this article are calculated, which play an essential role in the supernovae. Three different QRPA models are used to the GT strength distributions. QRPA models namely single quasi-particle (sqp), Pyatov Method (PM) and the Schematic Model (SM). Gamow-Teller distribution, ΣB(GT)-, the centroid of energy, the width of energy and ISR are calculated by using these models. The effect of particle-particle interaction on spherical nuclei and deformed nuclei on Gamow-Teller transitions is wanted to show. Deformed Woods-Saxon potential is used in calculations of Single-particle energies and wave functions. The results are also compared with previous theoretical calculations and measured strength distributions wherever available. It is expected that the current study of GT features would be helpful and may guide to a better knowledge of the presupernova progression of massive stars.
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References
- [1] Fuller G.M., Fowler W.A. and Newman M.J., Stellar weak-interaction rates for sd-shell nuclei. I. Nuclear matrix element systematics with application to 26Al and selected nuclei of importance to the supernova problem, Astrophys. J. Suppl. Ser., 42 (1980) 447-473
- [2] Aufderheide M.B., Fushiki I., Woosley S.E., Stanford E. and Hartmann D.H., Search for important weak interaction nuclei in presupernova evolution, Astrophys. J. Suppl. Ser., 91 (1994) 389–417.
- [3] Nabi J.-Un., Klapdor-Kleingrothaus H.V., Microscopic calculations of weak interaction rates of nuclei in stellar environment for A = 18 to 100, Eur. Phys. J. A, 5 (1999) 337–339.
- [4] Langanke K., Martínez-Pinedo G., Shell-model calculations of stellar weak interaction rates. II. Weak rates for nuclei in the mass range A = 45–65 in supernovae environments, Nucl. Phys. A, 673 (2000) 481-508.
- [5] Pyatov N.I., Salamov D.I., Conservation laws and collective excitations in nuclei, Nucleonica, 22 (1977) 1–127.
- [6] Civitarese O., Hess P.D., Hirsch J.G. and Reboiro M., Spontaneous and dynamical breaking of mean field symmetries in the proton neutron quasi particle random phase approximation, Phys. Rev. C, 59 (1998) 194-199.
- [7] Magierski P.,Wyss R., Self consistent effective interactions and symmetry restoration, Phys. Lett. B, 468 (2000) 54-60.
- [8] Kulliev A.A., Akkaya R., Ilhan M., Guliev E., Salamov C., Selvi S., Rotational invariant model of the states with Kπ = 1+ and their contribution to the scissors mode, Int. J. Mod. Phys. E, 9 (2000) 249-261.
Details
Primary Language
English
Subjects
-
Journal Section
Research Article
Authors
Şadiye Çakmak
*
0000-0001-9256-0571
Türkiye
Publication Date
March 22, 2020
Submission Date
November 22, 2019
Acceptance Date
February 17, 2020
Published in Issue
Year 2020 Volume: 41 Number: 1