Abstract
Excited states of the Po203 (Z=84,N=119) have been investigated after populating them through Pt194(C13,4n) fusion-evaporation reaction at Ebeam=74 MeV and using a large array of Compton-suppressed HPGe clover detectors as the detection setup for the emitted γ rays. Standard techniques of γ-ray spectroscopy have been applied towards establishing the level structure of the nucleus. Twenty five new γ-ray transitions have been identified therein, through γ-γ coincidence measurements, and spin-parity assignments of several states have been determined or confirmed, following the angular correlation and linear polarization measurements on the observed γ rays. The excited states have been interpreted in the framework of large basis shell-model calculations, while comparing their calculated and experimental energies. They have been principally ascribed to proton population in the h9/2 and i13/2 orbitals outside the Z=82 closure and neutron occupation of the f5/2, p3/2, and i13/2 orbitals in the N=126 shell.
| Original language | English |
|---|---|
| Article number | 044329 |
| Journal | Physical Review C |
| Volume | 106 |
| Issue number | 4 |
| DOIs | |
| State | Published - Oct 2022 |
| Externally published | Yes |
Bibliographical note
Publisher Copyright:© 2022 American Physical Society.
Funding
The authors wish to thank the staff associated with the Pelletron Facility at IUAC, New Delhi, for their help and support during the experiment. We record our deepest gratitude for Prof. Asimananda Goswami and Pradipta Kumar Das, of the Saha Institute of Nuclear Physics (SINP), Kolkata, for their guidance, help, and active contribution in the target preparation. Help and support received from Kausik Basu (UGC-DAE CSR, KC) during the experiment, is appreciated. Help of V. Vishnu Jyothi during the experiment is also acknowledged. P.C.S. acknowledges a research grant from SERB (India), CRG/2019/000556. B.M. acknowledges the support from Department of Science and Technology, Government of India through DST/INSPIRE Fellowship (No. DST/INSPIRE Fellowship/2020/IF200310). U.G. acknowledges the support from US National Science Foundation through Grants No. PHY1762495 and No. PHY2011890. This work is partially supported by the Department of Science and Technology, Government of India (No. IR/S2/PF-03/2003-II).
| Funders | Funder number |
|---|---|
| Kausik Basu | |
| Saha Institute of Nuclear Physics | |
| National Science Foundation | PHY2011890, PHY1762495, IR/S2/PF-03/2003-II |
| Department of Science and Technology, Ministry of Science and Technology, India | DST/INSPIRE Fellowship/2020/IF200310 |
| Science and Engineering Research Board | CRG/2019/000556 |
| UGC-DAE Consortium for Scientific Research, University Grants Commission | |
| Inter-University Accelerator Centre |