Evidence of antimagnetic rotational motion in Pd 103

A. Sharma, R. Raut, S. Muralithar, R. P. Singh, S. S. Bhattacharjee, S. Das, S. Samanta, S. S. Ghugre, R. Palit, S. Jehangir, N. Rather, G. H. Bhat, J. A. Sheikh, S. S. Tiwary, Neelam, P. V. Madhusudhana Rao, U. Garg, S. K. Dhiman

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12 Scopus citations

Abstract

Lifetime measurements have been carried out for the levels of the negative parity yrast sequence in Pd103 nucleus using the Doppler shift attenuation method. The levels were populated via Zr94(C13, 4nγ)Pd103 fusion-evaporation reaction at a beam energy of 55 MeV. De-exciting γ rays were detected by utilizing the Indian National Gamma Array. The extracted transition probabilities and other auxiliary observations indicate that the sequence may be resulting from the antimagnetic rotational (AMR) motion of valence nucleons. The key characteristic feature of the AMR motion is the steady decrease of the B(E2) transition probability with spin, which is seen in the present measured transitions for Pd103. The experimental results are compared with the theoretical predictions of tilted axis cranked approach based on the covariant density functional theory. It is noted that the properties of the AMR band structure for Pd103 predicted in this model analysis are in good agreement with the present experimental findings. Further, semi-classical particle-rotor model has been employed to substantiate the AMR interpretation of the observed band structure in Pd103 and it is shown that results are similar to the band structures observed in the neighboring isotopes, which have also been considered as candidates for AMR motion.

Original languageEnglish
Article number024324
JournalPhysical Review C
Volume103
Issue number2
DOIs
StatePublished - Feb 2021
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2021 American Physical Society.

Funding

The authors would like to thank the technical staff of IUAC pelletron facility for delivering a stable beam during the experiment. We acknowledge the INGA Collaboration, UGC and DST for providing support under INGA Project No. (IR/S2/PF-03/2003/I). We would also like to thank our colleagues Ritika Garg, Gurmeet Kumar, M. Idrees, Vishnu Jyoti, and Indu Bala for their help during the experiment. Valuable suggestions and support received during analysis from Himanshu K. Singh (IIT, Bombay) and Sutanu Bhattacharya (GGV, Bilaspur) are highly appreciated. Discussions with Dr. B. Qi and Dr. H. Jia (Shandong University) of their TAC-CDFT results on AMR in this nucleus are gratefully acknowledged. A.S. is grateful to the Inter University Accelerator Centre, New Delhi for financial support through UFR No. 62316. U.G. acknowledges the support by the US National Science Foundation (Grant Nos. PHY-1419765 and PHY-1713857) for this work. R.P. acknowledges the support from the Department of Atomic Energy, Government of India (Project Identification Code 12-R&D-TFR-5.02-0200). Authors (G.H.B., N.R., and J.A.S.) would like to acknowledge Science and Engineering Research Board, Department of Science and Technology, Govt. of India for providing financial support under Project No. CRG/2019/004960 to carry out a part of the research work. N.R. also acknowledges University Grant Commission for the Start-Up grant with letter No. F.30-498/2019(BSR), dated 18-05-2019.

FundersFunder number
National Science FoundationPHY-1713857, PHY-1419765
Department of Science and Technology, Ministry of Science and Technology, IndiaIR/S2/PF-03/2003/I
University Grants Commission18-05-2019, F.30-498/2019
Department of Atomic Energy, Government of IndiaD-TFR-5.02-0200, CRG/2019/004960
University Grants Committee
Université François-Rabelais62316
Inter-University Accelerator Centre

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