High spin spectroscopy and shape coexistence in As73

M. Kumar Raju, P. V. Madhusudhana Rao, S. K. Tandel, P. Sugathan, R. P. Singh, S. Muralithar, T. Seshi Reddy, B. V. Thirumala Rao, Jie Meng, Shuangquan Zhang, Jian Li, Q. B. Chen, Bin Qi, and R. K. Bhowmik
Phys. Rev. C 92, 064324 – Published 29 December 2015

Abstract

High spin states in As73 have been investigated through the fusion-evaporation reaction Ni64(C12,p2n)As73 with an incident beam energy of 55 MeV. The level scheme has been extended up to Jπ=(37/2) and excitation energy 8.7 MeV with the addition of 30 new γ-ray transitions. The microscopic origins of the observed positive- and negative-parity band structures are discussed in the context of the particle rotor model. Nucleon alignments and shape evolution with increasing angular momentum are discussed in the framework of the cranked shell model and relativistic mean-field calculations. The results offer insight into the nature of the observed band structures and indicate prolate-oblate shape coexistence between positive- and negative-parity bands at low spin.

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  • Received 29 September 2015

DOI:https://doi.org/10.1103/PhysRevC.92.064324

©2015 American Physical Society

Authors & Affiliations

M. Kumar Raju1,2,*, P. V. Madhusudhana Rao1, S. K. Tandel3, P. Sugathan1,4, R. P. Singh4, S. Muralithar4, T. Seshi Reddy1, B. V. Thirumala Rao1, Jie Meng5, Shuangquan Zhang5, Jian Li5, Q. B. Chen5, Bin Qi6, and R. K. Bhowmik4

  • 1Nuclear Physics Department, Andhra University, Visakhapatnam 530003, India
  • 2Department of Physics, University of the Western Cape, P/B X17, Bellville ZA-7535, South Africa
  • 3UM-DAE Centre for Excellence in Basic Sciences, Mumbai 400098, India
  • 4Inter-University Accelerator Centre, Aruna Asaf Ali Marg, New Delhi 110067, India
  • 5School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
  • 6School of Space Science and Physics, Shandong University at Weihai, 264209 Weihai, China

  • *kumar8284@gmail.com

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Vol. 92, Iss. 6 — December 2015

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