Coexisting single-particle and collective excitations in As70

R. A. Haring-Kaye, R. M. Elder, J. Döring, S. L. Tabor, A. Volya, P. R. P. Allegro, P. C. Bender, N. H. Medina, S. I. Morrow, J. R. B. Oliviera, and V. Tripathi
Phys. Rev. C 92, 044325 – Published 26 October 2015

Abstract

High-spin states in As70 were studied using the Mn55(O18,3n) fusion-evaporation reaction at a beam energy of 50 MeV. Prompt γγ coincidences were measured using the Florida State University Compton-suppressed Ge array consisting of three Clover detectors and seven single-crystal detectors. A reinvestigation of the known level scheme resulted in the addition of 32 new transitions and the rearrangement of 10 others. The high-spin decay pattern of yrast negative-parity states was modified and enhanced extensively. Spins were assigned based on directional correlation of oriented nuclei ratios. Lifetimes of seven excited states were measured using the Doppler-shift attenuation method. The B(E2) rates inferred from the lifetimes of states in the yrast positive-parity band imply substantial collectivity, in agreement with the results of previous studies. Substantial signature splitting and large alternations in the B(M1) strengths were observed in this band as well, supporting the interpretation of an aligned πg9/2νg9/2 intrinsic configuration for this structure beginning at the lowest 9+ state. Large-scale shell-model calculations performed for As70 reproduce the relative energy differences between adjacent levels and the B(M1) rates in the yrast positive-parity band rather well, but underestimate the B(E2) strengths. The g9/2 orbital occupancies for the lowest 9+ state predicted by the shell-model calculations provide additional evidence of a stretched πg9/2νg9/2 configuration for this state.

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  • Received 3 September 2015
  • Revised 21 September 2015

DOI:https://doi.org/10.1103/PhysRevC.92.044325

©2015 American Physical Society

Authors & Affiliations

R. A. Haring-Kaye1, R. M. Elder1, J. Döring2, S. L. Tabor3, A. Volya3, P. R. P. Allegro4, P. C. Bender3, N. H. Medina4, S. I. Morrow5, J. R. B. Oliviera4, and V. Tripathi3

  • 1Department of Physics and Astronomy, Ohio Wesleyan University, Delaware, Ohio 43015, USA
  • 2Bundesamt für Strahlenschutz, D-10318 Berlin, Germany
  • 3Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
  • 4Instituto de Física, Universidade de São Paulo, São Paulo, 05508-090 Brazil
  • 5Department of Physics, Houghton College, Houghton, New York 14744, USA

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Issue

Vol. 92, Iss. 4 — October 2015

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