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Strong population of a superdeformed band in {sup 142}Eu

Journal Article · · Physical Review, C
; ; ; ;  [1]; ;  [2]; ; ; ; ;  [3]; ; ;  [4];  [5]
  1. Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, L8S 4M1 (Canada)
  2. Department of Mathematical Physics, Lund Institute of Technology, P. O. Box 118, S-221 00 Lund (Sweden)
  3. AECL, Chalk River Laboratories, Chalk River, Ontario, K0J 1J0 (Canada)
  4. Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7 (Canada)
  5. Department of Physics, University of Ottawa, Ottawa, Ontario, K1N 6N5 (Canada)

A superdeformed band has been found in {sup 142}Eu. It is populated with 1.2(2)% of the total {gamma}-ray intensity that decayed into {sup 142}Eu via the reaction {sup 120}Sn({sup 27}Al,5{ital n}){sup 142}Eu at 152 MeV. The strength of the band is similar to that previously reported in {sup 143}Eu, where the superdeformed band is populated with an intensity of 1.1(1)%. This is unexpected, since both total Routhian surface (TRS) and cranked modified oscillator (MO) calculations predict that the superdeformed band in {sup 143}Eu becomes yrast at lower spin than that in {sup 142}Eu. This difference is {similar_to}4{h_bar} in the MO calculations and {similar_to}8{h_bar} in the TRS. Extrapolation of the ``normal``-deformed yrast states in {sup 143}Eu shows, however, that a difference of {similar_to}8{h_bar} in spin corresponds to a change in the relative energy of the superdeformed and normal-deformed yrast lines of only {similar_to}1 MeV.

OSTI ID:
69512
Journal Information:
Physical Review, C, Journal Name: Physical Review, C Journal Issue: 1 Vol. 52; ISSN PRVCAN; ISSN 0556-2813
Country of Publication:
United States
Language:
English

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