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Chinese Physics C> 2006, Vol. 30> Issue(S2) : 81-83 

Rotational Structures of Neutron Deficient Isotopes 125,127,129Ce

  •  China Institute of Atomic Energy, Beijing 102413, China

  • The configuration-dependent cranked Nilsson-Strutinsky approach has been used to investigate rotational structures of neutron deficient isotopes 125,127,129Ce. Signature splitting and deformation of yrast bands have been discussed. Shape coexistence may exist in 127,129Ce. The signature splitting of yrast bands for Ce isotopes is strongly dependent on occupied orbitals because of slight triaxial deformation.
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    [1] . Smith J F et al. Phys. Rev., 2004, C69: 0343392. Petrache C M et al. Eur. Phys. J., 2002, A14: 4393. Nyako B M et al. Z. Phys., 1989, A334: 5134. Galindo-Uribarri A et al. Phys. Rev., 1996, C54: R4545. Zeidan O et al. Phys. Rev., 2002, C65: 0243036. Bengtsson T, Ragnarsson I. Nucl. Phys., 1985, A436: 147. Afanasjev A V, Ragnarsson I. Nucl. Phys., 1995, A591:3878. Afanasjev A V et al. Phys. Rep., 1999, 322: 19. Hartley D J et al. Phys. Rev., 2000, C61: 04432810. Dong B G et al. Phys. Rev., 2006, C74: 014308

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MA Hai-Liang and DONG Bao-Guo. Rotational Structures of Neutron Deficient Isotopes 125,127,129Ce[J]. Chinese Physics C, 2006, 30(S2): 81-83.
MA Hai-Liang and DONG Bao-Guo. Rotational Structures of Neutron Deficient Isotopes 125,127,129Ce[J]. Chinese Physics C, 2006, 30(S2): 81-83. shu
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Received: 2006-10-13
Revised: 1900-01-01
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Rotational Structures of Neutron Deficient Isotopes 125,127,129Ce

    Corresponding author: MA Hai-Liang,
  • China Institute of Atomic Energy, Beijing 102413, China
  • Received Date: 2006-10-13
  • Accepted Date: 1900-01-01
  • Available Online: 2006-01-03

Abstract: The configuration-dependent cranked Nilsson-Strutinsky approach has been used to investigate rotational structures of neutron deficient isotopes 125,127,129Ce. Signature splitting and deformation of yrast bands have been discussed. Shape coexistence may exist in 127,129Ce. The signature splitting of yrast bands for Ce isotopes is strongly dependent on occupied orbitals because of slight triaxial deformation.

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