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Chinese Physics C> 2015, Vol. 39> Issue(5) : 054105 DOI: 10.1088/1674-1137/39/5/054105

Wobbling geometry in a simple triaxial rotor

  • The spectroscopic properties and angular momentum geometry of the wobbling motion of a simple triaxial rotor are investigated within the triaxial rotor model. The obtained exact solutions of energy spectra and reduced quadrupole transition probabilities are compared to the approximate analytic solutions from the harmonic approximation formula and Holstein-Primakoff formula. It is found that the low lying wobbling bands can be well described by the analytic formulae. The evolution of the angular momentum geometry as well as the K-distribution with respect to the rotation and the wobbling phonon excitation are studied in detail. It is demonstrated that with the increase of the wobbling phonon number, the triaxial rotor changes its wobbling motions along the axis with the largest moment of inertia to the axis with the smallest moment of inertia. In this process, a specific evolutionary track that can be used to depict the motion of a triaxial rotating nucleus is proposed.
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    [1] Bohr A, Mottelson B R. Nuclear Structure, Vol. II, Benjamin, New York, 1975[2] Frauendorf S, Meng J. Nucl. Phys. A, 1997, 617: 131[3] Frauendorf S. Rev. Mod. Phys., 2001, 73: 463[4] MENG J, ZHANG S Q. J. Phys. G: Nucl. Part. Phys., 2010, 37: 064025[5] degrd S W, Hagemann G B, Jensen D R, Bergstrm M, Herskind B, Sletten G, Trmnen S, Wilson J N, Tjm P O, Hamamoto I et al. Phys. Rev. Lett., 2001, 86: 5866[6] Jensen D R, Hagemann G B, Hamamoto I, degrd S W, Herskind B, Sletten G, Wilson J N, Spohr K, Hübel H, Bringel P et al. Phys. Rev. Lett., 2002, 89: 142503[7] Jensen D R, Hagemann G B, Hamamoto I, degrd S W, Bergstrom M, Herskind B, Sletten G, Tormanen S, Wilson J N, Tjom P O et al. Nucl. Phys. A, 2002, 703: 3[8] Schnwaer G, Hübel H, Hagemann G B, Bednarczyk P, Benzoni G, Bracco A, Bringel P, Chapman R, Curien D, Domscheit J et al. Phys. Lett. B, 2003, 552: 9[9] Amro H, MA W C, Hagemann G B, Diamond R M, Domscheit J, Fallon P, Gorgen A, Herskind B, Hubel H, Jensen D R et al. Phys. Lett. B, 2003, 553: 197[10] Hagemann G B. Eur. Phys. J. A, 2004, 20: 183[11] Bringel P, Hagemann G, Hübel H, Al-khatib A, Bednarczyk P, Bürger A, Curien D, Gangopadhyay G, Herskind B, Jensen D et al. Eur. Phys. J. A, 2005, 24: 167[12] Hartley D J, Janssens R V F, Riedinger L L, Riley M A, Aguilar A, Carpenter M P, Chiara C J, Chowdhury P, Darby I G, Garg U et al. Phys. Rev. C, 2009, 80: 041304[13] ZHU S J, LUO Y X, Hamilton J H, Ramayya A V, CHE X L, JIANG Z, Hwang J K, Wood J L, Stoyer M A, Donangelo R et al. Int. J. Mod. Phys. E, 2009, 18: 1717[14] Hamamoto I. Phys. Rev. C, 2002, 65: 044305[15] Hamamoto I, Mottelson B R. Phys. Rev. C, 2003, 68: 034312[16] Frauendorf S, Dnau F. Phys. Rev. C, 2014, 89: 014322[17] Shimizu Y R, Matsuzaki M. Nucl. Phys. A, 1995, 588: 559[18] Matsuzaki M, Shimizu Y R, Matsuyanagi K. Phys. Rev. C, 2002, 65: 041303[19] Matsuzaki M, Shimizu Y R, Matsuyanagi K. Eur. Phys. J. A, 2003, 20: 189[20] Matsuzaki M, Shimizu Y R, Matsuyanagi K. Phys. Rev. C, 2004, 69: 034325[21] Matsuzaki M, Ohtsubo S. Phys. Rev. C, 2004, 69: 064317[22] Shimizu Y R, Matsuzaki M, Matsuyanagi K. Phys. Rev. C, 2005, 72: 014306[23] Shimizu Y R, Shoji T, Matsuzaki M. Phys. Rev. C, 2008, 77: 024319[24] Shoji T, Shimizu Y R. Progr. Theor. Phys., 2009, 121: 319[25] Oi M, Ansari A, Horibata T, Onishi N. Phys. Lett. B, 2000, 480: 53[26] CHEN Q B, ZHANG S Q, ZHAO P W, MENG J. Phys. Rev. C, 2014, 90: 044306[27] Tanabe K, Sugawara-Tanabe K. Phys. Lett. B, 1971, 34: 575[28] Tanabe K, Sugawara-Tanabe K. Phys. Rev. C, 2006, 73: 034305[29] Tanabe K, Sugawara-Tanabe K. Phys. Rev. C, 2008, 77: 064318[30] Davydov A, Filippov G. Nuclear Physics, 1958, 8: 237[31] ZENG J Y. Quantume Mechanics, Vol. II. Beijing: Science Press, 2007 (in Chinese)[32] Holstein T, Primakoff H. Phys. Rev., 1940, 58: 1098[33] Oi M, Fletcher J. J. Phys. G, 2005, 31: S1753[34] Oi M. Phys. Lett. B, 2006, 634: 30[35] Sugawara-Tanabe K, Tanabe K, Yoshinaga N. Prog. Theor. Exp. Phys., 2014, 063D01[36] QI B, ZHANG S Q, MENG J, WANG S Y, Frauendorf S. Phys. Lett. B, 2009, 675: 175[37] QI B, ZHANG S Q, WANG S Y, YAO J M, MENG J. Phys. Rev. C, 2009, 79: 041302(R)[38] CHEN Q B, YAO J M, ZHANG S Q, QI B. Phys. Rev. C, 2010, 82: 067302[39] QI B, ZHANG S Q, WANG S Y, MENG J, Koike T. Phys. Rev. C, 2011, 83: 034303

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SHI Wen-Xian and CHEN Qi-Bo. Wobbling geometry in a simple triaxial rotor[J]. Chinese Physics C, 2015, 39(5): 054105. doi: 10.1088/1674-1137/39/5/054105
SHI Wen-Xian and CHEN Qi-Bo. Wobbling geometry in a simple triaxial rotor[J]. Chinese Physics C, 2015, 39(5): 054105.  doi: 10.1088/1674-1137/39/5/054105 shu
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Received: 2014-11-17
Revised: 1900-01-01
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Wobbling geometry in a simple triaxial rotor

    Corresponding author: CHEN Qi-Bo,
  • Received Date: 2014-11-17
  • Accepted Date: 1900-01-01
  • Available Online: 2015-05-05

Abstract: The spectroscopic properties and angular momentum geometry of the wobbling motion of a simple triaxial rotor are investigated within the triaxial rotor model. The obtained exact solutions of energy spectra and reduced quadrupole transition probabilities are compared to the approximate analytic solutions from the harmonic approximation formula and Holstein-Primakoff formula. It is found that the low lying wobbling bands can be well described by the analytic formulae. The evolution of the angular momentum geometry as well as the K-distribution with respect to the rotation and the wobbling phonon excitation are studied in detail. It is demonstrated that with the increase of the wobbling phonon number, the triaxial rotor changes its wobbling motions along the axis with the largest moment of inertia to the axis with the smallest moment of inertia. In this process, a specific evolutionary track that can be used to depict the motion of a triaxial rotating nucleus is proposed.

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