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The spin evolution of spin-3 ^(52)Cr Bose-Einstein condensate

The spin evolution of spin-3 ^(52)Cr Bose-Einstein condensate
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摘要 This paper studies theoretically the spin evolution of a Bose-Einstein condensate starting from a mixture of two or three groups of 52Cr (spin-3) atoms in an optical trap. The initial state is so chosen that the condensate has total magnetization zero so that the system does not distinguish up and down. It is assumed that the system is very dilute (particle number is very small), the temperature is very low, and the frequency of the harmonic trap is large enough. In these situations, the deviation caused by the neglect of the dipole-dipole interaction and by using the single-mode approximation is reduced. A theoretical calculation beyond the mean field theory is performed and the numerical results are helpful for the evaluation of the unknown strength go. This paper studies theoretically the spin evolution of a Bose-Einstein condensate starting from a mixture of two or three groups of 52Cr (spin-3) atoms in an optical trap. The initial state is so chosen that the condensate has total magnetization zero so that the system does not distinguish up and down. It is assumed that the system is very dilute (particle number is very small), the temperature is very low, and the frequency of the harmonic trap is large enough. In these situations, the deviation caused by the neglect of the dipole-dipole interaction and by using the single-mode approximation is reduced. A theoretical calculation beyond the mean field theory is performed and the numerical results are helpful for the evaluation of the unknown strength go.
出处 《Chinese Physics B》 SCIE EI CAS CSCD 2011年第1期157-164,共8页 中国物理B(英文版)
基金 Project supported by the National Natural Science Foundation of China(Grant Nos.10874249 and 11075223)
关键词 Bose-Einstein condensate spin evolution short-ranged interaction strength Bose-Einstein condensate, spin evolution, short-ranged interaction strength
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  • 1Ho T L 1998 Phys. Rev. Lett. 81 742.
  • 2Ohmi T and Machida K 1998 J. Phys. Soc. Jpn. 67 1822.
  • 3Stamper-Kurn D M, Andrews M R, Chikkatur A P, Inouye S, Miesner H J, Stenger J and Ketterle W 1998 Phys. Rev. Lett. 80 2027.
  • 4Stenger J, Inouye S, Stamper-Kurn D M, Miesner H J, Chikkatur A P and Ketterle W 1998 Nature (London) 396 345.
  • 5Law C K, Pu H and Bigelow N P 1998 Phys. Rev. Lett. 81 5257.
  • 6G"orlitz A, Gustavson T L, Leanhardt A E, Low R, Chikkatur A P, Gupta S, Inouye S, Pritchard D E and Ketterle W 2003 Phys. Rev. Lett. 90 090401.
  • 7Lewenstein M, Sanpera A, Ahufinger V, Damski B, Sen De A and Sen U 2007 Adv. Phys. 56 243.
  • 8Han J R, Liu X F and Wang Y J 2009 Chin. Phys. B 18 5301.
  • 9Griesmaier A, Werner J, Hensler S, Stuhler J and Pfau T 2005 Phys. Rev. Lett. 94 160401.
  • 10Diener R B and Ho T L 2006 Phys. Rev. Lett. 96 190405.

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