ATOMIC AND MOLECULAR PHYSICS |
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Cooling and Trapping 88Sr Atoms with 461nm Laser |
WANG Shao-Kai, WANG Qiang, LIN Yi-Ge, WANG Min-Ming, LIN Bai-Ke, ZANG Er-Jun, LI Tian-Chu, FANG Zhan-Jun |
National Institute of Metrology, Beijing 100013 |
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Cite this article: |
WANG Shao-Kai, WANG Qiang, LIN Yi-Ge et al 2009 Chin. Phys. Lett. 26 093202 |
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Abstract We report the experimental realization of a 88Sr magneto-optical trap (MOT) operating at the wavelength of 461nm. The MOT is loaded via a 32cm long spin-flip type Zeeman slower which enhances the MOT population by a factor of 22. The total laser power available in our experiment is about 300mW. We have trapped 1.6×108 88Sr atoms with a 679nm and 707nm repumping laser. The two repumping lasers enhance the trap population and trap lifetime by factors of 11 and 7, respectively. The 88Sr cloud has a temperature of about 2.3mK, measured by recording the time evolution of the absorption signal.
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Keywords:
32.30.-r
37.10.De
37.10.Gh
95.55.Sh
42.60.Fc
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Received: 09 June 2009
Published: 28 August 2009
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PACS: |
32.30.-r
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(Atomic spectra?)
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37.10.De
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(Atom cooling methods)
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37.10.Gh
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(Atom traps and guides)
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95.55.Sh
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(Auxiliary and recording instruments; clocks and frequency standards)
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42.60.Fc
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(Modulation, tuning, and mode locking)
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[1] Xu X Y et al 2003 Phys. Rev. Lett. 90 193002 [2] Zhao P Y et al 2008 Chin. Phys. Lett. 25 3631 [3] Katori H et al 1999 Phys. Rev. Lett. 82 1116 [4] Udem T et al 2001 Phys. Rev. Lett. 86 4996 [5] Zinner G et al 2000 Phys. Rev. Lett. 85 2292 [6] Xu X Y et al 2003 J. Opt. Soc. Am. B 20 968 [7] Chaneliere T et al 2005 J. Opt. Soc. Am. B 221819 [8] Takamoto M, Hong F L, Higashi R and Katori H 2005 Nature 435 7040 [9] Wang S K, Zhang Y Y, Lin B K, Wang M M and Fang Z J 2008 Proceedings of the Conference on Precision ElectromagneticMeasurement (Broomfield, Colorado, USA 8--13 June 2008) p 316 [10] Loftus T H, Ido T, Boyd M M, Ludlow A D and Ye J 2004 Phys. Rev. A 70 063413 [11] Maruyama R 2003 PhD thesis (University ofWashington) [12] Xu X Y Loftus T H, Smith M J, Hall J L, Gallagher A andYe J 2002 Phys. Rev. A 66 011401 [13] Weiss D S et al 1989 J. Opt. Soc. Am. B 62072 [14] Dedman C J et al 2004 Rev. Sci. Instrum. 755136 [15] Wieman C E and Hollberg L 1991 Rev. Sci. Instrum. 62\,1 [16] Sorrentino Ferrari G, Poli N, Drullinger R and Tino G M2006 arXiv:physics. 0609133 |
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