SCOPUS 정보 검색 플랫폼

Volumn 74, Issue 8, 1995, Pages 1311-1314

Long atomic coherence times in an optical dipole trap

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Indexed keywords

EID: 3743121064 PISSN: 00319007 EISSN: None Source Type: Journal
DOI: 10.1103/PhysRevLett.74.1311 Document Type: Article

Times cited : (186)

References (22)

1
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- Laser-cooled Cs frequency standard and a measurement of the frequency shift due to ultracold collisions
- 63, 612, M. A. Kasevich, E. Riis, S. Chu, R. G. DeVoe, Phys. Rev. Lett., A. Clairon, C. Salomon, S. Guellati, W. D. Phillips, Europhys. Lett., 16, 165
- (1989) Physical Review Letters , vol.70 , pp. 1771
- Gibble, K.¹ Chu, S.²

3
- 84927491472
- IQEC'94 Technical Digest, Optical Society of America, Washington
- (1994) , vol.9
- Libbrecht, K.¹ Willems, P.A.²

4
- 0000224370
- For a review of experiments on the reflection of atoms from evanescent light fields, see
- (1994) Phys. Rep. , vol.240 , pp. 143
- Adams, C.S.¹ Sigel, M.² Mlynek, J.³

5
- 84975576500
- Normal-incidence reflection of slow atoms from an optical evanescent wave
- (1990) Optics Letters , vol.15 , pp. 607
- Kasevich, M.A.¹ Weiss, D.S.² Chu, S.³

13
- 84927500869
- Data on the pressure dependence of the lifetime of atoms in a far-off resonance dipole trap can be found in, C. E. Wieman, D. Wineland, AIP, New York
- Atomic Physics 14: Proceedings of the International Conference on Atomic Physics
- Lee, H.J.¹ Adams, C.S.² Davidson, N.³ Young, B.⁴ Weitz, M.⁵ Kasevich, M.⁶ Chu, S.⁷

14
- 0003867616
- Oxford Univ. Press, London
- (1956) Molecular Beams
- Ramsey, N.F.¹

15
- 84927507304
- In the simulations, the classical equations of motion were integrated for 104 atoms with initial Gaussian distributions in position and velocities (the rms position and velocity were 500 μm and 25 cm/sec, respectively). ∼500 atoms remain in the P=15 W trap after 1 s. Changing the initial rms values by ×2 and ×0.5 changed the distribution of the Stark shifts by less then 10% (although the number of remaining atoms changes significantly).

16
- 84927466492
- The fringe contrast is calculated by ∫cos[πT( f-δf)]N( f) df/∫N( f) df, where N( f) is the light shift distribution of Fig. 4, and δf is the frequency shift of the Ramsey fringe that is found by maximizing the contrast.

17
- 84927490300
- The beams have the same dimensions and intensities as in the two-beam trap.

20
- 0000101653
- This application has also been considered by
- (1994) Phys. Rev. A , vol.49 , pp. R4285
- Bijlsma, M.¹ Verhaar, B.J.² Heinzen, D.J.³

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