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Volumn 74, Issue 17, 1995, Pages 3352-3355

Stable, tightly confining magnetic trap for evaporative cooling of neutral atoms

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Indexed keywords


EID: 11944272373     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.74.3352     Document Type: Article
Times cited : (482)

References (19)
  • 16
    • 84927501227 scopus 로고    scopus 로고
    • Variations across the cloud in the phase and amplitude of the small-amplitude circular motion, coupled with the secular motion of atoms through the cloud, will give rise to a very small viscous heating associated with each intra-trap collision. The scale of the velocity variation across the cloud is given by the ratio of the size of the cloud to the radius of the hole orbit, times the speed of the circular motion. As an atom moves across the cloud, there is a small amount of hysteresis, whose fractional scale is given by the trap frequency over the field rotation frequency, such that when short-range pairwise collisions take place the collision velocity will have an additive term of order δvcirc=(ωt/ωb)(l/R0)μBq′/mωb. This extra velocity, which gives rise to viscous heating, is for the present TOP parameters very small compared to (for instance) the zero-point motion of a hypothetical Bose condensate confined in the TOP trap.
  • 18
    • 84927494888 scopus 로고    scopus 로고
    • There are limits to the amount the bias field may be safely reduced. As the bias field is lowered, the oscillation frequencies in the TOP will no longer be much smaller than ωb, calling into question the validity of time averaging the potential. Furthermore, for very low bias fields the Larmor frequency will no longer be much larger than ωb, and the possibility of nonadiabatic flip loss is resurrected.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.