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Volumn 62, Issue 2, 2000, Pages 4-

Multifrequency evaporative cooling to Bose-Einstein condensation in a high magnetic field

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EID: 85037248904     PISSN: 10502947     EISSN: 10941622     Source Type: Journal    
DOI: 10.1103/PhysRevA.62.021601     Document Type: Article
Times cited : (1)

References (20)
  • 16
    • 85037248708 scopus 로고    scopus 로고
    • Note, however, that in time-averaged orbiting potential traps the bias field often exceeds 10 G, and hindered cooling may play a role, specially when the atomic ground-state hyperfine splitting is relatively small, as in sodium, for example
    • Note, however, that in time-averaged orbiting potential traps the bias field often exceeds 10 G, and hindered cooling may play a role, specially when the atomic ground-state hyperfine splitting is relatively small, as in sodium, for example.
  • 18
    • 85037231209 scopus 로고    scopus 로고
    • The (Formula presented) state is a trapping state in this manifold because of the nonlinearity of the Zeeman effect
    • The (Formula presented) state is a trapping state in this manifold because of the nonlinearity of the Zeeman effect.
  • 19
    • 85037208281 scopus 로고    scopus 로고
    • This conclusion was corroborated by a calculation of the energies of the dressed states for a given set (Formula presented) From the calculated energy splitting (Formula presented) at the (Formula presented) level crossing, we used the two-level Landau-Zener probability that the atoms will follow an adiabatic transition. We verified that for small Rabi frequencies (i.e., small evaporation efficiency), as in our experiment, this three-photon transition is the most probable transition at any sideband detuning (Formula presented) This numerical calculation can be used to fit the experimental data. We can estimate the one-photon Rabi frequency (Formula presented) kHz
    • This conclusion was corroborated by a calculation of the energies of the dressed states for a given set (Formula presented) From the calculated energy splitting (Formula presented) at the (Formula presented) level crossing, we used the two-level Landau-Zener probability that the atoms will follow an adiabatic transition. We verified that for small Rabi frequencies (i.e., small evaporation efficiency), as in our experiment, this three-photon transition is the most probable transition at any sideband detuning (Formula presented) This numerical calculation can be used to fit the experimental data. We can estimate the one-photon Rabi frequency (Formula presented) kHz.


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