Single-Photon Atomic Cooling - Raizen Lab - The University of ...

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translating the magnetically trapped atoms toward the optical box (as in Fig. 4.13), which yields a kinetic energy distribution independent of translation endpoint, we abruptly turn on the optical box and depopulation beam for the data in Fig. 4.14. In this situation, many atoms now transit the optical box far from their classical turning points, and if captured they contribute to an increased kinetic energy distribution and rate of escape. Figure 4.14: Captured atom number as a function of loading time. Data are given for separations between the optical and magnetic trap centers of 800µm, (▲), 600µm (●), 400µm (■), and 200µm (▼). Error bars indicate statistical uncertainty, and dashed curves are drawn through the data points to guide the eye. The slopes are initially dominated by the loading rate into the optical box. After some time, the loading rate decreases due to the depletion of the magnetic trap, and the slopes become dominated by escape out of the box. We performed Monte-Carlo simulations of the dynamics in the mag- 154
netic trap and transfer into the optical box. Atom trajectories are propagated through phase-space, in which a subspace representing trapped states in the optical box has been defined. As atoms reach this subspace they are counted as trapped. These simulations show an inverse relationship between the loading rate and the separation between the magnetic trap and optical box centers in agreement with the experimental results. Of utmost importance to the utility of this cooling technique is its ability to compress phase-space. With the single-photon atomic cooling scheme described in this section, we extract 1.5 × 10 5 atoms at a temperature of 7 µK from the magnetic trap. We compare this with the number of atoms captured out of the magnetic trap without the depopulation beam. This is just a conservative dipole trap: atoms that are caught inside the box at low enough kinetic energy will be trapped, while all others will be lost. We measure a factor of 23 ± 3 increase in atom number using the single-photon atomic cooling method with nearly identical velocity distributions. We do not resolve the internal magnetic states in our measurement. The atoms in the magnetic trap are in the F = 2 manifold, but can be in the mF = 1 and mF = 2 magnetic sublevels. The atoms caught in the optical box are in the F = 1 manifold but can be in the mF = 1 and mF = 0 magnetic sublevels. The factor of 23 refers to atom number, not directly to phase space density. The increase in the latter would be a factor of 12 in the worst case scenario, if all the atoms in the magnetic trap were in the F = 2, mF = 2 state and the atoms in the dipole trap were equally distributed between the two magnetic 155
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Copyright by Gabriel Noam Price 200
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Single-Photon Atomic Cooling by Gab
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Acknowledgments First, I would like
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Rubidium group when I first joined.
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Single-Photon Atomic Cooling Public
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2.5.2.4 Magneto-Optical Trap . . .
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List of Tables 2.1 87 Rb Physical P
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3.1 Vacuum Chamber . . . . . . . .
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Chapter 1 Introduction This chapter
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the momentum kicks due to absorptio
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samples by allowing for very long i
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Figure 1.2: The energy level struct
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quency regime [19]. This then led t
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Figure 1.4: Depiction of a simple,
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demonstrates the cooling power of a
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a) b) c) external potential one-way
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worked on by Brillouin [27-29], ide
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the atomic ensemble. Not surprising
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are untrappable. The SI unit for en
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the atomic transition and is called
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2.1 Rubidium Rubidium (Rb) is an al
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constant which is given by α = e2
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only one value of J is possible fro
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the latter of which only applies to
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Figure 2.1: 87 Rb D2 Transition Hyp
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Pluging Eq. 2.18 into this Hamilton
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Following the same logic leads to a
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gF = −1/2 using the approximate e
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mize their energy in high magnetic
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If we now consider the field from t
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where P is in torr. The lifetime of
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component of the dipole oscillation
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maxima. Our experiment makes extens
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atoms its wavefunction Ψ(t) is typ
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In this equation we let H = H0 + Hc
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The significance of Isat is that at
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Δ ω =ω−Δ ω =ω−Δ Δ
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where I/Isat ≪ 1 has been assumed
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λ λ Figure 2.9: The Sisyphus cool
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process repeats. If however, it dec
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σ σ σ Figure 2.10: Geomet
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to vary linearly with position alon
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0, ±1 and ∆mF = 0, ±1, allow ex
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this figure only the relevant hyper
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D2 transition in 87 Rb has a natura
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2.7.2 Saturation Absorption Spectro
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ground state depletion due to the p
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oadened background can be removed f
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where n is the number density of at
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where σ 2 c = σ 2 2 kBTt n + m .
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Chapter 3 Experimental Apparatus Th
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Figure 3.1: The vacuum chamber duri
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Nor-Cal Products Inc. (AMV-1502-CF)
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and monitor the necessary vacuum le
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3.1.3 Lower Chamber The lower chamb
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a) top ridge 1 cm b) metal jacket h
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to the appropriate frequency throug
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plexiglass cover piezo U stack grat
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λ Figure 3
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Page 121 and 122: eams. For example the MOT and optic
Page 123 and 124: λ Figure 3.12: The slave lasers
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Page 129 and 130: needed when forming a MOT or optica
Page 131 and 132: master laser is dithered at 20 kHz.
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Page 135 and 136: Output Power > 10 W Wavelength 532
Page 137 and 138: labeled 1, 2 and 3 in the Fig. 3.21
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Page 141 and 142: process. The two coils are arranged
Page 143 and 144: 19) connected in parallel. This arr
Page 145 and 146: 3.4.2 Horizontal Imaging The horizo
Page 147 and 148: Chapter 4 Single-Photon Atomic Cool
Page 149 and 150: 1 s, after which time ∼ 10 8 87 R
Page 151 and 152: (a) x z magnetically trapped atoms
Page 153 and 154: h x z magnetically trapped atoms y
Page 155 and 156: z y x magnetically trapped atoms cr
Page 157 and 158: Figure 4.5: The effective potential
Page 159 and 160: depopulation present and it indicat
Page 161 and 162: numbers sufficiently large to quant
Page 163 and 164: μ μ μ
Page 165 and 166: the potential landscape due to the
Page 167 and 168: Figure 4.12: The number of atoms lo
Page 169: Figure 4.13: Incremental atom captu
Page 173 and 174: temperature TB of atoms loaded into
Page 175 and 176: used to construct it into the remai
Page 177 and 178: μ μ μ Figure 4.18: Side view of
Page 179 and 180: Figure 4.20: Geometry of the optica
Page 181 and 182: could potentially have undergone th
Page 183 and 184: detunings. The result of scattering
Page 185 and 186: are switched off causing non-optica
Page 187 and 188: Figure 4.25: Number (■) and tempe
Page 189 and 190: traps. If we model the ensembles in
Page 191 and 192: Figure 4.26: Radius of the atomic c
Page 193 and 194: atoms were removed from the magneti
Page 195 and 196: trappable |F = 1,mF = −1〉 state
Page 197 and 198: the short lived 2p state. Atoms whi
Page 199 and 200: Bibliography [1] R. Frisch, “Expe
Page 201 and 202: [15] C. C. Bradley, C. A. Sackett,
Page 203 and 204: [31] E.T. Jaynes, “Information th
Page 205 and 206: [49] J. Ye, S. Swartz, P. Jungner,
Page 207 and 208: [66] J.P. Gordon and A. Ashkin, “
Page 209 and 210: [85] C.-S. Chuu, Direct Study of Qu
Page 211 and 212: adicals,” Phys. Rev. Lett. 94, 02
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