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the constant rate at which atoms are depopulated from the magnetic trap, the Figure 4.29: Atom accumulation in the optical trough as a function of the current in the quadrupole coils. Vertical lines indicate the point at which the magnetic field gradient produced by the current is no longer sufficient to levitate atoms against gravity for atoms in the mF = 1 and mF = 2 magnetic substates. loading rate into the optical trough is clearly non-linear. This graph indicates that atoms are more efficiently loaded at the end of the cooling sequence, when the magnetic field gradient is low. This trend may be explained as follows. As the magnetic gradient is reduced, atoms in the magnetically anti-trapped |F = 1,mF = 1〉 state gain less energy as they travel from the depopulation beam to the optical trough vertex or walls. Therefore a smaller fraction of these atoms will have sufficient energy to push through the bottom or sides of the trough’s potential. Also, at lower magnetic field gradients the magnetically 178
trappable |F = 1,mF = −1〉 state is not levitated out of the optical trough and becomes trappable in the optical trough. Together, these effects result in an increased transfer efficiency. The maximum transfer efficiency we have measured is 2.2(3)%. How- ever, it is clear from Eq. 4.6 that this number can be trivialy increased by increasing the phase space overlap of the two traps. This could be accomplished by reducing the size and temperature of the magnetic trap or increasing the size and depth of the optical trough. It should also be noted that one can use Eq. 4.6 to find an expression for the increase in the phase-space density of a non-interacting ensemble undergoing this process: ρO ρB = σ(z) B σ (z) O T (z) B T (z) O . (4.8) For a fixed optical trough geometry and depth, this ratio increases with TB in spite of a corresponding decrease in transfer efficiency. With initial magnetic trap parameters TB = 53µK and σB = 515µm, we have transfered 3.3 × 10 5 atoms at a temperature of 4.3µK with 0.3% transfer efficiency. This corresponds to a peak phase-space density of 4.9(3) × 10 −4 , which is roughly a 350-fold increase over the phase-space density of the magnetic trap. 4.5 Future Directions The power of the single-photon cooling technique will only be fully demonstrated when it has been successfully applied to a species not amenable 179
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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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Voltage a b c d e f Frequency Figur
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eams. For example the MOT and optic
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λ Figure 3.12: The slave lasers
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λ λ λ
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λ λ λ λ
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needed when forming a MOT or optica
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master laser is dithered at 20 kHz.
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λ λ
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Output Power > 10 W Wavelength 532
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labeled 1, 2 and 3 in the Fig. 3.21
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λ λ λ λ
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process. The two coils are arranged
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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 and 170: Figure 4.13: Incremental atom captu
Page 171 and 172: netic trap and transfer into the op
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: atoms were removed from the magneti
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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