- Page 1 and 2:
Copyright by Gabriel Noam Price 200
- Page 3 and 4:
Single-Photon Atomic Cooling by Gab
- Page 5 and 6:
Acknowledgments First, I would like
- Page 7 and 8:
Rubidium group when I first joined.
- Page 9 and 10:
Single-Photon Atomic Cooling Public
- Page 11 and 12:
2.5.2.4 Magneto-Optical Trap . . .
- Page 13 and 14:
List of Tables 2.1 87 Rb Physical P
- Page 15 and 16:
3.1 Vacuum Chamber . . . . . . . .
- Page 17 and 18:
Chapter 1 Introduction This chapter
- Page 19 and 20:
the momentum kicks due to absorptio
- Page 21 and 22:
samples by allowing for very long i
- Page 23 and 24:
Figure 1.2: The energy level struct
- Page 25 and 26:
quency regime [19]. This then led t
- Page 27 and 28:
Figure 1.4: Depiction of a simple,
- Page 29 and 30:
demonstrates the cooling power of a
- Page 31 and 32:
a) b) c) external potential one-way
- Page 33 and 34:
worked on by Brillouin [27-29], ide
- Page 35 and 36:
the atomic ensemble. Not surprising
- Page 37 and 38:
are untrappable. The SI unit for en
- Page 39 and 40:
the atomic transition and is called
- Page 41 and 42:
2.1 Rubidium Rubidium (Rb) is an al
- Page 43 and 44:
constant which is given by α = e2
- Page 45 and 46:
only one value of J is possible fro
- Page 47 and 48:
the latter of which only applies to
- Page 49 and 50:
Figure 2.1: 87 Rb D2 Transition Hyp
- Page 51 and 52:
Pluging Eq. 2.18 into this Hamilton
- Page 53 and 54:
Following the same logic leads to a
- Page 55 and 56:
gF = −1/2 using the approximate e
- Page 57 and 58:
mize their energy in high magnetic
- Page 59 and 60:
If we now consider the field from t
- Page 61 and 62:
where P is in torr. The lifetime of
- Page 63 and 64:
component of the dipole oscillation
- Page 65 and 66:
maxima. Our experiment makes extens
- Page 67 and 68:
atoms its wavefunction Ψ(t) is typ
- Page 69 and 70:
In this equation we let H = H0 + Hc
- Page 71 and 72:
The significance of Isat is that at
- Page 73 and 74:
Δ ω =ω−Δ ω =ω−Δ Δ
- Page 75 and 76:
where I/Isat ≪ 1 has been assumed
- Page 77 and 78:
λ λ Figure 2.9: The Sisyphus cool
- Page 79 and 80: process repeats. If however, it dec
- Page 81 and 82: σ σ σ Figure 2.10: Geomet
- Page 83 and 84: to vary linearly with position alon
- Page 85 and 86: 0, ±1 and ∆mF = 0, ±1, allow ex
- Page 87 and 88: this figure only the relevant hyper
- Page 89 and 90: D2 transition in 87 Rb has a natura
- Page 91 and 92: 2.7.2 Saturation Absorption Spectro
- Page 93 and 94: ground state depletion due to the p
- Page 95 and 96: oadened background can be removed f
- Page 97 and 98: where n is the number density of at
- Page 99 and 100: where σ 2 c = σ 2 2 kBTt n + m .
- Page 101 and 102: Chapter 3 Experimental Apparatus Th
- Page 103 and 104: Figure 3.1: The vacuum chamber duri
- Page 105 and 106: Nor-Cal Products Inc. (AMV-1502-CF)
- Page 107 and 108: and monitor the necessary vacuum le
- Page 109 and 110: 3.1.3 Lower Chamber The lower chamb
- Page 111 and 112: a) top ridge 1 cm b) metal jacket h
- Page 113 and 114: to the appropriate frequency throug
- Page 115 and 116: plexiglass cover piezo U stack grat
- Page 117 and 118: λ Figure 3
- Page 119 and 120: Voltage a b c d e f Frequency Figur
- Page 121 and 122: eams. For example the MOT and optic
- Page 123 and 124: λ Figure 3.12: The slave lasers
- Page 125 and 126: λ λ λ
- Page 127 and 128: λ λ λ λ
- Page 129: needed when forming a MOT or optica
- Page 133 and 134: λ λ
- Page 135 and 136: Output Power > 10 W Wavelength 532
- Page 137 and 138: labeled 1, 2 and 3 in the Fig. 3.21
- Page 139 and 140: λ λ λ λ
- 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 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 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