Experiments to Control Atom Number and Phase-Space Density in ...

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and thus to coat the viewports. Figure 7.29: Spectroscopy cell. lithium reservoir The spectroscopy cell is heated near the lithium reservoir with high-temperature heater tape. It is insulated using fiber glass. To avoid frequency shifts due to the presence of magnetic fields, the heater tape is wound around the cell in such a way as to minimize the resulting magnetic fields due to currents flowing through the tape. Except near the lithium reservoir the spectroscopy cell is kept near room temperature. Lithium atoms therefore stick to the walls of the cell, which reduces the risk of coating the viewports with lithium. The first time the lithium reservoir is heated to a temperature of about 450 ◦ C. This breaks any oxide layer that might have been formed on the surface of the lithium metal during the preparation and loading into the cell. 7.3.1.3 Frequency-Offset Lock Setups Frequency-offset locking has many applications in atomic physics experiments. Most importantly for the lithium setup, it is an easy method to lock the imaging diode laser and the master laser, used to seed the tapered amplifier, relative to the spectroscopy laser with a frequency offset ∆f. Using a tunable scheme, it is possible to dynamically change the laser frequency during the course of the experimental sequence. This is important especially for the master laser, where the frequency offset ∆f controls the MOT detuning. ∆f can then be changed to compress the MOT prior to loading atoms 121
into the CO2 laser. The optical layout for the frequency-offset lock is shown in figure 7.30. Fabry- Perot To Wavemeter f=25mm f=50mm f=200mm f=25mm 50:50 beam splitter cube ber coupler mirror spherical lens photodiode from Tapered Amplier Master Laser from Imaging Laser from Spectroscopy Laser polarizing bBeam splitter cube Figure 7.30: Optical layout of the frequency-offset lock optics. A 50:50 fixed ratio beamsplitter (Edmund Optics, NT49-005) distributes the spectroscopy laser into two beam paths. A second 50:50 fixed ratio beamsplitter cube then combines the spectroscopy laser with the imaging laser beam. An identical setup overlaps the spectroscopy laser with the master laser seeding the tapered amplifier. After the beams are combined, they are focused onto photodiodes that detect the interference signal between the spectroscopy and the imaging laser, and the spectroscopy and the master laser respectively. To create the interference signal, the polarizations of the beams have to be aligned. The remaining beam power from all three beams, spectroscopy, imaging and master, is then combined at a third 50:50 beamsplitter cube. The beam from one of the two output ports of this beam splitter is then coupled into the wavemeter using a multimode fiber. The second beam is coupled into a home-built Fabry-Perot cavity. 122
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Copyright by Kirsten Viering 2012
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Experiments to Control Atom Number
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Acknowledgments First of all, I wou
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Experiments to Control Atom Number
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Table of Contents Acknowledgments v
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Chapter 7. Lithium Apparatus 92 7.1
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List of Tables 2.1 Physical propert
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4.1 Vacuum chamber . . . . . . . .
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7.39 Future vertical axis optics .
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The development of techniques to la
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Ptorr 10 5 10 6 10 7 10 8 10 9 260
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Property Symbol Value Reference Ato
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2.3.2 Hyperfine Structure So far th
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The Wigner-Eckhart theorem can be u
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The total magnetic moment of an ato
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interaction. The shift in the energ
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(a) (b) scattering length a 0 Energ
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a laser field with frequency ω. Th
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Here ω0 is the resonance frequency
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Optical molasses do not provide a s
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J=1 J=0 -1 Δ σ + σ - σ - 0 +1 -
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phase-space density is defined as
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which maintains a constant η = U/k
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2.12.1 Saturated Absorption Spectro
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Figure 2.22: Saturation absorption
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Signal 0 Signal (a) (b) Signal Freq
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(a) (b) (c) (d) Figure 2.24: Absorp
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y more complex energy level structu
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ight side of the box. An irreversib
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time (a) (b) (c) Figure 3.3: Single
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them to move from B to A, but close
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Figure 4.1: Vacuum chamber. Photogr
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( ( Figure 4.3: Helicoflex seal. (a
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88 mm 4.2.3 Auxiliary Coils 62 mm Q
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5 2 P 3/2 5 2 S 1/2 384. 230 484 46
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distribution of the MOT master lase
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shifts. First a frequency shift of
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transition. However, the laser freq
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4.3.1.4 Upper MOT Horizontal Slave
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provides the beam for the upper MOT
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demon beam λ λ horizontal MOT bea
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scholar, Florian Schreck. It is wri
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Atoms are then optically pumped to
Page 87 and 88: ferred into the |F = 1,mF = 0〉 or
Page 89 and 90: 5.2 Branching Ratios and Population
Page 91 and 92: effect of the reflected beam at zer
Page 93 and 94: y the repulsive trough beams, gaini
Page 95 and 96: Figure 5.9: Atom number as a functi
Page 97 and 98: Figure 5.10: Radius of the magnetic
Page 99 and 100: on the collision rate of atoms insi
Page 101 and 102: ferred via the single-photon coolin
Page 103 and 104: By comparison an atomic Fock state
Page 105 and 106: of atoms in the two hyperfine groun
Page 107 and 108: difference in the lifetimes is dete
Page 109 and 110: Chapter 7 Lithium Apparatus Creatin
Page 111 and 112: angle valve rotary feedthrough ion
Page 113 and 114: an ion gauge controller (Granville
Page 115 and 116: viewports (MDC, 450002) are attache
Page 117 and 118: not trapped by the MOT impinge on t
Page 119 and 120: Should contamination of the vacuum
Page 121 and 122: Figure 7.12: The assembled Zeeman s
Page 123 and 124: 7.2.2 MOT Coils A second set of coi
Page 125 and 126: BGauss 250 200 150 100 50 30 20 10
Page 127 and 128: are required to create the high mag
Page 129 and 130: The coils are then checked for shor
Page 131 and 132: + B A Figure 7.23: Feshbach coil H-
Page 133 and 134: ensure that no particulates build u
Page 135 and 136: 118 Figure 7.26: Optical layout of
Page 137: The error signal shows three lines,
Page 141 and 142: Thorlabs PDA10A Coupler ZDC-10-1 to
Page 143 and 144: Imaging ber Imaging ber from Imagin
Page 145 and 146: Table 7.4 summarizes the beam power
Page 147 and 148: CO2 laser 40 MHz AOM f=2 in f=2 in
Page 149 and 150: 132 Figure 7.38: Optical layout aro
Page 151 and 152: Feshbach coil objective lenses atom
Page 153 and 154: MOT beams are no longer traveling a
Page 155 and 156: The second card (NI6733) offers eig
Page 157 and 158: Averaging over the magnetic subleve
Page 159 and 160: 2 2 P 3/2 D 2=670.977nm 2 2 S 1/2 m
Page 161 and 162: The right hand side of equation 7.1
Page 163 and 164: = E0 1 −n2 √2 exp σ0 ± iE0
Page 165 and 166: esidual potentials besides gravitat
Page 167 and 168: Figure 8.1: MOT loading. Typical lo
Page 169 and 170: A linear ramp typically changes the
Page 171 and 172: A typical MOT is density-limited at
Page 173 and 174: ubidium [113-115] and cesium[116].
Page 175 and 176: that most of the noise is due to th
Page 177 and 178: (a) (c) y . x z X=0.0mm Z=2.5mm 1)
Page 179 and 180: Figure 8.11: Different shapes of MO
Page 181 and 182: ZnSe lens f=5 in knife edge ZnSe wi
Page 183 and 184: shown in figure 8.13. By matching t
Page 185 and 186: Figure 8.15: Atom number and temper
Page 187 and 188: 275 Hz. Using these values the beam
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system. Maybe the easiest way to ac
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Appendix A Magic Wavelength of Hydr
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transitions for the excited state p
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Bibliography [1] J.J. Thomson. Cath
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[22] C.J. Foot. Atomic Physics. Oxf
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[46] E.D. Black. An introduction to
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[67] J.L. Hanssen. Controlling Atom
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[88] D.S. Naik, C.G. Peterson, A.G.
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[110] J.W. Goodman. Introduction to
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[132] C. Degenhardt, H. Stoehr, U.
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