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

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ω ω ω ω<br />

<br />

Figure 2.13: <strong>The</strong> Doppler effect shifts the observed frequency <strong>of</strong> radiation<br />

due to the atoms velocity. <strong>The</strong> atom travels to the right and sees radiation<br />

traveling to the right at a decreased frequency and radiation traveling to the<br />

left at an increased frequency.<br />

velocity distribution is given by the 1-D Maxwell-Boltzmann distribution<br />

<br />

f(v)dv = 1<br />

u √ v2<br />

e− u<br />

π 2 , (2.98)<br />

where u = 2kBT/m is the most probable speed for atoms. <strong>The</strong> absorption<br />

pr<strong>of</strong>ile g(ω) <strong>of</strong> this ensemble can be found by relating the velocity <strong>of</strong> the atoms<br />

with their corresponding absorption frequency using Eq. 2.97, the result being<br />

g(ω) =<br />

c<br />

√ e<br />

uω0 π<br />

c2<br />

−<br />

u2 ( ω−ω0 ) ω0 2<br />

. (2.99)<br />

This Doppler broadened pr<strong>of</strong>ile has a Gaussian shape and a full width at half<br />

maximum (FWHM) ∆ωD <strong>of</strong><br />

∆ωD = 2ω0<br />

√ u<br />

ln2 , (2.100)<br />

c<br />

which for 87 Rb is 1.4 × 10 −6 , limiting the resolution <strong>of</strong> spectroscopic mea-<br />

surements to approximately 1 part in 10 6 . Because we use a laser frequency<br />

locking scheme which is referenced to 87 Rb transition lines, the resolution with<br />

which we resolve these transitions places a limit on our ability to control the<br />

frequency <strong>of</strong> the lasers. <strong>The</strong> needed resolution is 1 part in 10 8 so we must use<br />

a spectroscopic technique which suppresses the effect <strong>of</strong> Doppler broadening.<br />

74

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