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

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D2 transition in 87 Rb has a natural linewidth <strong>of</strong> 6 MHz due to the process <strong>of</strong><br />

radiative damping [70]. Doppler broadening smears this line out increasing its<br />

observed width to ∼ 0.5 GHz at room temperature. <strong>The</strong> source <strong>of</strong> this broad-<br />

ening can be understood by considering the relationship between the angular<br />

frequency ω <strong>of</strong> radiation in the laboratory frame <strong>of</strong> reference and the angular<br />

frequency ω ′ seen in a frame <strong>of</strong> reference moving at velocity v<br />

ω ′ = ω − k · v, (2.96)<br />

where k is the wavevector <strong>of</strong> the radiation and has a magnitude k = ω/c. This<br />

equation is correct to first order in v/c and suffices in most situations, however<br />

higher order Doppler effects must be considered in extremely precise spectro-<br />

scopic measurements. As indicated by the dot product, it is the component <strong>of</strong><br />

velocity along the direction <strong>of</strong> ˆ k which is responsible for this shift. <strong>The</strong>refore<br />

to simplify this notation we assume a 1-D geometry so that k ·v = kv. Figure<br />

2.13 illustrates these ideas for a single atom moving with velocity v to the<br />

right. This atom sees radiation traveling to the right at a decreased frequency<br />

and radiation traveling to the left at an increased frequency.<br />

Consider now an ensemble which consists <strong>of</strong> atoms which absorb ra-<br />

diation at frequency ω0 in their rest frame, i.e. when ω ′ = ω0. Atoms with<br />

velocity v will absorb radiation when the Doppler effect shifts the frequency<br />

into resonance<br />

ω − ω0 = kv. (2.97)<br />

If we assume that the ensemble is in thermal equilibrium then the<br />

73

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