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

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momentum at the time <strong>of</strong> release. <strong>The</strong> final atomic distribution is therefore<br />

a convolution <strong>of</strong> the initial atomic distribution with the initial momentum<br />

distribution.<br />

This can be made more concrete by considering atoms originating from<br />

r0 and arriving at r after a time-<strong>of</strong>-flight t. If we assume that the velocity<br />

distribution for these particles is ζ(v) then we expect to find the number <strong>of</strong><br />

atoms in a volume element d 3 r located at position r at time t to be [80]<br />

dn = G(r,t;r0)d 3 r = ζ(v = [r − r0/t])d 3 v, (2.108)<br />

where G(r,t;r0) is the boundary Green’s function describing the evolution<br />

<strong>of</strong> the spatial distribution <strong>of</strong> the atoms. If the atoms have a 3-D Maxwell-<br />

Boltzmann velocity distribution initially, then the Green’s function is given by<br />

[80]<br />

G(r,t;r0) =<br />

<br />

m<br />

2πkBTt 2<br />

3/2 e −m|r−r0| 2 /2kBTt2 . (2.109)<br />

If we assume that the atomic sample has a Gaussian spatial distribution ini-<br />

tially, given by<br />

n0(r) =<br />

1<br />

(2πσ 2 n) 3/2e−r2 /2σ 2 n, (2.110)<br />

then we can solve for the spatial distribution after an expansion time t by<br />

evaluating<br />

<strong>The</strong> result is<br />

<br />

n(r,t) =<br />

n(r,t) =<br />

G(r,t;r0)n0(r0)0d 3 r0. (2.111)<br />

1<br />

(2πσ 2 c) 3/2e−r2 /2σ 2 c, (2.112)<br />

82

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