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

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component <strong>of</strong> the dipole oscillation. <strong>The</strong> dipole force can be found from the<br />

gradient <strong>of</strong> the potential energy and is therefore a conservative field.<br />

Fdip = −∇Udip(r) = 1<br />

Re(α)∇I(r) (2.47)<br />

2ǫ0c<br />

Thus the optical dipole force comes from the dispersive interaction <strong>of</strong> the<br />

induced dipole moment with the gradient <strong>of</strong> the driving light field [59, 64–66].<br />

We now turn our attention to modeling α which we do following Lorentz’s<br />

model <strong>of</strong> a classical oscillator. In this model the electron is considered to be<br />

a classical particle bound elastically to a nucleus and possessing an oscillation<br />

frequency ω0 which is identified with the frequency <strong>of</strong> the optical transition<br />

<strong>of</strong> interest. Damping is included in this model through Larmor’s formula for<br />

the power radiated by an accelerating charge [67]. This model has several<br />

limitations - it does not model an atom with multiple transitions and does<br />

not display any saturation behavior when strongly driven. In the far-detuned<br />

limit neither <strong>of</strong> these limitations are <strong>of</strong> concern.<br />

<strong>The</strong> equation <strong>of</strong> motion for a damped, driven harmonic oscillator<br />

¨x + ΓL ˙x + ω 2 0x = − eE(t)<br />

can be used to solve for α by noting that p = −ex = αE. <strong>The</strong> result is<br />

α = e2<br />

me<br />

me<br />

(2.48)<br />

1<br />

ω2 0 − ω2 , (2.49)<br />

− iωΓL<br />

where the damping coefficient ΓL is the classical Larmor energy damping rate<br />

due to radiative loss<br />

ΓL = e2 ω 2<br />

6πǫ0mec 3.<br />

47<br />

(2.50)

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