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

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atoms its wavefunction Ψ(t) is typically intractable. Instead we use the density<br />

matrix formalism which provides a convenient way <strong>of</strong> describing the evolution<br />

<strong>of</strong> the ensemble average expectation value <strong>of</strong> the dipole operator 〈µ(t)〉 even<br />

when Ψ(t) is unknown.<br />

<strong>The</strong> density matrix can be defined in two steps. In the first step, we<br />

consider the expectation value <strong>of</strong> the dipole operator for a single atom<br />

〈µ(t)〉 = 〈Ψ(r,t)|µ|Ψ(r,t)〉. (2.57)<br />

We then expand Ψ(r,t) in a complete set <strong>of</strong> orthonormal eigenfunctions <strong>of</strong> the<br />

unperturbed atomic Hamiltonian H0<br />

Ψ(r,t) = <br />

cn(t)un(r), (2.58)<br />

n<br />

where all <strong>of</strong> the time dependence has been placed in the coefficients cn(t). We<br />

then evaluate the expectation value <strong>of</strong> the dipole operator in this basis<br />

〈µ(t)〉 = <br />

c ∗ m(t)〈um(r)|µ|un(r)〉cn(t). (2.59)<br />

m,n<br />

By defining µmn ≡ 〈um(r)|µ|un(r)〉 and Rnm ≡ cnc ∗ m this can be written much<br />

more compactly as<br />

〈µ(t)〉 = <br />

Rnmµmn = <br />

(Rµ)nn = Tr(Rµ). (2.60)<br />

m,n<br />

n<br />

Next we apply this approach to an atomic ensemble. To do so we define<br />

ρnm(t) ≡ Rnm(t), (2.61)<br />

51

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