1994
DOI: 10.1103/physrevlett.73.1352
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Line Shapes of High Resolution Photoassociation Spectra of Optically Cooled Atoms

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Cited by 143 publications
(128 citation statements)
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“…where K(∆; I, p c , p r ) =h π k r µ e,g (2J g + 1) Γ pe Γ eg (I, ε r ) [∆ + ε D + ε r − ∆ e − E e (I, ε r ) − E rec,mol ] 2 + [Γ e (I, ε r )/2] 2 (2) is the loss rate [23,24,25] corresponding to particular momentum vectors of the relative motion of the two colliding atoms p r as well as the motion of their center of mass p c . Contributions from all possible transitions between excited bound and ground scattering states are included in this expression.…”
Section: Photoassociation Resonancementioning
confidence: 99%
“…where K(∆; I, p c , p r ) =h π k r µ e,g (2J g + 1) Γ pe Γ eg (I, ε r ) [∆ + ε D + ε r − ∆ e − E e (I, ε r ) − E rec,mol ] 2 + [Γ e (I, ε r )/2] 2 (2) is the loss rate [23,24,25] corresponding to particular momentum vectors of the relative motion of the two colliding atoms p r as well as the motion of their center of mass p c . Contributions from all possible transitions between excited bound and ground scattering states are included in this expression.…”
Section: Photoassociation Resonancementioning
confidence: 99%
“…The radiative collision data require modeling of the rate coefficient for the absorptions of a photon by a pair of ultracold Cs atoms [38]. However, we are interested in reproducing the location of Feshbach resonances, and not in the absolute absorption rates.…”
Section: Numerical Approachesmentioning
confidence: 99%
“…For an ensemble of atom pairs with a Maxwell-Boltzmann velocity distribution, employing an isolated photoassociation resonance, the photoassociation rate coeffcient is given by [28] Kṽ′…”
Section: Theoretical Frameworkmentioning
confidence: 99%