2013
DOI: 10.1080/09500340.2013.829264
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Interplay between radiation pressure force and scattered light intensity in the cooperative scattering by cold atoms

Abstract: The interplay between the superradiant emission of a cloud of cold two-level atoms and the radiation pressure force is discussed. Using a microscopic model of coupled atomic dipoles driven by an external laser, the radiation field and the average radiation pressure force are derived. A relation between the far-field scattered intensity and the force is derived, using the optical theorem. Finally, the scaling of the sample scattering cross section with the parameters of the system is studied.

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Cited by 15 publications
(13 citation statements)
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“…The relevant parameters to describe light scattering in dilute clouds of two-level systems is the resonant optical thickness of the cloud, which is given by b 0 = 2N/(k 0 σ R ) 2 with an on-resonant scattering cross section for a single atom given in the scalar model by σ sc = λ 2 /π . The detuning dependent optical thickness then (1), the far-field intensity in a direction k and at a distance r can be calculated using [23] …”
Section: Coupled Dipole Modelmentioning
confidence: 99%
“…The relevant parameters to describe light scattering in dilute clouds of two-level systems is the resonant optical thickness of the cloud, which is given by b 0 = 2N/(k 0 σ R ) 2 with an on-resonant scattering cross section for a single atom given in the scalar model by σ sc = λ 2 /π . The detuning dependent optical thickness then (1), the far-field intensity in a direction k and at a distance r can be calculated using [23] …”
Section: Coupled Dipole Modelmentioning
confidence: 99%
“…The microscopic and mean-field approaches have been shown to provide equivalent results on the presence of polaritonic modes in these clouds [13,14]. Optical forces [15,16] have also drawn some attention recently, yet the role of dipoledipole correlations have been discussed to be minor [17]. Recently, the microscopic theory emerged as an important tool to study the deviations from mean-field theory due to strong particle-particle correlations, as they appear in the high density regime [18,19] or close to the atomic resonance [20].…”
Section: Introductionmentioning
confidence: 96%
“…It only neglects refraction and diffraction effects, which could have an impact for very small clouds [7]. It also neglects the forward coherent lobe [10,42,43], which actually is diffracted/refracted light (this light is also responsible for the extinction paradox [44]). The Beer-Lambert result for the total intensity is equivalent to integrating in all directions the scattered intensity computed from the RW model.…”
Section: Beer-lambert Lawmentioning
confidence: 99%