2009
DOI: 10.1103/physreva.79.053405
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Light scattering from a dense and ultracold atomic gas

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Cited by 56 publications
(91 citation statements)
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“…As the computational difficulty increases rapidly with the number of atoms the atomic density is chosen not very big n = 0.05 which corresponds to the mean free path of photon l ph = 1.63. However, as it was shown in [32] the collective effects caused by dipole-dipole interaction play a significant role for such density.…”
Section: A Angular Distribution Of Scattered Lightmentioning
confidence: 99%
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“…As the computational difficulty increases rapidly with the number of atoms the atomic density is chosen not very big n = 0.05 which corresponds to the mean free path of photon l ph = 1.63. However, as it was shown in [32] the collective effects caused by dipole-dipole interaction play a significant role for such density.…”
Section: A Angular Distribution Of Scattered Lightmentioning
confidence: 99%
“…This matrix describes the multiple photon exchange among atoms and it depends both on the spatial location of atoms and on the frequency of probe light (see [26], [32]). The vector b…”
Section: Basic Assumptions and Approachmentioning
confidence: 99%
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“…Often continuous density distributions have been assumed which allow for analytical expressions to be obtained. The role of fluctuations of the atomic density is however by itself at the origin of interesting phenomena, such as Anderson localisation of light (2,3). In a series of theoretical and experimental studies, we have recently addressed the question of the quasi-resonant interaction of light with clouds of cold atoms, bridging the gap from single atom behavior, effects dominated by disorder to a mean field regime, where a continuous density distribution is the relevant description.…”
Section: Introductionmentioning
confidence: 99%
“…Light-matter interactions in dense regime is a very dynamic and challenging field of research [4][5][6] where one of the long standing problem is the understanding of the role of cooperative effects (superradiance [7,8], subradiance [9], collective Lamb shift [10]) and disorder (weak [11] and strong localization [12]). In order to reach this regime, a dipole trap can be used to compress the cloud to high densities where the strong localization phase transition [12] is expected to occur at a threshold given by the Ioffe-Reggel criterion [13] k · l ∼ 1, where k = 2π/λ is the light wavevector and l = 1/(nσ) is the mean free path (n the atomic density, σ the scattering cross section).…”
Section: Introductionmentioning
confidence: 99%