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9744259839
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note
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l = {1, 3, 5,...} terms are strictly forbidden and l = {4, 6, 8,...} terms have been calculated to be completely negligible for the energy interval of interest.
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28
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9744276299
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2 (x, y, z, t). Assuming the clouds to have initially Gaussian density distributions in all directions, this system was solved numerically to calculate the fraction of scattered particles and assess the scaling with the coupling parameter σ(T). Because of the prolate cloud shapes we neglect multiple scattering events.
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30
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zt).
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31
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9744223148
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to be published
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As a consequence of the broadening, some scattered atoms reach their maximum radial excursion point before the time of image acquisition. This effectively transfers them to angular bins closer to the collision axis. The slight left-right pattern asymmetry observable for some collision energies is a combined result of the clouds having slightly different speeds in the laboratory frame, a small offset on the z axis between collision and trap centers, and the size difference between colliding clouds [N. Kjærgaard, A. S. Mellish, and A. C. Wilson, New J. Phys. (to be published)].
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New J. Phys.
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Kjærgaard, N.1
Mellish, A.S.2
Wilson, A.C.3
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