2019
DOI: 10.1103/physreva.100.062709
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Differential positronium-formation cross sections for Ne, Ar, Kr, and Xe

Abstract: Experimental determinations of the absolute differential positronium-formation cross sections near 0 • for Ne, Ar, Kr, and Xe are presented and compared with theory. The degree of forward collimation, expressed by the ratios of the differential-to-integral positronium-formation cross sections, is also computed and compared with theories and other targets. Trends among targets and structures at low energies emerge when considered as a function of the reduced total energy.

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Cited by 6 publications
(7 citation statements)
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“…The Ps-formation DCS near the forward direction has been recently measured for positron collisions for a number of targets including helium [4][5][6]. While a dip was found in the measured near-forward direction Ps-formation DCS for positron collisions from Ne, Ar, Kr and Xe [5], it was not observed in the cross section for positron-helium collisions for the energy range of the experiment [4,6].…”
Section: Discussionmentioning
confidence: 99%
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“…The Ps-formation DCS near the forward direction has been recently measured for positron collisions for a number of targets including helium [4][5][6]. While a dip was found in the measured near-forward direction Ps-formation DCS for positron collisions from Ne, Ar, Kr and Xe [5], it was not observed in the cross section for positron-helium collisions for the energy range of the experiment [4,6].…”
Section: Discussionmentioning
confidence: 99%
“…The Ps-formation DCS near the forward direction has been recently measured for positron collisions for a number of targets including helium [4][5][6]. While a dip was found in the measured near-forward direction Ps-formation DCS for positron collisions from Ne, Ar, Kr and Xe [5], it was not observed in the cross section for positron-helium collisions for the energy range of the experiment [4,6]. However, we theoretically obtained a minimum in the Ps-formation DCS (θ = 0 • ) for positron-helium collisions at 17.9 eV, which is at a lower energy than the energies considered in the experiment for helium [4,6].…”
Section: Discussionmentioning
confidence: 99%
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