Modeling of positron thermalization in collisional traps
ORAL
Abstract
A Monte Carlo code has been used to follow the orbits of positrons thermalizing from approximately 10 eV down to very low energies. This technique is appropriate as positrons suffer only a very few collisions so their transport is fully non-hydrodynamic. We have studied how the initial energy distribution of a moderated positron beam changes to a low energy, trapped, group of positrons, and which processes contribute to that. We followed how energy and momentum are dissipated in collisions, the thermalization time, the role of the magnetic field, the size of the Larmor radius and geometry of the trap, and how different abundances of gases in the mixture affect the result and other aspects of low energy positron traps. Most importantly in all cases we could sample the efficiency of thermalization by following the losses of positrons due to Ps formation. Complete sets of cross sections covering all major, number, momentum and energy balance processes were included for gases such as Ar, He, H$_{2}$, N$_{2}$ and N$_{2}$/CF$_{4}$ mixture. Fore example our results indicate thermalization times of Nt= 2.51*10$^{17}$ sm$^{-3}$ for pure nitrogen and 1.41*10$^{16}$ sm$^{-3}$ for N$_{2}$/CF$_{4}$ mixture.
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Authors
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Ana Bankovic
Institute of Physics, Belgrade, Serbia
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Joan P. Marler
University of Aarhus, Aarhus, Denmark
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Gordana Malovic
Institute of Physics, Belgrade, Serbia, Institute of Physics, Pregrevica 118, 11080 Belgrade, Serbia
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Stephen Buckman
RSPhysSE, Australian National University, Canberra, Australia, CAMS, Australian National University, Australian National University
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Milovan Suvakov
Institute of Physics, Belgrade, Serbia
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Zoran Petrovic
Institute of Physics, Belgrade, Serbia, Institute of Physics, Belgrade-Serbia, Institute of Physics, Pregrevica 118, 11080 Belgrade, Serbia, Institute of Physics Belgrade, Institute of Physics