Transport properties of electron swarms in gaseous neon at low values ofE/N
Boyle, G.J., Casey, M.J.E., White, R.D., Cheng, Y., and Mitroy, J. (2014) Transport properties of electron swarms in gaseous neon at low values ofE/N. Journal of Physics D: applied physics, 47 (34). 345203. pp. 1-9.
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Abstract
A detailed analysis of electron swarm transport through neon gas at applied reduced electric fields of E/N < 2 Td is presented. The root mean square difference of transport parameters calculated from a recent all-order many-body perturbation theory treatment (Cheng et al 2014 Phys. Rev. A 89 012701) with drift velocity measurements by the Australian National University group (Robertson 1972 J. Phys. B 5 648) is less than 1%. Differences of about 3% exist with characteristic energies, DT/μ, (Koizumi et al 1984 J. Phys. B 17 4387) indicating an incompatibility at the 3% level between drift velocity and transverse diffusion coefficient measurements. Multi-term solutions of the Boltzmann equation indicate that the two-term approximation gives transport parameters accurate to better than 0.01%. The diffusion constant at thermal energies is found to be sensitive to the numerical representation of the cross section. A recommended elastic momentum transfer cross section has been constructed that has a maximum difference of 0.5% with all ANU drift velocity data for E/N < 1.6 Td and a root mean square difference that is about a factor of 2 smaller.
Item ID: | 34578 |
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Item Type: | Article (Research - C1) |
ISSN: | 1361-6463 |
Copyright Information: | © 2014 IOP Publishing Ltd |
Funders: | Australian Research Council (ARC) |
Date Deposited: | 14 Aug 2014 04:27 |
FoR Codes: | 02 PHYSICAL SCIENCES > 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics > 020201 Atomic and Molecular Physics @ 80% 02 PHYSICAL SCIENCES > 0204 Condensed Matter Physics > 020404 Electronic and Magnetic Properties of Condensed Matter; Superconductivity @ 20% |
SEO Codes: | 97 EXPANDING KNOWLEDGE > 970102 Expanding Knowledge in the Physical Sciences @ 100% |
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