Bulletin of the American Physical Society
63rd Annual Meeting of the APS Division of Plasma Physics
Volume 66, Number 13
Monday–Friday, November 8–12, 2021; Pittsburgh, PA
Session PP11: Poster Session VI:
BEAMS- Computational, Analytical, Measurement, and Diagnostic Techniques for Lasers and Beams, Laser-Plasma Wakefield, Beam-Plasma Wakefield, and Direct Laser Accelerators
Low Temperature Plasma
MFE- Edge and Pedestal Stellarators
Mini-Conference on Machine Learning
2:00 PM - 5:00 PM
Wednesday, November 10, 2021
Room: Hall A
Abstract: PP11.00017 : 0D Kinetic Modeling of Noble Gas Mixed N2-H2 Plasmas for Ammonia Synthesis*
Presenter:
James B Hall
(Princeton University)
Authors:
James B Hall
(Princeton University)
Shota Abe
(Princeton University)
Zhe Chen
(Princeton University)
Zihan Lin
(Princeton University)
Surabhi Jaiswal
(Princeton University)
Ahmed Diallo
(Princeton Plasma Physics Laboratory)
Bruce E Koel
(Princeton University)
A zero-dimensional (0D) kinetic model has been developed for N2-H2-noble gas (He or Ar) atmospheric pressure plasmas based on the ZDPlasKin plasma kinetics solver [1] to understand both the volumetric and surface (Ru or Fe on ??-Al2O3) reactions related to plasma-assisted catalysis as a potentially lower energy alternative to the standard Haber-Bosch process for ammonia synthesis. Results have shown that the dominant metastables, Armeta (1s5 and 1s3) and He(23S), formed via electron-impact excitation, can support N atom and ion formation through the reactions N2 + Armeta → 2N + Ar and N2 + He(23S) → N + N+ + He + e. These N species play an important role in NH3 formation via N + H2* →NH + H (H2* is an electronically excited species) in our dielectric barrier discharge reactor for electron number densities 106-1010 cm-3. Effects of the neutral gas flow rates for both He and Ar on the plasma chemistry are also investigated. We pair the He modeling results with a He Collisional-Radiative (CR) model for plasma diagnostics and compare with He line intensity ratios experimentally obtained by optical emission spectroscopy.
[1] S. Pancheshnyi et al., 2008 Computer code ZDPlasKin (www.zdplaskin.laplace.univ-tlse.fr)
*JBH and ZL acknowledge support by the Environmental Internship Program in Princeton's High Meadows Environmental Institute. ZC acknowledges partial support by the Program in Plasma Science and Technology at Princeton and ExxonMobil Research and Engineering Company, award no. EM09125.A1, Project 10011645. This material is based on work supported by DOE award DE-SC0020233, and PPPL through Prime Contract DE-AC02-09CH11466.
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