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Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas

[Image: see text] We report a combined experimental and modeling study of microwave-activated dilute CH(4)/N(2)/H(2) plasmas, as used for chemical vapor deposition (CVD) of diamond, under very similar conditions to previous studies of CH(4)/H(2), CH(4)/H(2)/Ar, and N(2)/H(2) gas mixtures. Using cavi...

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Autores principales: Truscott, Benjamin S., Kelly, Mark W., Potter, Katie J., Ashfold, Michael N. R., Mankelevich, Yuri A.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2016
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5293323/
https://www.ncbi.nlm.nih.gov/pubmed/27718565
http://dx.doi.org/10.1021/acs.jpca.6b09009
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author Truscott, Benjamin S.
Kelly, Mark W.
Potter, Katie J.
Ashfold, Michael N. R.
Mankelevich, Yuri A.
author_facet Truscott, Benjamin S.
Kelly, Mark W.
Potter, Katie J.
Ashfold, Michael N. R.
Mankelevich, Yuri A.
author_sort Truscott, Benjamin S.
collection PubMed
description [Image: see text] We report a combined experimental and modeling study of microwave-activated dilute CH(4)/N(2)/H(2) plasmas, as used for chemical vapor deposition (CVD) of diamond, under very similar conditions to previous studies of CH(4)/H(2), CH(4)/H(2)/Ar, and N(2)/H(2) gas mixtures. Using cavity ring-down spectroscopy, absolute column densities of CH(X, v = 0), CN(X, v = 0), and NH(X, v = 0) radicals in the hot plasma have been determined as functions of height, z, source gas mixing ratio, total gas pressure, p, and input power, P. Optical emission spectroscopy has been used to investigate, with respect to the same variables, the relative number densities of electronically excited species, namely, H atoms, CH, C(2), CN, and NH radicals and triplet N(2) molecules. The measurements have been reproduced and rationalized from first-principles by 2-D (r, z) coupled kinetic and transport modeling, and comparison between experiment and simulation has afforded a detailed understanding of C/N/H plasma-chemical reactivity and variations with process conditions and with location within the reactor. The experimentally validated simulations have been extended to much lower N(2) input fractions and higher microwave powers than were probed experimentally, providing predictions for the gas-phase chemistry adjacent to the diamond surface and its variation across a wide range of conditions employed in practical diamond-growing CVD processes. The strongly bound N(2) molecule is very resistant to dissociation at the input MW powers and pressures prevailing in typical diamond CVD reactors, but its chemical reactivity is boosted through energy pooling in its lowest-lying (metastable) triplet state and subsequent reactions with H atoms. For a CH(4) input mole fraction of 4%, with N(2) present at 1–6000 ppm, at pressure p = 150 Torr, and with applied microwave power P = 1.5 kW, the near-substrate gas-phase N atom concentration, [N](ns), scales linearly with the N(2) input mole fraction and exceeds the concentrations [NH](ns), [NH(2)](ns), and [CN](ns) of other reactive nitrogen-containing species by up to an order of magnitude. The ratio [N](ns)/[CH(3)](ns) scales proportionally with (but is 10(2)–10(3) times smaller than) the ratio of the N(2) to CH(4) input mole fractions for the given values of p and P, but [N](ns)/[CN](ns) decreases (and thus the potential importance of CN in contributing to N-doped diamond growth increases) as p and P increase. Possible insights regarding the well-documented effects of trace N(2) additions on the growth rates and morphologies of diamond films formed by CVD using MW-activated CH(4)/H(2) gas mixtures are briefly considered.
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spelling pubmed-52933232017-02-07 Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas Truscott, Benjamin S. Kelly, Mark W. Potter, Katie J. Ashfold, Michael N. R. Mankelevich, Yuri A. J Phys Chem A [Image: see text] We report a combined experimental and modeling study of microwave-activated dilute CH(4)/N(2)/H(2) plasmas, as used for chemical vapor deposition (CVD) of diamond, under very similar conditions to previous studies of CH(4)/H(2), CH(4)/H(2)/Ar, and N(2)/H(2) gas mixtures. Using cavity ring-down spectroscopy, absolute column densities of CH(X, v = 0), CN(X, v = 0), and NH(X, v = 0) radicals in the hot plasma have been determined as functions of height, z, source gas mixing ratio, total gas pressure, p, and input power, P. Optical emission spectroscopy has been used to investigate, with respect to the same variables, the relative number densities of electronically excited species, namely, H atoms, CH, C(2), CN, and NH radicals and triplet N(2) molecules. The measurements have been reproduced and rationalized from first-principles by 2-D (r, z) coupled kinetic and transport modeling, and comparison between experiment and simulation has afforded a detailed understanding of C/N/H plasma-chemical reactivity and variations with process conditions and with location within the reactor. The experimentally validated simulations have been extended to much lower N(2) input fractions and higher microwave powers than were probed experimentally, providing predictions for the gas-phase chemistry adjacent to the diamond surface and its variation across a wide range of conditions employed in practical diamond-growing CVD processes. The strongly bound N(2) molecule is very resistant to dissociation at the input MW powers and pressures prevailing in typical diamond CVD reactors, but its chemical reactivity is boosted through energy pooling in its lowest-lying (metastable) triplet state and subsequent reactions with H atoms. For a CH(4) input mole fraction of 4%, with N(2) present at 1–6000 ppm, at pressure p = 150 Torr, and with applied microwave power P = 1.5 kW, the near-substrate gas-phase N atom concentration, [N](ns), scales linearly with the N(2) input mole fraction and exceeds the concentrations [NH](ns), [NH(2)](ns), and [CN](ns) of other reactive nitrogen-containing species by up to an order of magnitude. The ratio [N](ns)/[CH(3)](ns) scales proportionally with (but is 10(2)–10(3) times smaller than) the ratio of the N(2) to CH(4) input mole fractions for the given values of p and P, but [N](ns)/[CN](ns) decreases (and thus the potential importance of CN in contributing to N-doped diamond growth increases) as p and P increase. Possible insights regarding the well-documented effects of trace N(2) additions on the growth rates and morphologies of diamond films formed by CVD using MW-activated CH(4)/H(2) gas mixtures are briefly considered. American Chemical Society 2016-10-08 2016-11-03 /pmc/articles/PMC5293323/ /pubmed/27718565 http://dx.doi.org/10.1021/acs.jpca.6b09009 Text en Copyright © 2016 American Chemical Society This is an open access article published under a Creative Commons Attribution (CC-BY) License (http://pubs.acs.org/page/policy/authorchoice_ccby_termsofuse.html) , which permits unrestricted use, distribution and reproduction in any medium, provided the author and source are cited.
spellingShingle Truscott, Benjamin S.
Kelly, Mark W.
Potter, Katie J.
Ashfold, Michael N. R.
Mankelevich, Yuri A.
Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title_full Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title_fullStr Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title_full_unstemmed Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title_short Microwave Plasma-Activated Chemical Vapor Deposition of Nitrogen-Doped Diamond. II: CH(4)/N(2)/H(2) Plasmas
title_sort microwave plasma-activated chemical vapor deposition of nitrogen-doped diamond. ii: ch(4)/n(2)/h(2) plasmas
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5293323/
https://www.ncbi.nlm.nih.gov/pubmed/27718565
http://dx.doi.org/10.1021/acs.jpca.6b09009
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