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

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          Abstract

          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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          The UMIST Database for Astrochemistry 1995

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            Cross Sections for Electron Collisions with Nitrogen Molecules

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              Franck–Condon Factors, r‐Centroids, Electronic Transition Moments, and Einstein Coefficients for Many Nitrogen and Oxygen Band Systems

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                Author and article information

                Journal
                J Phys Chem A
                J Phys Chem A
                jx
                jpcafh
                The Journal of Physical Chemistry. a
                American Chemical Society
                1089-5639
                1520-5215
                08 October 2016
                03 November 2016
                : 120
                : 43
                : 8537-8549
                Affiliations
                [1]School of Chemistry, University of Bristol , Bristol BS8 1TS, U.K.
                [2]Skobel’tsyn Institute of Nuclear Physics, Moscow State University , Leninskie gory, Moscow 119991, Russia
                [3]Institute of Applied Physics, IAP RAS , 46 Ulyanov st., Nizhny Novgorod 603950, Russia
                Author notes
                [* ]M.N.R.A. E-mail: mike.ashfold@ 123456bris.ac.uk . Tel: +44 (117) 9288312.
                [* ]Yu.A.M. E-mail: ymankelevich@ 123456mics.msu.su .
                Article
                10.1021/acs.jpca.6b09009
                5293323
                27718565
                f9efe0b2-b612-458f-8022-b95246281fb1
                Copyright © 2016 American Chemical Society

                This is an open access article published under a Creative Commons Attribution (CC-BY) License, which permits unrestricted use, distribution and reproduction in any medium, provided the author and source are cited.

                History
                : 06 September 2016
                : 05 October 2016
                Categories
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                Custom metadata
                jp6b09009
                jp-2016-09009u

                Physical chemistry
                Physical chemistry

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