z-logo
open-access-imgOpen Access
Direct Measurement of Radical-Catalyzed C6H6 Formation from Acetylene and Validation of Theoretical Rate Coefficients for C2H3 + C2H2 and C4H5 + C2H2 Reactions
Author(s) -
Mica C. Smith,
Guozhu Liu,
Zachary J. Buras,
TeChun Chu,
Jeehyun Yang,
William H. Green
Publication year - 2020
Publication title -
the journal of physical chemistry a
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.756
H-Index - 235
eISSN - 1520-5215
pISSN - 1089-5639
DOI - 10.1021/acs.jpca.0c00558
Subject(s) - chemistry , acetylene , radical , photoionization , benzene , photochemistry , mass spectrometry , yield (engineering) , computational chemistry , organic chemistry , thermodynamics , ion , physics , chromatography , ionization
The addition of vinylic radicals to acetylene is an important step contributing to the formation of polycyclic aromatic hydrocarbons in combustion. The overall reaction 3C 2 H 2 → C 6 H 6 could result in large benzene yields, but without accurate rate parameters validated by experiment, the extent of aromatic ring formation from this pathway is uncertain. The addition of vinyl radicals to acetylene was investigated using time-resolved photoionization time-of-flight mass spectrometry at 500 and 700 K and 5-50 Torr. The formation of C 6 H 6 was observed at all conditions, attributed to sequential addition to acetylene followed by cyclization. Vinylacetylene (C 4 H 4 ) was observed with increasing yield from 500 to 700 K, attributed to the β-scission of the thermalized 1,3-butadien-1-yl radical and the chemically activated reaction C 2 H 3 + C 2 H 2 → C 4 H 4 + H. The measured kinetics and product distributions are consistent with a kinetic model constructed using pressure- and temperature-dependent reaction rate coefficients computed from previously reported ab initio calculations. The experiments provide direct measurements of the hypothesized C 4 H 5 intermediates and validate predictions of pressure-dependent addition reactions of vinylic radicals to C 2 H 2 , which are thought to play a key role in soot formation.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom