4.6 Article

Direct detection of pyridine formation by the reaction of CH (CD) with pyrrole: a ring expansion reaction

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PHYSICAL CHEMISTRY CHEMICAL PHYSICS
卷 12, 期 31, 页码 8750-8758

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ROYAL SOC CHEMISTRY
DOI: 10.1039/c002135k

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  1. National Aeronautics and Space Administration [NNX09AB60G]
  2. Division of Chemical Sciences, Geosciences and Biosciences
  3. Office of Basic Energy Sciences
  4. U.S. Department of Energy
  5. National Nuclear Security Administration [DE-AC04-94-AL85000]
  6. Office of Science, Office of Basic Energy Sciences of the U.S. Department of Energy [DE-AC02-05CH11231]
  7. Australian Synchrotron
  8. Federal Government of Australia

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The reaction of the ground state methylidyne radical CH (X-2 Pi) with pyrrole (C4H5N) has been studied in a slow flow tube reactor using Multiplexed Photoionization Mass Spectrometry coupled to quasi-continuous tunable VUV synchrotron radiation at room temperature (295 K) and 363 K, at 4 Torr (533 Pa). Laser photolysis of bromoform (CHBr3) at 248 nm (KrF excimer laser) is used to produce CH radicals that are free to react with pyrrole molecules in the gaseous mixture. A signal at m/z = 79 (C5H5N) is identified as the product of the reaction and resolved from Br-79 atoms, and the result is consistent with CH addition to pyrrole followed by H-elimination. The photoionization efficiency curve unambiguously identifies m/z = 79 as pyridine. With deuterated methylidyne radicals (CD), the product mass peak is shifted by +1 mass unit, consistent with the formation of C5H4DN and identified as deuterated pyridine (d-pyridine). Within detection limits, there is no evidence that the addition intermediate complex undergoes hydrogen scrambling. The results are consistent with a reaction mechanism that proceeds via the direct CH (CD) cycloaddition or insertion into the five-member pyrrole ring, giving rise to ring expansion, followed by H atom elimination from the nitrogen atom in the intermediate to form the resonance stabilized pyridine (d-pyridine) molecule. Implications to interstellar chemistry and planetary atmospheres, in particular Titan, as well as gas-phase combustion processes, are discussed.

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