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Published July 7, 2020 | Supplemental Material
Journal Article Open

Photo-oxidation of aromatic hydrocarbons produces low-volatility organic compounds

Abstract

To better understand the role of aromatic hydrocarbons in new-particle formation, we measured the particle-phase abundance and volatility of oxidation products following the reaction of aromatic hydrocarbons with OH radicals. For this we used thermal desorption in an iodide-adduct Time-of-Flight Chemical-Ionization Mass Spectrometer equipped with a Filter Inlet for Gases and AEROsols (FIGAERO-ToF-CIMS). The particle-phase volatility measurements confirm that oxidation products of toluene and naphthalene can contribute to the initial growth of newly formed particles. Toluene-derived (C₇) oxidation products have a similar volatility distribution to that of α-pinene-derived (C₁₀) oxidation products, while naphthalene-derived (C₁₀) oxidation products are much less volatile than those from toluene or α-pinene; they are thus stronger contributors to growth. Rapid progression through multiple generations of oxidation is more pronounced in toluene and naphthalene than in α-pinene, resulting in more oxidation but also favoring functional groups with much lower volatility per added oxygen atom, such as hydroxyl and carboxylic groups instead of hydroperoxide groups. Under conditions typical of polluted urban settings, naphthalene may well contribute to nucleation and the growth of the smallest particles, whereas the more abundant alkyl benzenes may overtake naphthalene once the particles have grown beyond the point where the Kelvin effect strongly influences the condensation driving force.

Additional Information

© 2020 American Chemical Society. Received: April 4, 2020; Revised: June 2, 2020; Accepted: June 9, 2020; Published: June 9, 2020. We thank the European Organization for Nuclear Research (CERN) for supporting CLOUD with important technical and financial resources and for providing a particle beam from the CERN Proton Synchrotron. This research has received funding from the U.S. National Science Foundation under grants AGS-1447056, AGS-1439551, AGS-1649147, AGS-1602086, and AGS-1801897; the German Federal Ministry of Education and Research (No. 01LK1601A); ERC-Consolidator Grant NANODYNAMITE 616075; Horizon 2020 Marie Skłodowska-Curie Grant 656994 ("Nano-CAVa"); ERC Advanced "ATM-GP" grant No. 227463; the Presidium of the Russian Academy of Sciences, the Program "High energy physics and neutrino astrophysics" 2015; the Swiss National Science Foundation Projects 200020_152907, 20FI20_159851, 200021_169090, 200020_172602, and 20FI20_172622. The FIGAERO–CIMS was supported by an MRI grant for the U.S. NSF AGS-1531284 as well as the Wallace Research Foundation. O.G. thanks the Doctoral Programme in Atmospheric Sciences at the University of Helsinki for financial support. Author Contributions: M.W., D.C., M.X., J.K., D.R.W., U.B., J.Do., I.E.-H., and N.M.D. designed the research; M.W., D.C., M.X., Q.Y., D.S., V.H., P.Y., A.L.V., R.L.M., A.A., A.B., B.B., S.B., L.D., A.D., J.Du., H.F., O.G., X.H., C.R.H., C.K., A.K., K.L., F.L., U.M., T.P., V.P., L.L. J.Q., M.R., M.S., C.T., A.T., A.C.W., L.W., J.K., J.Do., and I.E.-H. performed the research; M.W., M.X., D.S., and N.M.D. contributed new reagents/analytic tools; M.W., M.X., D.S., P.Y., and M.S. analyzed the data; and M.W., D.C., M.X., A.L.V., U.M., J.K., U.B., J.Do., I.E.-H., and N.M.D. wrote the paper. The authors declare no competing financial interest.

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Additional details

Created:
August 19, 2023
Modified:
October 20, 2023