Skip to main content
Wiley Open Access Collection logoLink to Wiley Open Access Collection
. 2014 Mar 25;53(18):4547–4550. doi: 10.1002/anie.201400964

Rate Coefficients of C1 and C2 Criegee Intermediate Reactions with Formic and Acetic Acid Near the Collision Limit: Direct Kinetics Measurements and Atmospheric Implications**

Oliver Welz 1, Arkke J Eskola 1, Leonid Sheps 1, Brandon Rotavera 1, John D Savee 1, Adam M Scheer 1, David L Osborn 1, Douglas Lowe 2, A Murray Booth 2, Ping Xiao 3, M Anwar H Khan 3, Carl J Percival 2,*, Dudley E Shallcross 3,*, Craig A Taatjes 1,*
PMCID: PMC4499262  PMID: 24668781

Abstract

Rate coefficients are directly determined for the reactions of the Criegee intermediates (CI) CH2OO and CH3CHOO with the two simplest carboxylic acids, formic acid (HCOOH) and acetic acid (CH3COOH), employing two complementary techniques: multiplexed photoionization mass spectrometry and cavity-enhanced broadband ultraviolet absorption spectroscopy. The measured rate coefficients are in excess of 1×10−10 cm3 s−1, several orders of magnitude larger than those suggested from many previous alkene ozonolysis experiments and assumed in atmospheric modeling studies. These results suggest that the reaction with carboxylic acids is a substantially more important loss process for CIs than is presently assumed. Implementing these rate coefficients in global atmospheric models shows that reactions between CI and organic acids make a substantial contribution to removal of these acids in terrestrial equatorial areas and in other regions where high CI concentrations occur such as high northern latitudes, and implies that sources of acids in these areas are larger than previously recognized.

Keywords: atmospheric chemistry, Criegee intermediates, gas-phase chemistry, kinetics, organic acids


Gas-phase ozonolysis is a major degradation mechanism of alkenes in the Earth’s atmosphere and forms Criegee intermediates (CIs), carbonyl oxides, as reactive intermediates.[1] Many of these CIs have enough energy to decompose, but a fraction becomes collisionally stabilized. These so-called stabilized CIs (in the following simply denoted as CIs, as we consider only the stabilized fraction) can undergo subsequent bimolecular reactions. The chemistry of CIs plays a central role in controlling the budgets of many tropospheric species including OH, organic acids, and secondary organic aerosols (SOA). Until recently all knowledge of the reactivity of CIs had been derived from indirect ozonolysis experiments or theoretical kinetics calculations, and the rate coefficients for reactions of CIs with key atmospheric species have been uncertain by several orders of magnitude.[2] The discovery that CIs are formed in the reactions of α-iodoalkyl radicals with O2[3] has enabled direct kinetics measurements of CI reactions.[3,4] These measurements revealed that the rate coefficients of CI reactions with several key atmospheric species are substantially different than models had assumed.[2]

The reaction of CIs with organic acids can provide a pathway in which alkenes are converted to low-volatility compounds and thus contribute to the formation of SOA. Here we report the direct determination of the rate coefficients for the reactions of two CIs, CH2OO and both conformers[4d] of CH3CHOO, with formic acid (HCOOH) and acetic acid (CH3COOH) (reactions (1)–(6)).

graphic file with name anie0053-4547-m1.jpg (1)
graphic file with name anie0053-4547-m2.jpg (2)
graphic file with name anie0053-4547-m3.jpg (3)
graphic file with name anie0053-4547-m4.jpg (4)
graphic file with name anie0053-4547-m5.jpg (5)
graphic file with name anie0053-4547-m6.jpg (6)

Two complementary techniques are employed for time-resolved detection of the CIs: multiplexed photoionization mass spectrometry (MPIMS)[3,4d] (for CH2OO, syn- and anti-CH3CHOO) and cavity-enhanced broadband ultraviolet (UV) absorption spectroscopy[4a] (for CH2OO). The measured rate coefficients are in excess of 1×10−10 cm3 s−1, several orders of magnitude faster than results from experiments of alkene ozonolysis in the presence of carboxylic acids[5] and what modeling studies have employed.[6] With these rate coefficients, global atmospheric modeling and steady-state analysis shows that CI reactions with organic acids have significant effects on concentrations of acids and CI in the environment.

Figure 1 a shows time profiles of CH2OO from the MPIMS experiments, and Figure 2 a shows a corresponding plot for CH2OO from the UV absorption experiments. In the absence of added co-reactant, the CI signals follow a first-order decay, kloss, that reflects both loss on the walls (dominant under these low-pressure conditions), and unimolecular decomposition. Upon adding acid, the decay of CI becomes faster. The rate coefficients for reactions (1)–(6) were determined by measuring the CI decay as a function of the acid concentration. Time profiles of the CIs were fitted to a single exponential decay, convolved with the temporal instrument response function.[3,4] The rate coefficient for the pseudo-first-order loss of the CI depends linearly on [acid], with the slope yielding the second-order rate coefficient for the CI reaction with acid and the intercept reflecting kloss. Such plots are shown in Figure 1 b for reactions (1), (3), and (4), in Figure 2 b for reaction (2), and for the other reactions in Figures S1 and S2 (see the Supporting Information).

Figure 1.

Figure 1

Kinetics results from the MPIMS experiments. a) CH2OO time traces as a function of [HCOOH] taken using a H2 discharge lamp for ionization, and fits to the experimental data. b) Dependence of the decay constant of CH2OO (black; taken with a H2 discharge), anti-CH3CHOO (blue; taken using 9.35 eV synchrotron radiation), and syn-CH3CHOO (blue; taken using 10.5 eV synchrotron radiation). The solid lines are fits to the experimental data. The slopes are the second-order rate coefficients for the CI+acid reactions. Error bars reflect the 1σ uncertainties from the fits of the experimental time profiles.

Figure 2.

Figure 2

Kinetics results from the UV absorption experiments. a) CH2OO time traces for [CH3COOH] in the range (1.86–22.39)×1012 cm−3, and fits to the experimental data. b) Dependence of the decay constant of CH2OO on [CH3COOH]. The solid line is a fit to the experimental data with the slope as the second-order rate coefficient for the CH2OO+CH3COOH reaction. Error bars shown are 15 % of the nominal value as estimated from repeated experiments at identical conditions.

Table 1 summarizes the rate coefficients for reactions (1)–(6) determined in this work. The values for the CH2OO reactions obtained with the two independent experimental techniques are in close agreement. Furthermore, the rate coefficient does not decrease with increasing size of either the CI or the carboxylic acid, suggesting that the rate coefficients of other CI+carboxylic acid reactions are also large. We find negligible conformer dependence in the rate coefficients for the anti- and syn-CH3CHOO reactions.

Table 1.

Rate coefficients for CI+carboxylic acid reactions determined in this work at 298 K. Error bounds represent 95 % confidence interval.

Reaction k [×10−10 cm3 s−1] Method p [Torr]
(1) CH2OO+HCOOH 1.1±0.1 MPIMS 4
1.1±0.1 UV 5
(2) CH2OO+CH3COOH 1.3±0.1 MPIMS 4
1.2±0.1 UV 5
(3) anti-CH3CHOO+HCOOH 5±3 MPIMS 4
(4) syn-CH3CHOO+HCOOH 2.5±0.3 MPIMS 4
(5) anti-CH3CHOO+CH3COOH 2.5±0.6 MPIMS 4
(6) syn-CH3CHOO+CH3COOH 1.7±0.5 MPIMS 4

No direct measurements of CI+carboxylic acid reactions exist in the literature. However, Neeb et al.[7] derived a ratio of k1 to the rate coefficient for Reaction (7)

graphic file with name anie0053-4547-m7.jpg (7)

of k1/k7≈14 000 at 293 K and 730 Torr from ethylene ozonolysis experiments in the presence of water vapor. Taking k7<9×10−17 cm3 s−1,[4b] this ratio would yield k1<1.3×10−12 cm3 s−1. By adding acetic acid to the O3/2-methylbut-2-ene system Johnson et al.[5a] derived k(CI+CH3COOH)<1×10−14 cm3 s−1. The present rate coefficients are more than two orders of magnitude larger than these literature upper limits. However, recent ozonolysis measurements[8] show CI reactions with acids to be about three times faster than the rapid[3,4d] reaction with SO2. Quantum-chemical studies suggest that the CH2OO+HCOOH reaction proceeds through barrierless association to hydroperoxymethyl formate (HPMF, HC(O)OCH2OOH), with no stable “pre-reactive” complex identified.[9] The slower CI reactions with aldehydes and ketones,[4c] do exhibit reactant-channel van der Waals complexes that may affect the overall kinetics.[10] The large CI+acid rate coefficients corroborate the absence of an entrance barrier and suggest that the bottlenecks to reaction of CI with carbonyl groups are absent in reaction of CI with acids. Facile transfer of the acidic -OH hydrogen to the basic terminal O atom of the CI, forming the hydroperoxyalkyl carboxylate (e.g., HPMF), may act to prevent any kinetically significant entrance-channel complex.

Reliable kinetics information for individual CI reactions can be difficult to obtain from ozonolysis experiments owing to its inherent complexity,[2] and large removal rate coefficients in the direct determinations suggest reinterpretation of earlier ozonolysis measurements.[5a,7,11] However, the consequences of the reaction of CI with acids in indirect ozonolysis experiments will depend on the products of the reactions. Ozonolysis experiments by Neeb et al.[11] found evidence that the CH2OO+HCOOH reaction forms HPMF, which subsequently dehydrates to formic anhydride (FAN, (CHO)2O). As discussed in the Supporting Information, no significant product signal is detected at the parent masses of HPMF (m/z=92) and FAN (m/z=74). However, signal observed at m/z=64 and m/z=31 might arise from dissociative ionization of HPMF or from hydroperoxymethanol (HOCH2OOH, m/z=64). For reactions (2)–(6), no significant product signal appears at the parent masses of the CI–acid adducts, although ion signals are observed that may arise from dissociative ionization of these adducts. Further work is necessary to characterize products from the CI+acids reactions.

The large rate coefficients determined here suggest that CIs could be important reaction partners for organic acids, and that reaction with organic acids could compete with unimolecular decay and reaction with water as key loss processes for CIs under some conditions. A simple comparison of loss rates (Table S2) considers CH2OO+H2O [R (7)] alongside Reactions (8) and (9).

graphic file with name anie0053-4547-m8.jpg (8)
graphic file with name anie0053-4547-m9.jpg (9)

Assuming values for k7 of 1×10−16 cm3 s−1 or 1×10−17 cm3 s−1,[2,4b] setting k8 to 100 s−1, and applying values of k9 of 1×10−10 cm3 s−1 or 5×10−10 cm3 s−1 suggests that removal by organic acids (RCOOH) will become significant for CIs at acid levels of around 1 ppb (Table S2). Such levels have been observed in forest environments,[12] in urban outflow,[13] and also in urban environments,[14] where a direct emission source from vehicles has been inferred.

The analysis of Vereecken et al.,[6] which employs smaller estimates of k8, predicted CH2OO and anti-CH3CHOO to be principally consumed by reactions with H2O or (H2O)2. For the reaction of CIs with acids, Vereecken et al.[6] assumed a lumped rate coefficient of 5×10−12 cm3 s−1. Using k1=1.1×10−10 cm3 s−1 as a proxy for all CH2OO+acids reactions, and using the most recent rate coefficients[4b] for the reaction with water, k7<9×10−17 cm3 s−1 (cf. 5.6×10−15 cm3 s−1 in Ref. [6]) and with the water dimer, k(CH2OO+(H2O)2)<3×10−13 cm3 s−1 (deduced from Ref. [4b] and the 2 H2O⇌(H2O)2 equilibrium constant; cf. 1×10−10 cm3 s−1 in Ref. [6]), predicts that in the boreal forest environment 10 % of CH2OO react with acids. The impact of acid reactions would be relatively larger for syn-CH3CHOO, which reacts much more slowly with water.[15] The present results suggest that all rate coefficients for reaction of a CI with a carboxylic acid are on the order of 1×10−10 cm3 s−1. If so, it is very likely that reaction with acids will be a significant loss process for larger CIs.

The effect of these reactions on the acid concentrations is shown by surface HCOOH fields derived from a global model integration, assuming an even more conservative k8=150 s−1 (Figure 3). The reaction with CIs contributes substantially to organic acid removal in equatorial regions, and also in some northern high latitude locations (where the model generates elevated terpene levels). This model is too coarse to interrogate urban environments, where there may also be elevated levels of CIs[16] and hence a substantial reduction in organic acid lifetime. The indoor environment is another region where CI reactions with organic acids may be important;[2] recent estimates[17] suggest that peak indoor CI levels could be in the region of 105 or even 106 cm−3.

Figure 3.

Figure 3

Ratio of formic acid concentration predicted using the present rate coefficients for reaction of CIs with organic acids (case 2, Table S1) to the concentration from a base model neglecting CI reactions with acids.

Reactions of CIs with acids may lead to adduct formation; preliminary calculations suggest that these adducts may have lower vapor pressures than the reactants, as shown in Table S3. If the products are more condensable than the parent acid these reactions could contribute to SOA formation. Quantification of reaction products and rate coefficients as a function of the structure are needed before the impact of CI reactions with carboxylic acids on SOA can be fully assessed. Nevertheless, the increased removal rates indicated by the present direct kinetics determinations imply that environmental sources of organic acids must be correspondingly larger to agree with field measurements.

Supporting information for this article is available on the WWW under http://dx.doi.org/10.1002/anie.201400964.

anie0053-4547-sd1.pdf (642.5KB, pdf)

References

  • [1].Sander W. Angew. Chem. 2014;126:370–372. [Google Scholar]; Angew. Chem. Int. Ed. 2014;53 [Google Scholar]
  • [2].Taatjes CA, Shallcross DE, Percival CJ. Phys. Chem. Chem. Phys. 2014;16:1704–1718. doi: 10.1039/c3cp52842a. [DOI] [PubMed] [Google Scholar]
  • [3].Welz O, Savee JD, Osborn DL, Vasu SS, Percival CJ, Shallcross DE, Taatjes CA. Science. 2012;335:204–207. doi: 10.1126/science.1213229. [DOI] [PubMed] [Google Scholar]
  • [4a].Sheps L. J. Phys. Chem. Lett. 2013;4:4201–4205. doi: 10.1021/jz402191w. [DOI] [PubMed] [Google Scholar]
  • [4b].Stone D, Blitz M, Daubney L, Howes NUM, Seakins P. Phys. Chem. Chem. Phys. 2014;16:1139–1149. doi: 10.1039/c3cp54391a. [DOI] [PubMed] [Google Scholar]
  • [4c].Taatjes CA, Welz O, Eskola AJ, Savee JD, Osborn DL, Lee EPF, Dyke JM, Mok DWK, Shallcross DE, Percival CJ. Phys. Chem. Chem. Phys. 2012;14:10391. doi: 10.1039/c2cp40294g. [DOI] [PubMed] [Google Scholar]
  • [4d].Taatjes CA, Welz O, Eskola AJ, Savee JD, Scheer AM, Shallcross DE, Rotavera B, Lee EPF, Dyke JM, Mok DKW, Osborn DL, Percival CJ. Science. 2013;340:177–180. doi: 10.1126/science.1234689. [DOI] [PubMed] [Google Scholar]
  • [5a].Johnson D, Lewin AG, Marston G. J. Phys. Chem. A. 2001;105:2933–2935. [Google Scholar]
  • [5b].Neeb P, Horie O, Moortgat GK. Int. J. Chem. Kinet. 1996;28:721–730. [Google Scholar]
  • [5c].Tobias HJ, Ziemann PJ. J. Phys. Chem. A. 2001;105:6129–6135. [Google Scholar]
  • [6].Vereecken L, Harder H, Novelli A. Phys. Chem. Chem. Phys. 2012;14:14682–14695. doi: 10.1039/c2cp42300f. [DOI] [PubMed] [Google Scholar]
  • [7].Neeb P, Sauer F, Horie O, Moortgat GK. Atmos. Environ. 1997;31:1417–1423. [Google Scholar]
  • [8].Sipilä M, Jokinen T, Berndt T, Richters S, Makkonen R, Donahue NM, III RLMauldin, Kurten T, Paasonen P, Sarnela N, Ehn M, Junninen H, Rissanen MP, Thornton J, Stratmann F, Herrmann H, Worsnop DR, Kulmala M, Kerminen V-M, Petäjä T. Atmos. Chem. Phys. 2014;14:3071–3098. [Google Scholar]
  • [9a].Aplincourt P, Ruiz-Lopez MF. J. Phys. Chem. A. 2000;104:380–388. [Google Scholar]
  • [9b].Long B, Cheng J-R, Tan X-f, Zhang W-j. J. Mol. Struct. Theochem. 2009;916:159–167. [Google Scholar]
  • [10].Jalan A, Allen JW, Green WH. Phys. Chem. Chem. Phys. 2013;15:16841–16852. doi: 10.1039/c3cp52598h. [DOI] [PubMed] [Google Scholar]
  • [11].Neeb P, Horie O, Moortgat GK. J. Phys. Chem. A. 1998;102:6778–6785. [Google Scholar]
  • [12].Sanhueza E, Figueroa L, Santana M. Atmos. Environ. 1996;30:1861–1873. [Google Scholar]
  • [13a].Grosjean D. Atmos. Environ. 1992;26:3279–3286. [Google Scholar]
  • [13b].Le Breton M, Bacak A, Muller J, Xiao P, Shallcross B, Batt R, Cooke MC, Shallcross DE, Bauguitte SJ-B, Percival CJ. Atmos. Environ. 2014;83:166–175. [Google Scholar]
  • [13c].Le Breton M, McGillen MR, Muller J, Shallcross DE, Xiao P, Huey LG, Tanner D, Percival CJ. Atmos. Meas. Tech. 2012;5:3029–3039. [Google Scholar]
  • [14].Bannan TJ, Bacak A, Muller J, Booth AM, Jones B, Le Breton M, Leather KE, Ghalaieny M, Xiao P, Shallcross DE, Percival CJ. Atmos. Environ. 2014;83:301–310. [Google Scholar]
  • [15].Anglada JM, Gonzalez J, Torrent-Sucarrat M. Phys. Chem. Chem. Phys. 2011;13:13034–13045. doi: 10.1039/c1cp20872a. [DOI] [PubMed] [Google Scholar]
  • [16].Percival C, Welz O, Eskola AJ, Savee JD, Osborn DL, Topping DO, Lowe D, Utembe S, Bacak A, McFiggans G, Cooke M, Archibald AT, Jenkin M, Derwent RG, Riipinen I, Mok D, Lee EPF, Dyke J, Taatjes CA, Shallcross DE. Faraday Discuss. 2013;165:45–73. doi: 10.1039/c3fd00048f. [DOI] [PubMed] [Google Scholar]
  • [17].D. E. Shallcross, C. A. Taatjes, C. J. Percival, Indoor Air2014in press. [DOI] [PubMed]

Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

anie0053-4547-sd1.pdf (642.5KB, pdf)

Articles from Angewandte Chemie (International Ed. in English) are provided here courtesy of Wiley

RESOURCES