Scott A. Epstein

Adventures in ozoneland: down the rabbit-hole

In this perspective we describe a 15 year pursuit of the Stabilized Criegee Intermediate (SCI). We have conducted several complementary experiments to measure the pressure dependence of product yields-including OH radical and ozonides-on sequences of alkene + ozone systems. In so doing we have been able to bring into gradual focus a succession of weakly bound intermediates, starting with the primary ozonide, then the SCI, and finally a vinyl hydroperoxide (VHP) product of SCI rearrangement. We have narrowed the phase space in our hunt for direct SCI observations to a range of alkene carbon numbers and system pressures, but the system continues to deliver surprises. One surprise is strong evidence that the VHP is a significant bottleneck along the reaction coordinate. These findings support the search for the SCI, build our fundamental understanding of collisional energy transfer in highly excited, multiple-well, chemically activated systems, and finally directly inform atmospheric chemistry on topics including HO(x) radical formation and reactions associated with secondary organic aerosol formation.

A Semiempirical Correlation between Enthalpy of Vaporization and Saturation Concentration for Organic Aerosol

To model the temperature-induced partitioning of semivolatile organics in laboratory experiments or atmospheric models, one must know the appropriate heats of vaporization. Current treatments typically assume a constant value of the heat of vaporization or else use specific values from a small set of surrogate compounds. With published experimental vapor-pressure data from over 800 organic compounds, we have developed a semiempirical correlation between the saturation concentration (C*, microg m(-3)) and the heat of vaporization (deltaH(VAP), kJ mol(-1)) for organics in the volatility basis set. Near room temperature, deltaH(VAP) = -11 log(10)C(300)(*) + 129. Knowledge of the relationship between C* and deltaH(VAP) constrains a free parameter in thermodenuder data analysis. A thermodenuder model using our deltaH(VAP) values agrees well with thermal behavior observed in laboratory experiments.

Why do organic aerosols exist? Understanding aerosol lifetimes using the two-dimensional volatility basis set

Environmental context Fine particles (aerosols) containing organic compounds are central players in two important environmental issues: aerosol-climate effects and human health effects (including mortality). Although organics constitute half or more of the total fine-particle mass, their chemistry is extremely complex; of critical importance is ongoing oxidation chemistry in both the gas phase and the particle phase. Here we present a method for representing that oxidation chemistry when the actual composition of the organics is not known and show that relatively slow oxidant uptake to particles plays a key role in the very existence of organic aerosols. Abstract Organic aerosols play a critical role in atmospheric chemistry, human health and climate. Their behaviour is complex. They consist of thousands of organic molecules in a rich, possibly highly viscous mixture that may or may not be in phase equilibrium with organic vapours. Because the aerosol is a mixture, compounds from all sources interact and thus influence each other. Finally, most ambient organic aerosols are highly oxidised, so the molecules are secondary products formed from primary emissions by oxidation chemistry and possibly non-oxidative association reactions in multiple phases, including gas-phase oxidation, aqueous oxidation, condensed (organic) phase reactions and heterogeneous interactions of all these phases. In spite of this complexity, we can make a strong existential statement about organic aerosol: They exist throughout the troposphere because heterogeneous oxidation by OH radicals is more than an order of magnitude slower than comparable gas-phase oxidation.

Direct photolysis of α-pinene ozonolysis secondary organic aerosol: effect on particle mass and peroxide content.

Primary and secondary organic aerosols (POA and SOA) contain a complex mixture of multifunctional chemicals, many of which are photolabile. Much of the previous work that aimed to understand the chemical evolution (aging) of POA and SOA has focused on the reactive uptake of gas-phase oxidants by particles. By stripping volatile compounds and ozone from α-pinene ozonolysis SOA with three 1-m-long denuders, and exposing the residual particles in a flow cell to near-ultraviolet (λ>300 nm) radiation, we find that condensed-phase photochemistry can induce significant changes in SOA particle size and chemical composition. The particle-bound organic peroxides, which are highly abundant in α-pinene ozonolysis SOA (22 ± 5% by weight), have an atmospheric photolysis lifetime of about 6 days at a 24-h average solar zenith angle (SZA) of 65° experienced at 34° latitude (Los Angeles) in the summer. In addition, the particle diameter shrinks 0.56% per day under these irradiation conditions as a result of the loss of volatile photolysis products. Experiments with and without the denuders show similar results, suggesting that condensed-phase processes dominate over heterogeneous reactions of particles with organic vapors, excess ozone, and gas-phase free radicals. These condensed-phase photochemical processes occur on atmospherically relevant time scales and should be considered when modeling the evolution of organic aerosol in the atmosphere.

Experimental and Theoretical Study of Aqueous cis-Pinonic Acid Photolysis

Direct aqueous photolysis of cis-pinonic acid (PA; 2-(3-acetyl-2,2-dimethylcyclobutyl)acetic acid; CAS Registry No. 473-72-3) by 280-400 nm radiation was investigated. The photolysis resulted in Norrish type II isomerization of PA leading to 3-isopropenyl-6-oxoheptanoic acid (CAS Registry No. 4436-82-2), also known as limononic acid, as the major product, confirmed by (1)H and (13)C NMR analysis, chemical ionization mass spectrometry, and electrospray ionization mass spectrometry. Several minor products resulting from Norrish type I splitting of PA were also detected. The molar extinction coefficients of aqueous PA were measured and used to calculate the photolysis quantum yield of aqueous PA as 0.5 ± 0.3 (effective average value over the 280-400 nm range). The gas-phase photolysis quantum yield of 0.53 ± 0.06 for PA methyl ester (PAMe; CAS Registry No. 16978-11-3) was also measured for comparison. These results indicate that photolysis of PA is not significantly suppressed by the presence of water. This fact was confirmed by photodissociation dynamics simulations of bare PA and of PAMe hydrated with one or five water molecules using on-the-fly dynamics simulations on a semiempirical potential energy surface. The calculations correctly predicted the occurrence of both Norrish type I and Norrish type II photolysis pathways, both driven by the dynamics on the lowest triplet excited state of PA and PAMe. The rate of removal of PA by direct aqueous photolysis in cloudwater and in aerosol water was calculated for a range of solar zenith angles and compared with rates of other removal processes such as gas-phase oxidation by OH, aqueous-phase oxidation by OH, and gas-phase photolysis. Although the direct photolysis mechanism was not the most significant sink for PA in cloud and fog droplets, direct photolysis can be expected to contribute to removal of PA and more soluble/less volatile biogenic oxidation products in wet particulate matter.

Physical properties of ambient and laboratory‐generated secondary organic aerosol

The size and thickness of organic aerosol particles collected by impaction in five field campaigns were compared to those of laboratory-generated secondary organic aerosols (SOA). Scanning transmission X-ray microscopy was used to measure the total carbon absorbance (TCA) by individual particles as a function of their projection areas on the substrate. Particles with higher viscosity/surface tension can be identified by a steeper slope on a plot of TCA versus size because they flatten less upon impaction. The slopes of the ambient data are statistically similar indicating a small range of average viscosities/surface tensions across five field campaigns. Steeper slopes were observed for the plots corresponding to ambient particles, while smaller slopes were indicative of the laboratory-generated SOA. This comparison indicates that ambient organic particles have higher viscosities/surface tensions than those typically generated in laboratory SOA studies.

Absorption Spectra and Photolysis of Methyl Peroxide in Liquid and Frozen Water

Methyl peroxide (CH(3)OOH) is commonly found in atmospheric waters and ices in significant concentrations. It is the simplest organic peroxide and an important precursor to hydroxyl radical. Many studies have examined the photochemical behavior of gaseous CH(3)OOH; however, the photochemistry of liquid and frozen water solutions is poorly understood. We present a series of experiments and theoretical calculations designed to elucidate the photochemical behavior of CH(3)OOH dissolved in liquid water and ice over a range of temperatures. The molar extinction coefficients of aqueous CH(3)OOH are different from the gas phase, and they do not change upon freezing. Between -12 and 43 °C, the quantum yield of CH(3)OOH photolysis is described by the following equation: Φ(T) = exp((-2175 ± 448)1/T) + 7.66 ± 1.56). We use on-the-fly ab initio molecular dynamics simulations to model structures and absorption spectra of a bare CH(3)OOH molecule and a CH(3)OOH molecule immersed inside 20 water molecules at 50, 200, and 220 K. The simulations predict large sensitivity in the absorption spectrum of CH(3)OOH to temperature, with the spectrum narrowing and shifting to the blue under cryogenic conditions because of constrained dihedral motion around the O-O bond. The shift in the absorption spectrum is not observed in the experiment when the CH(3)OOH solution is frozen suggesting that CH(3)OOH remains in a liquid layer between the ice grains. Using the extinction coefficients and photolysis quantum yields obtained in this work, we show that under conditions with low temperatures, in the presence of clouds with a high liquid-water content and large solar zenith angles, the loss of CH(3)OOH by aqueous photolysis is responsible for up to 20% of the total loss of CH(3)OOH due to photolysis. Gas phase photolysis of CH(3)OOH dominates under all other conditions.

The kinetics of tetramethylethene ozonolysis: decomposition of the primary ozonide and subsequent product formation in the condensed phase.

We report data from real-time FTIR temperature programmed reaction spectroscopy on a cryogenic zinc selenide window revealing the intermediates from ozonation of 2,3-dimethyl-2-butene (TME). We have found convincing evidence of a 1,2,3-trioxolane (the primary ozonide, POZ), which decomposes at 185 K to yield a 1,2,4-trioxolane product (the secondary ozonide, SOZ). Computational infrared spectra confirmed the presence of the POZ and SOZ. The barrier height for POZ decomposition, determined experimentally, was found to be 13.8 +/- 1.0 kcal mol(-1), and the A factor calculated with RRKM theory based on density functional reactant and transition state frequencies was found to be 4.16 x 10(13) s(-1). The TME SOZ has not previously been observed without the presence of a polyethylene surface. SOZ formation kinetics from the reaction of the POZ decomposition products along with the competing reaction pathways were examined with computational chemistry calculations using DFT. These calculations confirm our experimental observation of SOZ formation.

Ozonolysis of cyclic alkenes as surrogates for biogenic terpenes: primary ozonide formation and decomposition.

Alkene ozonolysis reactions proceed through an unstable intermediate, the primary ozonide (POZ). POZ decomposition controls the complex mechanism. We probe the kinetics of primary ozonide decomposition using temperature programmed reaction spectroscopy (TPRS), revealing primary ozonide decomposition barrier heights of 9.1 +/- 0.4, 9.4 +/- 0.4, and 11.9 +/- 1.2 kcal mol(-1) for cyclohexene, 1-methyl-cyclohexene, and methylene-cyclohexane, respectively. We compare experimental decomposition spectra with spectral predictions using density functional theory (DFT) to reveal decomposition products resembling vinyl-hydroperoxides and dioxiranes. We do not find evidence of secondary ozonides. Additional computations with DFT, scaled with the TPRS barrier height, yield barrier heights ranging from 9.4 to 12.1 kcal mol(-1) for the four competing decomposition pathways of the 1-methyl-cyclohexene POZ. Entropic differences were minimal, indicating that POZ decomposition branching is controlled purely by enthalpic variations. These kinetic computations were used to calculate a hydroxyl radical yield for 1-methyl-cyclohexene ozonolysis of 0.85 at 298 K.

Wall effects in smog chamber experiments: A model study

ABSTRACT Wall losses of condensable organic vapors are a significant complication for smog-chamber experiments designed to constrain production of Secondary Organic Aerosols (SOA). Here we develop a dynamical mass-balance model based on the Volatility Basis Set (VBS) to explore various pathways for mass transfer between the bulk of a smog-chamber volume (the vapors and suspended particles) and reservoirs near the chamber walls (deposited and/or nucleated particles on the walls, adsorption to the walls, and sorption into Teflon walls). We consider various limiting cases and explore the sensitivity of inferred SOA yields to assumptions about the actual parameters in a given SOA experiment. We also present data suggesting that adsorptive uptake to Teflon for typical SOA is modest. Broadly, we find that walls become a sink for condensable vapors when those vapors interact with either deposited particles of the Teflon walls, with qualitatively similar effects on the suspended particles. Finally, we show that having a relatively high seed condensation sink is vital to reliable chamber mass balances. Copyright