Formation reaction mechanism and infrared spectra of anti-trans-methacrolein oxide and its associated precursor and adduct radicals
Methacrolein oxide (MACRO) is an important carbonyl oxide produced in ozonolysis of isoprene, the most abundantly-emitted non-methane hydrocarbon in the atmosphere. We employed a step-scan Fourier-transform infrared spectrometer to investigate the source reaction of MACRO in laboratories. Upon UV irradiation of precursor CH 2 IC(CH 3 )CHI (1), the CH 2 C(CH 3 )CHI radical (2) was detected, confirming the fission of the allylic C-I bond rather than the vinylic C-I bond. Upon UV irradiation of (1) and O 2 near 21 Torr, anti-trans-MACRO (3a) was observed to have an intense OO-stretching band near 917 cm −1 , much greater than those of syn-CH 3 CHOO and (CH 3 ) 2 COO, supporting a stronger O-O bond in MACRO because of resonance stabilization. At increased pressure (86-346 Torr), both reaction adducts CH 2 C(CH 3 )CHIOO (4) and (CHI)C(CH 3 )CH 2 OO (5) radicals were observed, indicating that O 2 can add to either carbon of the delocalized propenyl radical moiety of (2). The yield of MACRO is significantly smaller than other carbonyl oxides.
<!>Results and discussion<!>Conclusion<!>Methods
<p>I soprene [2-methyl-1,3-butadiene, CH 2 = CH-C(CH 3 ) = CH 2 ] is the most abundantly emitted non-methane volatile organic compound (VOC) emitted into Earth's atmosphere; an emission budget ~530 Tg year −1 , ~70% of the total biogenic VOC emission, was estimated 1,2 . Ozone is responsible for the removal of ~10% of isoprene 3,4 . The ozonolysis of isoprene produces three carbonyl oxides (so-called Criegee intermediates); formaldehyde oxide (CH 2 OO), methyl vinyl ketone oxide [MVKO, C 2 H 3 C (CH 3 )OO], and methacrolein oxide [MACRO, CH 2 C(CH 3 ) CHOO] are produced with estimated branching ratios 58, 23, and 19%, respectively 3,5,6 .</p><p>Previously, detecting carbonyl oxides from ozonolysis of alkenes in laboratories was difficult because these source reactions are slow but the carbonyl oxides thus produced are highly reactive. Welz et al. reported an original reaction scheme to generate the simplest carbonyl oxide CH 2 OO in laboratories from the reaction of CH 2 I with O 2 on photolysis of CH 2 I 2 in O 2 with ultraviolet (UV) light 7 . Further extension of this scheme to produce substituted carbonyl oxides has promoted active research, as discussed in several reviews [8][9][10][11][12][13][14] .</p><p>To produce MACRO, CH 2 C(CH 3 )CHOO, following this method from photolysis of CH 2 C(CH 3 )CHI 2 in O 2 is, however, difficult because this precursor is extremely unstable. Vansco et al. reported a unique method to produce MACRO on photolysis at 248 nm of a gaseous mixture of 1,3-diiodo-2-methyl-prop-1-ene [CH 2 IC(CH 3 )CHI] (1) and O 2 that was pulsed into a quartz capillary reactor tube 15 . These authors assumed that photolysis of CH 2 IC(CH 3 )CHI (1) at 248 nm resulted in a preferential dissociation of the allylic, rather than the vinylic, C-I bond, to form the iodoalkenyl radical 3-iodo-2-methyl-prop-1en-3-yl [CH 2 C(CH 3 )CHI] (2). Subsequent addition of O 2 with this resonance-stabilized radical (2) to form adduct 3-hydroperoxy-3-iodo-2-methyl-prop-1-ene CH 2 C(CH 3 )CHIOO (4) that readily breaks the remaining C-I bond to produce the carbonyl oxide MACRO (3). A detailed reaction scheme appears in Fig. 1; the chemical formula and labels of key species are also presented. Four conformers of MACRO, anti-trans, syn-cis, syn-trans, and anti-cis (with increasing energy, shown in Fig. 1) are predicted to exist; syn-and anti-indicate the orientation of the CH 2 = C(CH 3 ) moiety relative to the terminal oxygen atom, and cis-and transindicate the relative orientation of the C = C bond and the C = O bond. The UV-visible spectrum of jet-cooled MACRO was obtained by means of UV-visible depletion of the parent ion signal of MACRO at m/e = 86 upon photoionization at 10.5 eV 15 , but this spectrum with maximum absorption near 380 nm provides no specific information on the conformation of MACRO; equal populations of the conformers were assumed because these four conformers were predicted to have energies within 13.3 kJ mol −1 according to the CCSD(T)-F12/CBS(TZ-F12,QZ-F12)// B2PLYP-D3/cc-pVTZ method 15 . Lin et al. reported the direct UV-visible absorption spectrum of MACRO with a maximum at 397 nm upon photoirradiation of the same precursors at 248 nm and 298 K 16 . Unlike MVKO 17 , the near-infrared action spectra of MACRO could not be obtained by probing OH radicals because OH is not a significant reaction product. The mechanism for the formation of MACRO, including the characterization of the associated iodoalkenyl radical (2) before its reaction with O 2 and the iodoperoxy radical adducts (4) and (5) before the fission of the second C-I bond, has not been identified. The mid-infrared spectrum of MACRO and other related intermediates will provide a clue to the conformation of these species and a detailed mechanism for the production of MACRO from UV photolysis of (1) in O 2 .</p><p>We have previously employed a unique step-scan Fouriertransform infrared (FTIR) absorption technique to detect unstable species 18 . The wide spectral and temporal coverage enables us to monitor several reaction intermediates simultaneously; their temporal behavior provides valuable information to understand the detailed reaction mechanism. With this technique, we have successfully detected infrared spectra of carbonyl oxides CH 2 OO 19,20 , CH 3 CHOO 21 , (CH 3 ) 2 COO 22 , MVKO 23 , and the associated adduct CH 2 IOO 24 ; we explored also the mechanism and the intermediates in reactions of CH 2 OO with CH 2 OO 25 , SO 2 26 , HC(O)OH 27 , and HCl 28 . In this work, we extended our focus to MACRO and investigated the UV photodissociation of the precursor CH 2 IC(CH 3 ) CHI (1) to observe the CH 2 C(CH 3 )CHI radical (2), confirming that only the allylic C-I bond was broken. When oxygen at varied pressure was added, the IR spectra of the anti-trans-MACRO [CH 2 C(CH 3 )CHOO] (3a) and the adducts CH 2 C(CH 3 )CHIOO (4) and (CHI)C(CH 3 )CH 2 OO (5) radicals were characterized. The IR spectrum of MACRO indicates that the preferred conformation is anti-trans and provides direct spectral evidence for resonance stabilization and hyper-conjugation of MACRO.</p><!><p>Quantum-chemical calculations. Although Vansco et al. 15 has reported high-level calculations for conformers of MACRO, we performed calculations at the B3LYP/aug-cc-pVTZ level of theory mainly for predictions of vibrational wavenumbers and IR intensities of various conformers of MACRO and other associated species. As summarized in Supplementary Note 1, the optimized geometries and Cartesian coordinates of conformers of precursors (1), iodoalkenyl radicals CH 2 C(CH 3 )CHI (2) and CH 2 IC(CH 3 )CH (6), carbonyl oxides MACRO (3), a possible cyclic peroxide product dioxole from unimolecular isomerization of MACRO 29,30 , and iodoperoxy radical adducts (4) and (5) are presented in Supplementary Figs. 1-4 and Supplementary Tables 1-4. Relative energies of conformers are also listed in these figures and those of MACRO are compared with high-level calculations by Vansco et al. 15 .</p><p>Computed scaled harmonic vibrational wavenumbers and IR intensities of these species are listed in Supplementary Tables 5-9, respectively. The harmonic vibrational wavenumbers of all species discussed in this paper were scaled according to the equation y = 0.9683 x + 11.5, in which y and x are scaled and harmonic vibrational wavenumbers, respectively; this equation was derived on fitting the observed bands of precursor (1a) with computed harmonic vibrational wavenumbers. The average absolute deviation of scaled harmonic vibrational wavenumbers of (1a) from observed wavenumbers is 7.5 ± 6.4 cm −1 ; the error represents one standard deviation in the fitting. The computed anharmonic vibrational wavenumbers of the four conformers of MACRO, (3a)−(3d), and dioxole are also listed in Supplementary Table S7. The rotational parameters for each vibrational state of (3a)−(3d) are listed in Supplementary Table S10.</p><p>IR spectra of the iodoalkenyl radical CH 2 C(CH 3 )CHI (2). Precursor (1) is predicted to exist in (Z)-and (E)-conformations; the (E)-conformer (1a) is predicted to have energy 1.6 kJ mol −1 greater than the (Z)-conformer (1b) at the B3LYP/aug-cc-pVTZ level of theory. The IR spectra of (1a) and (1b) are shown in Supplementary Fig. 5 and their wavenumbers are listed in Supplementary Table 5. These spectra and results on photolysis (Fig. 2, same as Supplementary Fig. 6) are discussed in Supplementary Note 2. When precursor (1), a mixture of (1a) and (1b) with spectrum shown in Fig. 2a, was irradiated with light at 248 nm, the intensity of its bands decreased significantly and weak new features appeared (Fig. 2b). Processing these difference spectra (Fig. 2c-e) by adding back the loss of the precursor yielded Fig. 2f-h, as discussed in Supplementary Note 2; the regions in which the absorption of the precursor might interfere are marked with gray rectangles. Three features near 1312, 1178, and 778 cm −1 with greater intensities and two weak ones near 1364 and 1002 cm −1 appeared upon UV irradiation and decreased in intensity with reaction period following nearly the same proportions; these transient features in group A, marked as A 1 -A 5 in Fig. 2f, are associated with the primary photolysis product. Four features near 1380, 1084, 1014, and 902 cm −1 increased in intensity continuously; these features in group X, marked as X 1 -X 4 in Fig. 2h, are associated with the final product.</p><p>The spectrum consisting of bands in group A is reproduced in Fig. 3a as the red trace. A corresponding spectrum observed in experiments with (E)-CH 2 IC(CH 3 )CHI (1a) is shown as a black trace in Fig. 3a; these two traces are similar except that the red trace has a better signal-to-noise ratio (SNR). The stick IR spectra of both conformers of two possible photolysis products, (E)-and (Z)-CH 2 C(CH 3 )CHI, (2a) and (2b), and (E)-and (Z)-CH 2 IC(CH 3 )CH, (6a) and (6b), according to the scaled harmonic vibrational wavenumbers and intensities predicted with the B3LYP method are shown in Fig. 3b-e. The observed new features near 1364, 1312, 1178, 1002, and 778 cm −1 agree best, in terms of wavenumbers and relative intensities, with lines predicted near 1355, 1304, 1187, 1004, and 793 cm −1 for (2a), the conformer with the least energy; a small contribution of (2b) cannot be positively excluded because of the similarity in predicted spectra. A comparison of observed bands with calculations in this spectral region is presented in Table 1. In contrast, the observed features in group A agree poorly with the spectra predicted for (6a) and (6b). This observation of bands of (2) confirms that irradiation of (1) at 248 nm caused the breaking of the allylic C-I bond rather than the vinylic C-I bond. Furthermore, because the spectra observed after photolysis of (1a) and (1) are similar, we deduced that the conformation of (2) was scrambled upon UV photolysis of (1); the barrier to convert (2b) to (2a) is ~50 kJ mol −1 , much smaller than the excess energy ~300 kJ mol −1 at 248-nm photolysis. The calculated energy difference, ~1.5 kJ mol −1 , between (2a) and (2b) implies a population ratio 65:35 according to the Boltzmann distribution at 298 K, but the observed spectra seem to show a contribution of (2b) smaller than the predicted ratio if one considers that a doublet of similar intensity was predicted for the (Z)-conformer in region 1300-1350 cm −1 (Fig. 3c), but only one significant feature was observed. We are, however, uncertain about this population ratio because the predicted IR intensities might have large errors.</p><p>The product of dimerization of iodo-radicals (2) was also observed at a later period. Because of resonance, two forms 1iodo-2-methyl-prop-1-en-3-yl (2-1) and 3-iodo-2-methyl-prop-1-en-3-yl (2-2) might exist for (2), as shown in Fig. 4a for the Econformer as an example. Possible secondary reactions are shown in Fig. 4b-e, with diene products (7)− (10). The observed spectrum of the end product, group X, is reproduced in Fig. 5a and compared with predicted spectra of (7)− (10) in Fig. 5b-e. Observed bands in group X near 1380, 1084, 1014, and 902 cm −1 agree with scaled harmonic vibrational wavenumbers and relative intensities predicted near 1381, 1079, 1008, and 927 cm −1 for 3,4diiodo-2,5-dimethyl-hexa-1,5-diene (7), produced from dimerization of (2-2), shown in Fig. 4b. The observation of end product (7) further supports that only the allylic C-I bond rather than the vinylic C-I bond was broken upon irradiation at 248 nm, and that the radical thus produced, (2), exists in 3-iodo-2-methyl-prop-1en-3-yl (2-2) as its major form (in which C1-C4 has a double bond character), consistent with the predicted bond length of C1-C4 (1.380 Å) slightly smaller than that of C1-C2 (1.391 Å) for (2a); C1 is the central carbon atom and C2 is the carbon with the I atom, as labeled in Supplementary Fig. 1c.</p><p>IR spectrum of carbonyl oxide anti-trans-MACRO (3a). Results and data processing of photolysis of flowing mixtures of (1) (30 mTorr) and O 2 (20.0-21.0 Torr), recorded with external and internal ADC (with improved SNR), are presented in Supplementary Figs. 7 and 8 (reproduced as Fig. 6), respectively, and discussed in detail in Supplementary Note 3. Processing observed difference spectra recorded with an internal ADC (Fig. 6a-c) by removing contributions of (2) and end product methacrolein and adding back the loss of the precursor yielded Fig. 6d-f; the regions in which the absorption of the precursor might interfere are marked with gray rectangles. Further processing by taking out contributions of other stable products (Fig. 6f) produced cleaner spectra, as shown in Fig. 6g, h. Only one prominent band near 917 cm −1 showed a transient nature and attained its maximum 5-10 µs after irradiation; we mark this as B 1 in Fig. 6h. Weak features B 2 -B 4 near 1025, 1332, and 1386 cm −1 might also belong to  this group; as we are uncertain about these bands because of their small intensities and possible interference from absorption of the parent or the stable products, we indicate them with ? marks. The photolysis of a mixture of precursor (1) and O 2 at 248 nm is expected to produce carbonyl oxide MACRO (3), as reported by Vansco et al. 15 . The spectrum of group B in Fig. 6h is reproduced in Fig. 7a to compare with the simulated spectra of four conformers of the carbonyl oxides MACRO: anti-trans-, syncis-, syn-trans-, and anti-cis-CH 2 C(CH 3 )CHOO, (3a)−(3d), in Fig. 7b-e. We employed anharmonic vibrational wavenumbers (Supplementary Table 7) and rotational parameters (Supplementary Table 10) predicted with the B3LYP method and simulated the rotational contours with the PGOPHER program (Supplementary Figs. 9 and 10) 31 , as described in detail in the Supplementary Note 4. The spectrum of a possible product dioxole simulated according to anharmonic vibrational calculations is also shown in Fig. 7f for comparison.</p><p>Observed intense band B 1 near 917 cm −1 matches best with the spectrum simulated for anti-trans-MACRO (3a) in terms of vibrational wavenumbers and relative intensities. The OOstretching (ν 15 ) band of (3a) was predicted at 944 cm −1 and to have the largest IR intensity (201 km mol −1 ); other bands in region 850-1450 cm −1 have IR intensities less than 26 km mol −1 . For the four conformers, only (3a) was predicted to have a single intense band in this region; others were predicted to have more than two bands with comparable intensities. Furthermore, two ctype bands were predicted for modes ν 24 and ν 25 of (3a) near 950 and 924 cm −1 ; they might correspond to the small narrow features near 921 902 cm −1 , indicated with arrows in Fig. 7a; other conformers were predicted to have only one c-type band near 900 cm −1 . A comparison of observed bands with predicted vibrational wavenumbers and intensities of (3a) is listed in Table 2. The observed band near 917 cm −1 appears to have an insignificant Q-branch and a broader rotational contour as compared with that simulated with the PGOPHER program, presumably because of the contribution of hot bands from excited states of the low-energy vibrational modes. Similar broadening was observed for carbonyl oxides containing a methyl rotor, CH 3 CHOO 21 , (CH 3 ) 2 COO 22 , and MVKO 23 .</p><p>A small contribution of syn-cis-MACRO (3b), the second leastenergy conformer with energy 7.5 (3.8 from CCSD(T)-F12 15 ) kJ mol −1 greater than anti-trans-MACRO (3a), might be assigned to the observed weak bands B 2 -B 4 , but we are unable to confirm this definitively because of the small intensity and interference. The observed bands near 1025, 1332, and 1386 cm −1 agree satisfactorily with the more intense bands of (3b) predicted near 1030, 1346, and 1383 cm −1 . The band predicted near 907 cm −1 might overlap with band B 1 of (3a); two bands predicted near 980 cm −1 might suffer interference from the parent absorption, so they are unobserved.</p><p>The agreement of observed bands with those predicted for the syn-trans-and anti-cis-MACRO, (3c) and (3d), is less satisfactory. Considering the computed relative energies of these two conformers, 10.5 (13.4) and 13.3 (14.7) kJ mol −1 above (3a), our observation of predominant anti-trans-MACRO (3a) with a negligibly small contribution of (3c) and (3d) is reasonable; the listed energies are from CCSD(T)-F12 15 and B3LYP (listed parenthetically). The observed spectrum agrees poorly with that predicted for dioxole (Fig. 7f).</p><p>Resonance stabilization of MVKO and MACRO (3). We compared the lengths of bonds O-O and C-O and the OOstretching vibrational wavenumbers of (3a) with syn-trans-MVKO, syn-CH 3 CHOO, anti-CH 3 CHOO, and (CH 3 ) 2 COO in Table 3 to confirm the resonance stabilization of MVKO and MACRO. The O-O lengths 1.365 Å for (3a) and 1.353 Å for syntrans-MVKO are significantly smaller than those of other carbonyl oxides (~1.380 Å). The observed OO-stretching vibrational wavenumbers 917 cm −1 for (3a) and 948 cm −1 for syn-trans-MVKO are much greater than the corresponding values 871-887 cm −1 for other species. All this evidence supports that the COO moieties of MACRO and MVKO are resonance stabilized by the adjacent vinyl group so that the extended π-electron delocalization strengthens the O-O bond significantly; the major resonance structures of MACRO and MVKO are shown in Supplementary Fig. 11a and b, respectively; the major resonance structures for four conformers of MACRO are also depicted in Fig. 1. Furthermore, the molecular orbitals of MACRO and MVKO also show delocalization of π-electron densities over the CCCOO skeleton, as shown in Supplementary Fig. 11c for node = 0-2; a more complete set of molecular orbitals have been reported by Vansco et al. 15 .</p><p>That the observed vibrational wavenumber 917 cm −1 for the OO-stretching mode of (3a) is smaller than a value, 948 cm −1 , observed for MVKO can be explained with a concept of hyperconjugation generally employed in organic chemistry; this resonance structure is also shown in Supplementary Fig. 11a. In this hyper-conjugation structure, the O-O bond has single-bond character, whereas the adjacent C=O bond has double-bond character; this contribution explains that MACRO has a longer O-O bond length and a shorter C-O length, with R OO = 1.365 Å and R CO = 1.266 Å for MACRO and R OO = 1.353 Å and R CO = 1.297 Å for MVKO. Our observation of the OO-stretching wavenumbers of carbonyl oxides provided a direct spectral confirmation of the resonance stabilization and hyperconjugation of MACRO. Because of this resonance stabilization, a smaller reactivity of MACRO and MVKO was predicted and observed 16,32,33 .</p><p>Assignments of iodoperoxy radical adducts. Results on photolysis of a flowing mixture of (1) (60 mTorr) and O 2 (21-346 Torr)  are discussed in detail in Supplementary Note 5. Figure 8 (same as Supplementary Fig. 12) shows the results of experiments on CH 2 IC(CH 3 )CHI (1)/O 2 (0.060/334 Torr) in a flowing mixture. Details in processing observed difference spectra (Fig. 8b-d) by stripping bands of MACRO and methacrolein and adding back the decrease in precursor bands to obtain Fig. 8g-i are discussed in Supplementary Note 5; the regions in which the absorption of the precursor might interfere are marked with gray rectangles. Two sets of new bands were observed. Bands of group D near 1333, 1243, 990, and 886 cm −1 , marked D 1 -D 4 in Fig. 8i, are associated with a more stable intermediate; bands of group C near 1116, 1031, 914, and 888 cm −1 , marked C 1 -C 4 in Fig. 8j, are associated with a less stable intermediate, according to their temporal profiles.</p><p>For the simplest carbonyl oxide CH 2 OO, both CH 2 OO and the adduct ICH 2 OO were produced from UV photolysis of CH 2 I 2 + O 2 ; the yield of ICH 2 OO increased with pressure because the adduct was stabilized at high pressure 24 . Similarly, the adduct C 2 H 3 C(CH 3 )IOO was produced on photolysis of a mixture of the precursor of MVKO, (CH 2 I)HC = C(CH 3 )I, and O 2 at 248 nm at high pressure 23 . As discussed previously, photolysis of precursor (1) produces only CH 2 C(CH 3 )CHI (2), not CH 2 IC(CH 3 )CH (6); possible structures of the adducts are hence CH 2 C(CH 3 )CHIOO (4) or (CHI)C(CH 3 )CH 2 OO (5), with O 2 added to the carbon atom on either side of the delocalized propenyl radical moiety.</p><p>Six conformers exist for (4) (Supplementary Fig. 3). The conformer of least energy is designated (4a). Only conformer (4b) has energy within 3 kJ mol −1 of (4a); the other four conformers have energies 9-16 kJ mol −1 greater than (4a). Two conformers exist for (CHI)C(CH 3 )CH 2 OO (5) (Supplementary Fig. 4).</p><p>Conformer (5b) has energy 0.6 kJ mol −1 greater than (5a). The energy of (4a) is greater than that of (5a) by 2.6 kJ mol −1 .</p><p>The spectra of bands in groups C and D are reproduced in Fig. 9a, d, respectively. These spectra are compared with the predicted stick spectra of the two least-energy conformers CH 2 C(CH 3 )CHIOO, (4a) and (4b), in Fig. 9b, c, respectively, and the two conformers of (CHI)C(CH 3 )CH 2 OO, (5a) and (5b), and dioxole in Fig. 9e-g, respectively. Observed bands C 1 -C 4 near 1116, 1031, 914, and 888 cm −1 agree satisfactorily with the scaled harmonic vibrational wavenumbers predicted for the four most intense bands of (4a), near 1135, 1022, 937, and 902 cm −1 in this region (Table 4). We could not positively exclude a possible contribution of (4b) to the observed spectrum because of the similarity in predicted spectra. The other four conformers (4c) −(4 f) are expected to have insignificant contributions because of greater energy.</p><p>Observed bands D 1 -D 4 near 1333, 1243, 990, and 886 cm −1 agree satisfactorily with the four most intense bands of (CHI)C(CH 3 ) CH 2 OO (5a) predicted near 1332, 1280, 1034, and 889 cm −1 in this region (Table 4). Similarly, we could not exclude positively a possible contribution of (5b) to the observed spectrum of group D because of the similarity in predicted spectra. Neither spectrum of group C or D shows a satisfactory agreement with that predicted for dioxole, even though we cannot exclude the possibility that dioxole might contribute to part of band C 1 .</p><p>Adducts (4) and (5) correspond to the addition of O 2 to either carbon of the delocalized propenyl radical moiety of (2); this is the first case that both adducts were observed. Because the C-I bond in (4) is allylic, whereas that in (5) is vinylic, we expect that the dissociation of the C-I bond of (5) has a greater barrier; (5) is hence expected to be more stable, as was observed experimentally.</p><p>Relative yields of (3), (4), and (5) as a function of pressure. We performed similar experiments with O 2 at pressures near 21, 86, 229, and 346 Torr and recorded the spectra with an external digitizer. The processed spectra for 0-5 and 30-35 μs after photolysis are compared in Supplementary Fig. 13. We estimated the relative yields of (3), (4), and (5) at varied pressures using two methods, as discussed in Supplementary Note 6 and summarized in Supplementary Table 11. The relative variations in intensities derived from spectral stripping factors for bands in groups C and D (method I) are more reliable. For (3), the ratio relative to the experiment at 21.0 Torr remains similar (1.29-1.38) at 86-346 Torr. For (4) and (5), the ratios increase with pressure, with ratios 1.91 and 1.62 at 346 Torr, respectively; (4) increases more than (5). Unlike what was observed for CH 2 OO 24 and MVKO 23 , our experiments show no significant increase of (4) at the expense of (3) as pressure increases. Furthermore, even though the estimate might have large errors due to uncertainties in predicted IR intensities, the yield of MACRO (3a) from photolysis of the precursor is significantly smaller than other carbonyl oxides, in the range 6-8% as listed in Supplementary Table 11.</p><p>We calculated the potential-energy scheme for the source reaction with the CCSD(T)//B3LYP/aug-cc-pVTZ-pp method, as shown in Fig. 10. The formation of adducts (4a) and (5a) from (2a) + O 2 is exothermic by ~73 and 75 kJ mol −1 , respectively, whereas the formation of (3a) + I is endothermic by ~10 kJ mol −1 . This endothermicity might explain that MACRO was produced with a yield significantly smaller than other carbonyl oxides because other reactions are slightly exothermic. The smaller pressure effect for (5) than for (4) is consistent with a larger barrier for the C-I bond fission of (5). It is unclear, however, why the yield of MACRO did not decrease for pressure above 21 Torr. One possibility is that O 2 serves as a reactor instead of a quencher and some decomposition occurs at 21 Torr. Further investigations are needed to clarify this.</p><!><p>In the absence of O 2 , upon irradiation of gaseous precursor 1,3diiodo-2-methyl-prop-1-ene (1), CH 2 IC(CH 3 )CHI, at 248 nm, iodoalkenyl radical CH 2 C(CH 3 )CHI (2) was produced, as characterized with bands near 1364, 1312, 1178, 1002, and 778 cm −1 . This result provided direct spectral evidence to confirm that only the allylic C-I bond, not the vinylic C-I bond, dissociated upon photolysis through observation of only radical product (2), not (6), and only end product 3,4-diiodo-2,5-dimethyl-hexa-1,5diene (7), produced from the dimerization reaction of (2).</p><p>When O 2 at 21.0 Torr was added to the system, we report the identification of anti-trans-CH 2 C(CH 3 )CHOO (3a) with its intense infrared OO-stretching band near 917 cm −1 , whereas some weaker bands might be tentatively attributed to the syn-cisconformer (3b). The observation of a significantly larger OOstretching wavenumber provides also direct spectral support for a resonance stabilization of MACRO; a OO-stretching wavenumber smaller than that of its isomer MVKO is associated with the hyper-conjugation of MACRO that weakens the O-O bond slightly.</p><p>With O 2 at greater pressure, iodoperoxy radical adducts 3hydroperoxy-3-iodo-2-methyl-prop-1-ene (4), CH 2 C(CH 3 )CHIOO, characterized with infrared absorption bands at 1116, 1031, 914, and 888 cm −1 , and 3-hydroperoxy-1-iodo-2-methyl-prop-1-ene (5), (CHI)C(CH 3 )CH 2 OO, characterized with infrared absorption bands at 1333, 1243, 990, and 886 cm −1 , were observed. This spectral evidence shows O 2 can add to either end of the propenyl radical moiety in (2). As pressure increases, the yield of (3) remained small, whereas those of (4) and (5) increased; the enhancement with pressure was more for (4), consistent with the expectation that (5) has a much larger barrier for the C-I fission. The much smaller yield of (3) than for other carbonyl oxides produced from similar reaction schemes is explained by a small endothermicity for the formation of (3) + I from (2) + O 2 ; formation reactions of other carbonyl oxides are slightly exothermic.</p><p>The IR spectra of these four intermediates (2)−( 5) are new; they provide valuable information to probe the associated species  to understand the mechanism for the formation of carbonyl oxide MACRO from the source reaction. These spectral detections are also valuable to probe anti-trans-MACRO and associated adducts to investigate reactions of MACRO with atmospheric species in laboratories, even though the limited detectivity of this technique and the small yield of MACRO might require a much greater proportion of the precursor.</p><!><p>Experimental. The step-scan Fourier-transform infrared (FTIR) absorption technique is described in detail elsewhere 18,19 . A White cell of effective path length 3.6 m (base length 15 cm) and volume ~1370 cm 3 was installed on the external port of the spectrometer to serve as a reactor and an absorption cell. A KrF excimer laser (248 nm, 6-11 Hz, ≈ 230 mJ pulse −1 , beam size 1.2 × 9.3 cm 2 ) was employed to photodissociate either pure (E)-CH 2 IC(CH 3 )CHI (1a) or a mixture of (E)-CH 2 IC(CH 3 )CHI (1a) and (Z)-CH 2 IC(CH 3 )CHI (1b), denoted</p><p>. The photolysis laser beam was multiply reflected between a pair of external laser mirrors and propagated sideways, nearly perpendicular to the IR beams in the White cell.</p><p>The IR probe light from the FTIR spectrometer was detected with a HgCdTe detector at 77 K; the signal was sent to an external 14-bit digitizer with a temporal resolution 4 ns. Period 40 μs (10,000 data points) was typically covered. In some cases, an internal 24-bit digitizer (temporal resolution 12.5 µs) was used to cover a longer period with an improved SNR. We employed appropriate optical filters to limit the spectral region so as to perform undersampling to decrease the dataacquisition time. For spectral range 753-1504 cm −1 at instrumental resolution 1 cm −1 , 1523 scan steps (each averaged with 6-11 laser shots) were completed in ≈50 min. The spectral width (full width at half maximum) after apodization with the Blackman-Harris 3-term function is 1.28 times the listed instrumental resolution. In all, 3-7 spectra accumulated under similar conditions were averaged to yield a spectrum with a satisfactory SNR.</p><p>The liquid sample of (1) was placed in a dark flask at 298 K; a stream of gaseous N 2 or O 2 was passed over the sample to carry the vapor into the reactor. The partial pressures of (1) were estimated with Beer's law using the observed integrated absorbance of IR bands in regions 1362-1412, 1272-1301, 759-791 cm -1 , and calculated IR intensities. The average photolysis fraction of (1) was estimated to be typically ~19% according to its decrease in infrared absorbance. The decrease of the precursor upon irradiation was estimated to be (8.9-11.1) × 10 13 molecule cm −3 . The flow rates were F N2 ≈ 21.4 STP cm 3 s -1 (STP denotes standard temperature 273 K and pressure 1 atm) or F O2 ≈ 21.1-73.9 STP cm 3 s −1 . Partial pressures were P CH2IC(CH3)CHI ≈ 32-55 mTorr, P N2 ≈ 20.0 Torr, or P O2 = 21.0-346 Torr. (E)-CH 2 IC(CH 3 )CHI (1a) (>95%, Accela ChemBio), 1:1 mixture of (E)-/(Z)-CH 2 IC(CH 3 )CHI (1) (>97%, Accela ChemBio, the ratio of conformation was determined with NMR), N 2 (99.9995%, Chiah-Lung), and O 2 (99.99%, Chiah-Lung) were used as received. In this paper, we denote the mixture of conformers (E)-/(Z)-CH 2 IC(CH 3 )CHI as CH 2 IC(CH 3 )CHI or (1); the mixture is significantly more economical than (1a).</p><p>Computational. Quantum-chemical calculations were performed with the Gaussian 16 program suite 34 . The equilibrium geometry, rotational parameters, harmonic vibrational wavenumbers, and IR intensities of all conformers of precursor (1), isomers of CH 2 C(CH 3 )CHI (2) and CH 2 IC(CH 3 )CH (6), MACRO (3), dioxole, and the iodoperoxy adducts CH 2 C(CH 3 )CHIOO (4) and (CHI)C(CH 3 )CH 2 OO (5) were computed with the B3LYP density-functional theory (DFT), which uses Becke's three-parameter hybrid exchange functional with a correlation functional of Lee et al. [35][36][37] . The anharmonic vibrations were calculated for isomers of MACRO with a second-order perturbation approach using an effective finite-difference evaluation of the third and semi-diagonal fourth derivatives; as MACRO contains no I atom, anharmonic vibrational calculations for these species are more practical. In both methods, the standard Dunning's correlation-consistent basis set augmented with diffuse functions, aug-cc-pVTZ, was used 38,39 . For the iodine atom, the additional  pseudopotential, indicated as pp, was implemented 40 . In some cases, the geometries obtained from the B3LYP/aug-cc-pVTZ method were used for calculations of single-point electronic energies with the coupled-cluster singledouble and perturbative triple, CCSD(T), method 41 . All energies were corrected for zero-point vibrational energy (ZPVE), which was taken from the harmonic vibrational energies calculated at the B3LYP level.</p>