JOURNAL OF CHEMICAL PHYSICS VOLUME 114, NUMBER 17 1 MAY 2001 Three-center versus four-center elimination in photolysis of vinyl fluoride and vinyl bromide at 193 nm: Bimodal rotational distribution of HF and HBr „ v Ï5… detected with time-resolved Fourier transform spectroscopy Shiaw-Ruey Lin, Shih-Che Lin, Yu-Chang Lee, Yung-Ching Chou, I-Chia Chen, and Yuan-Pern Leea) Department of Chemistry, National Tsing Hua University, 101, Sec. 2, Kuang Fu Road, Hsinchu, Taiwan 30013, Republic of China 共Received 25 September 2000; accepted 1 December 2000兲 Following photodissociation of vinyl fluoride (CH2 CHF) and vinyl bromide (CH2 CHBr) at 193 nm, fully resolved vibration–rotational emission spectra of HF and HBr in spectral regions 3050– 4900 and 2000–2900 cm⫺1 , respectively, are temporally resolved with a step–scan Fourier transform spectrometer. With a data acquisition window 0–5 s suitable for spectra with satisfactory ratio of signal-to-noise, emission from HX 共with X ⫽ F or Br兲 up to v ⫽6 is observed. All vibrational levels show bimodal rotational distributions. For CH2 CHF, these two components of HF have average rotational energies ⬃2 and 23 kJ mol⫺1 and vibrational energies ⬃83 and 78 kJ mol⫺1 , respectively; the values are corrected for small quenching effects. For CH2 CHBr, these two components of HBr correspond to average rotational energies ⬃4 and 40 kJ mol⫺1 , respectively, and similar vibrational energies ⬃68 kJ mol⫺1 . The separate statistical ensemble 共SSE兲 model is suitable for three-center 共␣, ␣兲 elimination of HX because of the loose transition state and a small exit barrier for this channel; predicted vibrational energy distributions of HX are consistent with those observed for the high-J component. An impulse model taking into account geometries and displacement vectors of transition states during bond breaking predicts substantial rotational excitation for three-center elimination of HX but little rotational excitation for four-center 共␣, 兲 elimination; observed rotational energies of low-J and high-J components are consistent with those predicted for four-center and three-center elimination channels, respectively. The model also explains why observed rotational energy of HF produced via three-center elimination of CH2 CHF is smaller than that of HCl from CH2 CHCl. Ratios of rate coefficients 共0.66:0.34 and 0.88:0.12兲 predicted for three-center or four-center elimination channels based on Rice–Ramsberger–Kassel– Marcus theory are consistent with estimated branching ratios ⬃0.75:⬃0.25 and ⬃0.81:0.19 determined based on counting vibrational distribution of HF and HBr, respectively, to v ⭐5 for high-J and low-J components and considering possible quenching effects within 5 s. Hence we conclude that, similar to photolysis of CH2 CHCl, observed high-J and low-J components correspond to HX ( v ,J) produced from three-center and four-center elimination channels, respectively. The results are compared with those from photolysis of vinyl chloride at 193 nm. © 2001 American Institute of Physics. 关DOI: 10.1063/1.1343079兴 I. INTRODUCTION ceed on the ground electronic surface; these include elimination of H, H2 , HCl, and Cl 共translationally cold兲. Two secondary channels eliminating H after elimination of Cl, and Cl after elimination of H from CH2 CHCl are also identified. Recently we employed a step–scan Fourier transform spectrometer to record fully resolved vibration–rotational emission spectra of HCl during photolysis of CH2 CHCl at 193 nm.2 All vibrational levels 共up to v ⫽6兲 of HCl show bimodal rotational distributions with low-J components corresponding to HCl ( v , J兲 produced from four-center 共␣, 兲 elimination and high-J components corresponding to HCl from three-center 共␣, ␣兲 elimination, respectively. The branching ratio of 0.84:0.16 determined for three-center or four-center elimination is consistent with rate coefficients for unimolecular decomposition predicted for these two channels based on RRKM 共Rice–Ramsberger–Kassel–Marcus兲 theory. Trobridge and Jennings3 performed Hg photosensitized Although photolysis of vinyl halides (CH2 CHX, X⫽F, Cl, or Br兲 was investigated by numerous researchers, a detailed mechanism of its dissociation is still uncertain partly because its dissociation proceeds via multiple channels. Among these halides, vinyl chloride (CH2 CHCl兲 was studied most extensively. The most detailed investigation is reported by Blank et al. 1 who employed photofragment translational spectroscopy 共PTS兲 using VUV synchrotron radiation to ionize products and observed five primary dissociation channels following excitation of CH2 CHCl at 193 nm. Most Cl atoms are translationally hot; they originate from dissociation via an electronically excited state. The remaining channels proa兲 Author to whom correspondence should be addressed. Also at the Institute of Atomic and Molecular Sciences, Academia Sinica, Taipei, Taiwan. Electronic mail: [email protected] 0021-9606/2001/114(17)/7396/11/$18.00 7396 © 2001 American Institute of Physics Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 decomposition of CH2 CHF and reported that HF and C2 H2 are the sole products. Kirk and Tschuikow-Roux4 identified reaction products C2 H2 , C2 HF, and 1,1-C2 H2 F2 from photolysis of CH2 CHF at 147 nm. Based on the pressure dependence of the relative yield of 1,1-C2 H2 F2 with respect to C2 H2 , they proposed that secondary reactions of F atoms with excited C2 H2 F take place. Berry and Pimentel5 observed laser emission of HF and HCl following UV photolysis of CH2 CHF and CH2 CHCl. Further studies by Sirkin and Pimentel6 resulted in observation of 33 laser transitions of HF ranging from J ⬙ ⫽8 – 31 and v ⬙ ⫽0 – 5. They concluded that HF was mainly produced via four-center elimination based on a similarity in the rotational pattern of laser emission resulting from photolysis of CH2 CHF and CH2 CF2 . 7 They also collected and analyzed products of flash photolysis of CH2 CHF 共⬎155 nm兲 with gas chromatography.8 Primary branching ratios of 0.82, 0.13, and 0.05 were determined for HF, F, and H2 elimination channels. Caballero and Wittig9 determined reaction products from infrared multiphoton dissociation 共IRMPD兲 of CH2 CDF with gas chromatography and concluded that the branching ratio for threecenter to four-center elimination is 3:7. Sato et al.10 employed PTS to probe reaction dynamics upon photolysis of CH2 CHF at 157 nm. They reported elimination channels producing HF, H, and H2 and proposed that HF is mainly from four-center elimination because it possesses substantial 共⬃170 kJ mol⫺1 ) translational energy. Three measurements of vibrational distribution of HF upon photolysis of CH2 CHF using various methods are reported. Quick and Wittig11 employed a low-resolution monochromator to resolve HF emission produced upon IRMPD of CH2 CHF and determined relative vibrational population for v ⫽1 – 4 to be 1.00:0.55:0.15:⬍0.05. Watanabe et al.12 carried out Hg sensitized decomposition of CH2 CHF and observed IR emission of HF by a modulation technique to determine population ratios 1.00:0.56:0.42:0.24 for v ⫽1 – 4. Donaldson et al.13 investigated the energy distribution of HF produced from the reaction F⫹C2 H3 with a modified arrested relaxation infrared chemiluminescence technique in which vinyl radicals are prepared from reaction of F with C2 H4 . They reported relative population of HF( v ) for v ⫽3 – 7 as 0.44:0.25:0.17:0.10:0.04; HF emission from reaction of F with C2 H4 interfered with values for v ⫽1 and 2. Previous kinetic studies14–16 yielded an activation energy in the range 280–341 kJ mol⫺1 . Several theoretical calculations10,17,18 predict geometries and energies of transition states of three-center and four-center HF-elimination channels of CH2 CHF; the two channels are predicted to have similar barriers in the range 335–360 kJ mol⫺1 . Kato and Morokuma17 also calculated rate coefficients for unimolecular decomposition by RRKM theory including quantummechanical tunneling effects; they predicted that three-center elimination is favored by a factor ⬃1.3 over four-center elimination. Palma et al.19 investigated the role of H migration in dissociation of CH2 CHF and found a barrier 共⬃293 kJ mol⫺1 ) slightly smaller than that for HF elimination. They also pointed out that, as CHCH2 F is not a true local minimum, formation of CH3 CF is more facile than CHCH2 F with respect to HF elimination via H migration. Photolysis of vinyl fluoride and vinyl bromide 7397 Experimental investigations on dissociation of CH2 CHBr are sparse. Johnson and Price20 photolyzed CH2 CHBr with a Xe flash lamp and reported that HBr formation is the major channel. However, Wodtke et al.21 employed PTS to measure distributions of translational energy and anisotropy parameters of photodissociation products Br and HBr from CH2 CHBr at 193 nm, and reported a branching ratio of 1.28⫾0.05 between these two channels. Photofragment ion imaging was applied by Katayanagi et al.22 in photolysis of CH2 CHBr in a molecular beam to determine production of Br in both spin–orbit ( 2 P 1/2 and 2 P 3/2) states with a branching ratio of 关Br*兴/关Br兴 of 0.06 ⫾ 0.03. Saito et al.23 employed a shock tube to investigate thermal decomposition of CH2 CHBr at 1300–2000 K; they derived a barrier height ⬃ 230 kJ mol⫺1 . This value is much smaller than theoretically predicted barriers of 308 and 340 kJ mol⫺1 for three-center and four-center HBr-elimination channels, respectively.24 Experiments on photolysis of HBr and C2 H2 共Ref. 25兲 and of CH2 CHBr 共Ref. 26兲 in a Kr matrix lead to extensive theoretical investigations on decomposition of CH2 CHBr. 24,27–29 Abrash et al.24 used a classical trajectory method on an analytic global potential-energy surface to predict that, at thermal energies, the only brominated decomposition product is HBr. As excitation energy is increased to 619 kJ mol⫺1 共corresponding to excitation at 193 nm兲, reaction channels with elimination of H2 共48%兲, HBr 共44%兲, Br 共5%兲, and H 共3%兲 occur. Abrash et al.24 also predicted that elimination of H2 or HBr occur almost exclusively via a three-center mechanism. In summary, current experimental results indicate that, upon photodissociation of CH2 CHF, HF is formed via either exclusively four-center elimination or both three-center and four-center channels in a ratio of 3:7, even though theoretical calculations predict a preference for three-center elimination. No rotational energy distribution of HF is reported; three reports on vibrational distribution of HF are inconsistent. No experimental result on the internal energy distribution of HBr and the branching between three-center and four-center HBr-elimination paths of CH2 CHBr is available, but theoretical calculations predict a nearly exclusive three-center elimination channel. We have demonstrated that step–scan time-resolved Fourier transform spectroscopy 共TR-FTS兲 provides much improved resolution and sensitivity over previous IR emission techniques30,31 and reported vibration–rotational emission from HCl (1⭐ v ⭐7, J⭐32) during photolysis of CH2 CHCl at 193 nm.2 Observation of bimodal rotational distributions of HCl in all vibrational states yields enhanced understanding of three-center and four-center HCl elimination channels, as described previously. Here we report our continuing effort to investigate HX elimination channels for CH2 CHF and CH2 CHBr. II. EXPERIMENT The apparatus employed to obtain step–scan timeresolved Fourier transform spectra resembles that described previously,2,30,31 only variation from Ref. 2 is described. A telescope served to mildly focus the photolysis beam from an ArF laser 共193 nm兲 to ⬃10 and 20 mm2 at the reaction center Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7398 Lin et al. J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 FIG. 1. Infrared emission spectra of HF in spectral region 4410–3100 cm⫺1 recorded 0–5 s after photolysis of CH2 CHF 共180 mTorr兲 in Ar 共270 mTorr兲. Spectral resolution is 2.0 cm⫺1 ; 100 laser pulses were averaged at each scan step. Four spectra recorded under similar conditions were averaged. Assignments are shown in stick diagrams. with fluences ⬃100 and 40 mJ cm⫺2 for experiments with CH2 CHF and CH2 CHBr, respectively. Filters passing either 3050–4900 cm⫺1 共Corion, RL-2000F and Spectrogon, SP3056.6, for detection of HF兲 or 2000–2900 cm⫺1 共OCLI, W04212-4, for detection of HBr兲 were placed in the sample compartment of the spectrometer. The detected transient signal was amplified with a gain of (5 – 20)⫻106 V/A 共effective bandwidth 1MHz兲 before being sent to an internal A/D converter 共16 bit, 200 kHz兲 of the spectrometer. Typically 300 time-slices were acquired at 5 s intervals and the signal was averaged for 60–100 laser pulses at each scan step; 2517 or 4498 scan steps were performed to yield a spectrum with resolution 2.0 or 0.4 cm⫺1 in the spectral range for detection of HF and HBr, respectively. The partial pressure of CH2 CHF 共or CH2 CHBr) was kept in a range 180–190 共or 135–190兲 mTorr. Ar 共270–320 mTorr, 570 mTorr in one experiment for CH2 CHF) was added near the entrance photolysis port to suppress formation of brown deposit on the quartz window. CH2 CHF 共Lancaster, ⬎98%兲 and CH2 CHBr 共Merck, ⬎99.5%兲 were used without purification except for degassing; no impurity was detected in IR spectra. III. RESULTS Although we employed an instrumental configuration capable of measurements at 1 s resolution in our previous study of photolysis of CH2 CHCl,2 the signal-to-noise 共S/N兲 ratio achievable in this work with such a configuration was unsatisfactory because emission from HF and HBr are much weaker. Compared with CH2 CHCl, photolysis of CH2 CHF is limited by its small absorption cross section at 193 nm, whereas experiments on CH2 CHBr are limited by the small Einstein coefficients of HBr. Hence satisfactory data acquisition was achieved only with an internal 16-bit A/D converter of the spectrometer with a temporal resolution of 5 s. Temporal evolution of emission of HF or HBr up to 1.5 ms was recorded. In this study, we focus on only the first avail- able acquisition window 共0–5 s兲 to obtain information on a nearly nascent vibration–rotational distribution of HX after photolysis. A. Photolysis of CH2 CHF To improve the S/N ratio, we averaged four spectra recorded under identical conditions. Figure 1 is a partial emission spectrum of HF recorded 0–5 s after photolysis of CH2 CHF 共0.180 Torr兲 and Ar 共0.270 Torr兲 with a resolution of 2.0 cm⫺1 . Partial assignments, based on spectral parameters reported by Sengupta et al.32 and Ram et al.,33 are shown as stick diagrams. The spectrum clearly shows emission from high vibration–rotational levels of HF with J ⬘ up to 17 and v ⬘ up to 6. Each vibration–rotational line in the R-branch was normalized with the instrument response function, integrated, and divided by its respective Einstein coefficient34 to yield relative population P v (J). For partially overlapped lines, deconvolution was applied before integration. Semilogarithmic plots of P v (J)/(2J⫹1) of HF for v ⫽1–5 produced from CH2 CHF are shown in Fig. 2, in which v and J indicate vibrational and rotational levels of the emitting state. Bimodal rotational distributions observed for all vibrational levels are fitted with biexponential functions to yield two rotational temperatures, as listed in Table I. We denote these two components as high-J and low-J components. B. Photolysis of CH2 CHBr For improved S/N ratio, we averaged four spectra recorded under nearly identical conditions. Figure 3 shows a partial emission spectrum of HBr recorded 0–5 s after photolysis of CH2 CHBr with a resolution of 0.4 cm⫺1 . Partial assignments shown in Fig. 3 are based on spectral parameters reported by Coxon and Hajigeorgious.35 The spectrum exhibits emission from HBr with J ⬘ up to 32 and v ⬘ up to 6; R bandheads for v ⭐3 are clearly visible. Each vibration– rotational line in the R-branch was analyzed similarly to Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 Photolysis of vinyl fluoride and vinyl bromide 7399 IV. DISCUSSION A. Effects of quenching in photolysis of CH2 CHCl Our previous investigation on photolysis of CH2 CHCl 共Ref. 2兲 showed that rotational quenching of HCl ( v , J兲 is nonnegligible under our experimental conditions when the data acquisition window was set at 0–5 s, especially for v ⬎4. However, the weak signal in this work prevents us from recording satisfactory data at periods less than 5 s. Nevertheless, we can estimate errors introduced due to quenching by comparison of results obtained from 0–1 s 共nearly collisionless兲 and 0–5 s windows after photolysis of CH2 CHCl at 193 nm. A detailed discussion may be found in the Electronic Physics Auxiliary Publication Service 共EPAPS兲 of Ref. 2.37 In summary, rotational energy of the low-J components are nearly unaffected by quenching during the 0–5 s acquisition period, whereas observed vibrational energy decreases by ⬃4%. Observed rotational energy and vibrational energy of the high-J components decrease by about 20% and 11%, respectively. As a consequence, observed branching ratio for three-center to four-center HCl elimination varies from 81:19 to 74:26 when the acquisition window is increased to 0–5 s. B. HF„ v , J … from photolysis of CH2 CHF at 193 nm FIG. 2. Semilogarithmic plots of relative rotational populations of HF ( v ⫽1 – 5, symbol •兲 averaged 0–5 s after photolysis of CH2 CHF 共180 mTorr兲 in Ar 共270 mTorr兲 at 193 nm. Data reported by Donaldson et al. 共Ref. 13; symbol ⌬, for v ⫽3 – 6) are also shown. Solid lines represent least-squares fits of low-J and high-J components. yield relative population P v (J); Einstein coefficients reported by Malins and Setser were used.36 Semilogarithmic plots of P v (J)/(2J⫹1) of HBr for v ⫽1 – 5 produced from CH2 CHBr are shown in Fig. 4. Bimodal rotational distributions observed for all vibrational levels are fitted with biexponential functions to yield two rotational temperatures, as listed in Table II. 1. Bimodal rotational distribution According to Fig. 2 and Table I, photolysis of CH2 CHF produces HF in vibrational states v ⭐5 with bimodal rotational distribution, similar to CH2 CHCl. The rotational temperatures of the high-J and low-J components of HF with v ⭐4 are ⬃2500⫾350 K and 150⫾20 K, respectively; the uncertainties only reflect deviations among various vibrational levels. Although Donaldson et al.13 showed stick diagrams for populations of HF( v ,J) with v ⭓3 on reacting F with C2 H3 共with flow rates F CH2CHF⫽2 and F CF4⫽0.5 mol s⫺1 , pressure unspecified兲 using arrested relaxation, rotational distributions were not analyzed. Their results are compared with ours in Fig. 2 共symbol ⌬兲; they are nearly identical to our data for v ⫽ 3 and 4. Our data for v ⫽5 show TABLE I. Experimental conditions, fitted rotational temperature, and total rotational population of HF( v ) after photolysis of CH2CHF at 193 nm. Expt. no P CH2CHF /mTorr P Ar /mTorr t/s /s 1 180 270 0–5 2 190 570 0–5 Low-J component ./mTorrv High-J component v 1 2 3 4 5 1 2 3 4 5 T rot/K 兺 J P v (J) 2800⫾1000 2600⫾700 1900⫾800 2200⫾1400 1000⫾800 2900⫾1200 2600⫾1000 2100⫾800 2800⫾1400 1700⫾1400 590 共545兲 545共510兲 390共370兲 205共180兲 60共60兲 520共480兲 410共390兲 310共280兲 200共160兲 45共40兲 b a c E rot/kJ 23.1 共18.4兲 20.1共16.6兲 14.6共12.5兲 14.4共10.8兲 4.4共4.4兲 23.2共18.6兲 20.3共17.0兲 15.6共11.8兲 16.6共11.7兲 5.3共4.2兲 b c T rot/K 兺 J P v (J) a E rot/kJ 160⫾60 100⫾70 140⫾80 130⫾70 100⫾80 150⫾80 150⫾120 160⫾70 180⫾110 100⫾80 315 290 200 105 30 230 240 185 90 35 1.8 1.3 0.9 1.0 0.5 2.1 1.7 1.0 1.1 0.5 P v (J)⫽共relative integrated emittance兲/关共instrumental response factor兲 共Einstein coefficient兲兴. Fitted values; extrapolated populations up to J max⫽28 are included. See text. c Summed values are listed in parentheses; only observed levels are summed. See text. a b Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7400 J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 Lin et al. FIG. 3. Infrared emission spectra of HBr in spectral region 2820–2150 cm⫺1 recorded 0–5 s after photolysis of CH2 CHBr 共190 mTorr兲 in Ar 共320 mTorr兲. Spectral resolution is 0.4 cm⫺1 ; 100 laser pulses were averaged at each scan step. Four spectra recorded under similar conditions were averaged. Assignments are shown in stick diagrams. significant quenching. Their observation of both low-J and high-J components of HF in their experiments under relaxation-free conditions in a flowing system supports our conclusion that observed low-J components are nascent, rather than from rotational quenching. FIG. 4. Semilogarithmic plots of relative rotational populations of HBr ( v ⫽1 – 5, symbol 兲 averaged 0–5 s after photolysis of CH2 CHBr 共190 mTorr兲 in Ar 共320 mTorr兲 at 193 nm. Solid lines represent least-squares fits of low-J and high-J components. Lines associated with high-J in a state with large v are more difficult to detect because of limited sensitivity. We assume a Boltzman distribution for the high-J component and associate an extrapolated population with unobserved lines up to J max(v) for each vibrational level. J max(v) are 28, 25, 21, 15, and 7 for v ⫽1 – 5, corresponding to a vibration– rotational energy ⬃19 100 cm⫺1 for the highest observed level of HF in v ⫽5. We refer to populations derived from observed levels as ‘‘summed’’ values, and those from observed and extrapolated values as ‘‘fitted’’ values. Fitted and summed populations of the high-J component in each vibrational state of HF are listed in column ⌺ J P v (J) of Table I, with the latter in parentheses. Fitted and summed rotational populations for the low-J component are nearly identical; hence, only fitted values are listed in Table I. Rotational energies of high-J components obtained on summing a product of level energy and normalized population for each rotational level including extrapolated values for J⭐J max are listed in columns E rot of Table I 共referred to as ‘‘fitted’’ values兲; corresponding values calculated on considering only observed vibration–rotational lines are listed parenthetically 共referred to as ‘‘summed’’ values兲. Averaged rotational energies for v ⫽1 – 5 are derived on multiplying E rot( v ) in Table I by its corresponding population; values for the high-J component of HF are 19⫾1 and 15⫾1 kJ mol⫺1 for fitted and summed values, respectively; the error limits represent only deviations between two experiments. Assuming that quenching effects are similar to those in our previous experiments on CH2 CHCl, we estimate a nascent rotational energy of 23⫾5 kJ mol⫺1 for the high-J component of HF; the uncertainty covers the observed value before correction. The average rotational energy of the low-J component is 1.4 Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 Photolysis of vinyl fluoride and vinyl bromide 7401 TABLE II. Comparison of relative vibrational populations of high-J and low-J components of HF and HBr from photolysis of CH2CHF and CH2CHBr, respectively, at 193 nm with statistical calculations for three-center elimination. Species HF HBr Component Expt. no. v ⫽0 a high-J 1–2 0.40⫾0.06 low-J high-J PST 共three-center兲 SSE 共three-center兲 1–2 3–4 0.25⫾0.10 0.37⫾0.06 low-J PST 共three-center兲 SSE 共three-center兲 3–4 0.35⫾0.10 v ⫽1 b 0.340⫾0.010 共0.341⫾0.014兲c 0.470 0.418 0.318⫾0.021b 0.309⫾0.006b 共0.297⫾0.011兲c 0.361 0.326 0.324⫾0.038b v ⫽2 v ⫽3 v ⫽4 v ⫽5 0.291⫾0.013 共0.297⫾0.009兲 0.262 0.257 0.306⫾0.001 0.274⫾0.003 共0.286⫾0.005兲 0.247 0.238 0.224⫾0.012 0.214⫾0.005 共0.215⫾0.007兲 0.140 0.153 0.225⫾0.012 0.226⫾0.004 共0.225⫾0.005兲 0.166 0.171 0.231⫾0.044 0.124⫾0.010 共0.114⫾0.007兲 0.071 0.087 0.113⫾0.004 0.121⫾0.002 共0.119⫾0.005兲 0.110 0.122 0.159⫾0.021 0.032⫾0.002 共0.033⫾0.005兲 0.034 0.048 0.040⫾0.006 0.071⫾0.003 共0.075⫾0.003兲 0.071 0.085 0.063⫾0.004 a Estimated value; see text. Derived from fitted values listed in Table I; uncertainties represent only deviations between two experiments. c Derived from summed values listed in Table I and listed in parentheses; uncertainties represent only deviations between two experiments. b ⫾0.2kJ mol⫺1 . Considering errors propagated from fitting the high-J components, we estimate that the rotational energy of the low-J component is 1–4 kJ mol⫺1 . 2. Vibrational distribution of HF Values of ⌺ J P v (J) associated with each vibrational state were normalized to yield a relative vibrational population 共for both ‘‘summed’’ and ‘‘fitted’’ values兲, as listed in Table II. Distributions derived from fitted values are used for discussion, unless noted. The vibrational distribution of the high-J component is compared with those of previous reports and statistical predictions in Fig. 5A. Our observed distribution agrees well with those reported by Watanabe et al.12 共symbol 䊊, for v ⭐4) and Donaldson et al.13 共symbol ⵜ, for v ⭓3) except for v ⫽5 in which quenching is significant in our experiments. A vibrational distribution reported by Quick and Wittig11 appears to correspond to a much smaller temperature, presumably due to their use of a 100 kHz RC filter and possible vibrational quenching in their system. Based on observed vibrational distribution for v ⫽1 – 3 of the high-J component, we estimate by linear extrapolation the relative population of v ⫽0 of HF to be 0.40⫾0.06 in Fig. 5. Because the population in Fig. 5 was normalized for HF ( v ⫽1–5兲, this value indicates that about 29% 共⫽0.4/1.4兲 of the total population of HF is in its v ⫽0 state. The vibrational population of the low-J component 关shown in Fig. 5共B兲兴 appears to be nearly inverted at v ⫽1. The population of v ⫽0 for the low-J component is estimated by fitting Fig. 5 with a smooth curve; relatively large uncertainties are associated with this estimate, 0.25⫾0.10. Averaged vibrational energies for both components are thus derived to be 70⫾3 kJ mol⫺1 共high-J兲 and 80⫾6 kJ mol⫺1 共low-J兲. Assuming similar quenching effects as in photolysis of CH2 CHCl under our experimental conditions, we estimate Evib to be 78⫾11 共high-J兲 and 83⫾9 kJ mol⫺1 共low-J兲; the uncertainties cover observed values before correction. C. HBr„v, J… from photolysis of CH2 CHBr at 193 nm 1. Bimodal rotational distribution FIG. 5. Comparison of relative vibrational distributions of HF for both high-J and low-J components after photolysis of CH2 CHF 共180 mTorr兲 in Ar 共270 mTorr兲 at 193 nm. 䉱: this work 共from ‘‘fitted population’’兲; ⵜ: Donaldson et al. 共Ref. 13兲; 䊊: Watanabe et al. 共Ref. 12兲; 䊐: Quick and Wittig 共Ref. 11兲; solid lines: SSE calculation; dotted lines: PST calculations. Similar to CH2 CHF and CH2 CHCl, photolysis of CH2 CHBr produces bimodal rotational distributions of HBr in vibrational states v ⭐5 共Fig. 4兲. The rotational temperatures of the high-J and low-J components of HBr with v ⭐3 are ⬃6500⫾900 K and 330⫾50 K 共Table III兲, respectively; the uncertainties only reflect deviations among various vibrational levels. Similarly, the population is extrapolated to J max(v) for each vibrational level. J max(v) are 38, 34, 30, 24, and 18 for v ⫽1 – 5, corresponding to a vibration–rotational energy of ⬃15 600 cm⫺1 for the highest observed level in v ⫽5. Fitted and summed populations of the high-J component in each vibrational state of HBr are listed in column ⌺ J P v (J) of Table III; only fitted values are listed for the low- J com- Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7402 Lin et al. J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 TABLE III. Experimental conditions, fitted rotational temperature and total rotational population of HBr( v ) after photolysis of CH2CHBr at 193 nm. Expt. no P CH2CHBr /mTorr High-J component P Ar /mTorr t s 3 135 300 0–5 4 190 320 0–5 T rot/K 兺 J P v (J) a 6500⫾1400 6900⫾1000 5800⫾1800 4500⫾1600 3400⫾1400 8200⫾1300 5500⫾1200 6400⫾1600 3700⫾1400 3600⫾1200 4340 共3905兲 3745共3575兲 3070共2790兲 1640共1450兲 1020共970兲 3920共3435兲 3570共3490兲 2960共2750兲 1590共1475兲 880共880兲 v 1 2 3 4 5 1 2 3 4 5 b Low-J component. E rot/kJ c 40.1 共33.1兲 35.3共32.8兲 27.6共23.2兲 20.8共15.7兲 11.3共9.1兲 50.0共39.6兲 33.4共31.8兲 30.9共27.5兲 20.0共17.3兲 12.5共12.5兲 b c T rot/K 兺 J P v (J) a E rot/kJ 270⫾180 400⫾150 320⫾170 420⫾130 270⫾160 260⫾140 310⫾160 410⫾120 370⫾130 220⫾140 1785 1045 920 885 290 1470 1210 1410 710 340 4.7 3.3 2.6 3.1 1.9 3.2 2.3 3.4 2.8 1.3 P v (J)⫽共relative integrated emittance兲/关共instrumental response factor兲 共Einstein coefficient兲兴. Fitted values; extrapolated populations up to J max⫽38 are included. See text. c Summed values are listed in parentheses; only observed levels are summed. See text. a b ponent in Table II. Averaged rotational energies for v ⫽1 – 5 for the high-J components of HBr are 33⫾2 and 28⫾2 kJ mol⫺1 for fitted and summed values, respectively. Assuming similar quenching effects as in photolysis of CH2 CHCl, we estimate a rotational energy of 40⫾9 kJ mol⫺1 for the high-J component. The average rotational energy of the low-J component is 3.2⫾0.4 kJ mol⫺1 . Considering possible errors propagated from fitting the high-J component, we report a rotational energy 3 – 6 kJ mol⫺1 for the low-J component. 2. Vibrational distribution of HBr We performed calculations to optimize structures of transition states of three-center 共TS3兲 and four-center 共TS4兲 elimination of HF from CH2 CHF with MP2共Full兲/ 6-31G** and B3LYP/aug-cc-pVTZ density functional theory38,39 using GAUSSIAN 98 programs.40 Geometries of transition states TS3 and TS4 of CH2 CHF predicted with the B3LYP method are shown in Fig. 7; structural parameters predicted with MP2共full兲 are listed parenthetically for comparison. Predicted structures of TS3 and TS4 are similar to previous reports.10,17 Displacement vectors corresponding to each imaginary vibrational wave number are shown in the lower part of Fig. 7; they are similar to those reported previously17 Vibrational distributions of high-J and low-J components are listed in Table II and shown in Fig. 6. To our knowledge, no experimental data on the rotational or vibrational distribution of HBr are reported. Based on observed vibrational distribution for v ⫽1 – 3, we estimate by linear extrapolation the relative population of v ⫽0 of HBr to be 0.37⫾0.06 and 0.35⫾0.10 in Fig. 6 for high-J and low-J components, respectively. The vibrational distribution of the low-J component has larger errors and appears to be non-inverted, unlike for photolysis of CH2 CHF and CH2 CHCl. Averaged vibrational energies thus derived are similar for both components: 61⫾3 kJ mol⫺1 共high-J 兲 and 65⫾5 kJ mol⫺1 共low-J兲. Considering possible quenching effects under our experimental conditions, we estimate E vib to be 68⫾10 共high-J兲 and 68⫾8 kJ mol⫺1 共low-J兲; the uncertainties cover observed values before correction. D. Transition states of CH2 CHF and CH2 CHBr The ultraviolet absorption of vinyl halides CH2 CHX is characterized by an intense band near 190 nm dominated by a *← valence transition. Several nearby repulsive surfaces, Ã 1 A ⬙ ( *), b̃ 3 A ⬙ ( *), and c̃ 3 A⬘( *) in the case of vinyl bromide,27 lead to rapid C – X bond fission either by surface crossing or direct absorption. On the other hand, relaxation to the ground electronic state leads to elimination of H, X, H2 , and HX.1,24 Hence, we only investigate the ground electronic surface for HX elimination channels. FIG. 6. Relative vibrational distributions of HBr for both high-J and low-J components after photolysis of CH2 CHBr 共190 mTorr兲 in Ar 共320 mTorr兲 at 193 nm. 䉱: this work 共from ‘‘fitted population’’兲; solid lines: SSE calculation; dotted lines: PST calculations. Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 Photolysis of vinyl fluoride and vinyl bromide 7403 FIG. 8. Comparison of energies 共in kJ mol⫺1 ) of transition states 共TS3 and TS4兲 and dissociation products relative to CH2 CHX for X⫽F 共italicized兲, Cl 共bold兲, and Br 共underlined兲. For X⫽F and Cl, values using QCISD共T兲/6-311 ⫹G共d,p兲 at MP2共full兲/6-31G** optimized geometries are used with zeropoint energy corrected; for X⫽Br, values are taken from Ref. 24 共MP4兲. FIG. 7. Geometries of transition states for three-center elimination 共TS3兲 and four-center elimination 共TS4兲 of HF from CH2 CHF predicted with the B3LYP/aug-cc-pVTZ method. Parameters predicted with the MP2 共Full兲/631G** method are also listed in parentheses for comparison. Bond lengths are in Å. Displacement vectors corresponding to imaginary wave numbers are shown in the lower part. except that the angle between the motion of H with respect to the H–F bond decreases from ⬃16° to 12° for TS3 in our calculations. Predicted vibrational wave numbers for TS3 and TS4 of CH2 CHF are listed in Table IV. Abrash et al.24 reported geometries and energies of TS3 and TS4 of CH2 CHBr using HF and MP4 method, but we found that TS3 of CH2 CHBr is difficult to characterize accurately with the B3LYP method. Kato and Morokuma17 used singles and doubles configuration interaction 关共S⫹D兲 CI⫹QC兴 with a 6-31G** basis set to predict barriers 334 and 339 kJ mol⫺1 for TS3 and TS4 of CH2 CHF, respectively; the zero-point energies were corrected. Sato et al.10 employed MP2/6-31G** method to predict barriers of 357 and 344 kJ mol⫺1 for three-center and four-center elimination of HF. We performed similar calculations using a QCISD共T兲/6-311⫹G** method with geometry optimized at MP2共full兲/6-31G** and obtained nearly identical barriers 310 kJ mol⫺1 for both channels. Calculations using the B3LYP/aug-cc-pVTZ method yield barriers of 295 and 293 kJ mol⫺1 for three-center and four-center elimination, respectively. We concluded that barrier height for these two channels are similar. TABLE IV. Vibrational wave numbers (cm⫺1) of transition states TS3 and TS4 for CH2CHF predicted with the B3LYP/aug-cc-pVTZ method. TS3 CH2CHF 3216 1281 519 1160i 3131 897 464 2226 854 230 TS4 1661 824 3395 973 702 1807i 3323 947 523 1828 739 500 1710 736 Relative energies and barriers of three-center and fourcenter HX elimination channels for elimination of HX from CH2 CHX 共X⫽F, Cl, and Br兲 are compared in Fig. 8; values predicted with the QCISD共T兲 method are used for X⫽F so as to compare with values reported previously for CH2 CHCl.2,41 Energies for X⫽Br are taken from Ref. 24; transition states were calculated with the MP4 method. Potential energy differences for HX elimination channels of CH2 CHX are similar for X⫽F, Cl, and Br, with variations in energy less than 25 kJ mol⫺1 in all cases. E. Statistical model calculations Similar to CH2 CHCl,2 we performed statistical theories such as phase space theory 共PST兲42,43 and separate statistical ensemble 共SSE兲44 to predict rotational and vibrational distribution of HX products from the three-center elimination channel which is characterized with a loose transition state and a small exit barrier. We employed vibrational wave numbers of vinylidene predicted theoretically by Chang et al.45 and energies 共corrected for zero-point energy兲 of precursor and products predicted from QCISD共T兲 calculations. Vibrational wave numbers of 2000 cm⫺1 for HF and 1300 cm⫺1 for HBr were used in the simulation. These values are taken as half the vibrational wave numbers of HF and HBr. For comparison, predicted imaginary wave numbers are 1977i关MP2共full兲/6-31G**兴 and 1807i 共B3LYP/aug-ccpVTZ兲 for TS4 and 1191i 关MP2共full兲兴 and 1160i 共B3LYP兲 for TS3 of CH2 CHF, and, according to Ref. 24, 1144i 共TS4兲 and 921i 共TS3兲 for CH2 CHBr. The SSE model predicts greater vibrational excitation of products than PST. The vibrational distributions of HF predicted for three-center elimination with both models are shown in Table II and Fig. 5共A兲; they correspond to average vibrational energies 57 共PST兲 and 69 kJ mol⫺1 共SSE兲. The latter value is slightly smaller than experimental observation of 78⫾11 kJ mol⫺1 , whereas predicted rotational energy Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7404 Lin et al. J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 TABLE V. Comparison of average internal energies of high-J and low-J components of HX 共X⫽F, Cl, and Br兲 with statistical and impulse model calculations. Species Energy /kJ mol⫺1 High-J component Low-J component CH2CHF E rot 23⫾5d 共19⫾1兲e 78⫾11d 共70⫾3兲e E vib CH2CHClg E rot E vib CH2CHBr E rot E vib Four-center eliminationb Three-center eliminationa PST SSE Impulsec Impulsec 1–4d 共1.4⫾0.2兲e 83⫾9d 共80⫾6兲e 38 37 14 共24兲f 9.4 57 69 47⫾2h 共37⫾2兲e 74⫾3h 共66⫾3兲e 3–7h 共3.8⫾0.3兲e 81⫾2h 共78⫾2兲e 37 36 52 2.8 55 66 40⫾9d 共33⫾2兲e 68⫾10d 共61⫾3兲e 3–6d 共3.2⫾0.4兲e 68⫾8d 共65⫾5兲e 36 35 60 71 a Available energies are 354 (CH2CHF), 341 (CH2CHCl兲, and 337 (CH2CHBr), respectively. Available energies are 528 (CH2CHF), 515 (CH2CHCl), and 512 (CH2CHBr), respectively. c Assuming that the impulse force is along the displacement vector corresponding to the imaginary mode of the transition state; see text. d Corrected for possible quenching effects; see text. e Data obtained with a 0–5 s detection window are listed parenthetically. f Using displacement vectors in Ref. 17. g From Ref. 2. h Data obtained with a 0–1 s 共near collisionless兲 detection window. b ⬃37 kJ mol⫺1 is greater than experimental observation of 23 ⫾ 5 kJ mol⫺1 . The vibrational distributions of HBr calculated for threecenter elimination with both models using HBr⫽1300 cm⫺1 , shown in Table III and Fig. 6共A兲, correspond to average vibrational energies 60 共PST兲 and 71 kJ mol⫺1 共SSE兲. The latter is close to experimental observation of 68⫾10 kJ mol⫺1 for both components. However, predicted rotational energy ⬃35 kJ mol⫺1 is consistent with experimental value of 40 ⫾ 9 kJ mol⫺1 for the high-J component. Statistical calculations were also performed for fourcenter elimination channel for comparison, even though one expects unsatisfactory results in view of the tight transition state and a large exit barrier for this channel. Rotational energy ⬃50 kJ mol ⫺1 and vibrational energy ⬃102 kJ mol⫺1 for both HF and HBr were derived with the SSE model; predicted vibrational distributions are also shown in Figs. 5共B兲 and 6共B兲. Observed internal energies of HX 共X⫽F, Cl, and Br兲 from both high-J and low-J components are compared with those according to PST and SSE calculations for three-center elimination in Table V. Predicted rotational energies of HX from three-center elimination match better with those observed for the high-J components. For X⫽Cl and Br, observed rotational energies are ⬃5–11 kJ mol⫺1 共12%–23%兲 greater than statistical prediction, whereas for X⫽F observed rotational energy is ⬃14 kJ mol⫺1 smaller. Statistical models fail to explain why rotational energy of HF is much smaller than HCl or HBr from similar paths. For vibrational energies, observed values are ⬃8 kJ mol⫺1 greater than those pre- dicted for X⫽F and Cl, but is nearly identical to statistical prediction for X⫽Br. Rotational energies of low-J components are much smaller than those predicted statistically for either elimination channel. This suggests that, similar to HCl from CH2 CHCl, the low-J component may be associated with a dynamically controlled dissociation process that typically associates with a tight transition state. F. The impulse model Because dissociation occurs with simultaneous breaking of two bonds, regular impulsive model is not applicable for channels involving TS3 and TS4. Hence, we consider motions of the reaction coordinates described by displacement vectors associated with imaginary modes of transition states TS3 and TS4 of CH2 CHF. The direction of the repulsive force is assumed to be parallel to these displacement vectors. Hence displacement vectors shown in Fig. 7 indicate substantially more rotational excitation of HF in three-center elimination than in four-center elimination because in the former case the H atom moves toward the F atom with a larger impact parameter. If we distribute available energy between H and C2 H2 according to classical mechanics and calculate the dynamics after the energized H atom moves toward the X atom along the displacement vector predicted with theory, rotational energies are predicted according to the equation E rot⫽ 关 m Xm C / 共 m H⫹m X兲共 m H⫹m C兲兴 E avail sin2 ␣ , Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 in which E avail is available energy and ␣ is the angle between direction of motion of H and that of the H–X bond. With an available energy of 354 kJ mol⫺1 and ␣ ⫽12.1°, rotational energy of 13.4 kJ mol⫺1 is predicted for three-center elimination; with ␣⫽16° 共as predicted in Ref. 17兲, the energy increases to 24 kJ mol⫺1 . The latter value is similar to the experimental value of 23⫾5 kJ mol⫺1 . If an available energy of 528 kJ mol⫺1 is used, rotational energies 20 and 34 kJ mol⫺1 for HF is predicted for ␣⫽12.1° and 16°, respectively; these values are maximal because all available energy from isomerization of vinylidene is utilized. It should be noted that predicted rotational energy is sensitive to ␣ which might vary appreciably depending on methods of theoretical calculations. For the high-J component, observed rotational energy of HF 共23⫾5 kJ mol⫺1 兲 is much smaller than that of HCl 共47⫾2 kJ mol⫺1 兲 even though the barrier and exothermicity are similar for both reactions. This situation may be rationalized on comparison of displacement vectors of TS3 of CH2 CHF and CH2 CHCl; with ␣⫽12°–16° in the former case, the H atom moves toward F in TS3 of CH2 CHF with an impact parameter smaller than that of the motion of the H atom toward Cl in TS3 of CH2 CHCl with ␣⫽24°.2 In contrast, little rotational excitation is predicted for four-center elimination according to associated displacement vectors in Fig. 7 because the H atom is moving toward F with a small impact parameter. The expectation is consistent with results of calculations of the intrinsic reaction coordinate 共IRC兲 of CH2 CHF by Kato and Morokuma17 for fourcenter elimination in which HF moves away with a substantial decrease in bond length but little rotational motion. In contrast, the IRC shows substantial rotation of HF for threecenter elimination. With a maximal available energy of 528 kJ mol⫺1 a rotational energy of 9.4 kJ mol⫺1 is predicted for this channel, slightly greater than the experimental value of 1–4 kJ mol⫺1 . Similarly, in the case of CH2 CHBr, three-center elimination is expected to produce HBr with substantial rotational excitation whereas four-center elimination produces HBr with little rotational excitation. However, TS3 for CH2 CHBr cannot be characterized successfully with theory; hence the rotational energy of HBr in this channel cannot be predicted. The impulse model using displacement vectors of imaginary frequencies hence describes satisfactorily rotational distributions observed for high-J and low-J components of HX as resulting from three-center and four-center elimination, respectively. It also provides a possible explanation for the reason why observed rotational energy of HF is smaller than that of HCl in three-center elimination of CH2 CHX. As a comparison, the statistical model fails to describe a variation in rotational energies between HF and HCl produced from three-center elimination even though it describes vibrational distributions of HX satisfactorily. In the case of photolysis of CH2 CHCl, because observed translational energy of HCl is greater than that predicted statistically for three-center elimination, a model considering that the exothermicity of isomerization of vinylidene to acetylene may provide further excitation of HX was proposed previously.1,46 If such a ‘‘kick’’ for HX from isomerization Photolysis of vinyl fluoride and vinyl bromide 7405 of vinylidene to acetylene occurs, one expects the effect be greater for X⫽F than for X⫽Br because of differences in bond distances and masses. Our data, showing that observed vibrational energies of HBr for the high-J component are close to statistical prediction whereas those observed for HCl and HF are ⬃8 kJ mol⫺1 greater than prediction, are consistent with such a picture. G. Branching ratio and RRKM rates of dissociation We estimate the rate of dissociation on the ground electronic surface of vinyl halides irradiated at 193 nm with a microcannonical transition state theory. The Whitten– Rabinovitch equations 47 were used to calculate the density of states and number of transition states. Rates of dissociation for HF elimination depend on the accuracy of predicted potential energy barrier and wave numbers of the transition states. With identical energies 309 kJ mol⫺1 for transition states TS3 and TS4, and vibrational wave numbers predicted with B3LYP/aug-cc-pVTZ 共Table V兲, rates of dissociation for three-center and four-center elimination are calculated to be 7.8 and 4.0⫻1011 s⫺1 , respectively. Accordingly, the branching ratio for formation of HF according to three- and four-center processes is estimated to be 0.66:0.34. Taking into account of estimated population at v ⫽0 as described previously, we determine the branching ratio for the high-J and low-J components of HF with 0⭐v ⭐5 to be 0.68⫾0.03:0.32⫾0.03. The actual branching ratio is estimated to be ⬃0.75:⬃0.25 if quenching effects similar to those observed for HCl from CH2 CHCl 共as discussed in Sec. IV A兲 are assumed. The estimated value is consistent with that predicted for three-center and four-center elimination channels with RRKM theory. The branching ratio is expected to vary only slightly if populations of higher vibrational states are extrapolated because the distributions of v ⬎5 for both channels are similar. Previous work on photolysis of CH2 CDF using IRMPD by Caballero and Wittig9 yielded a branching ratio of 0.3:0.7, inconsistent with our results and RRKM calculations. A possibility remains that migration of the H atom plays an important role for the ratio of 关HF兴/关DF兴, as the barrier for this channel is predicted to be ⬃293 kJ mol⫺1 by Palma et al.19 Further experiments on internal energy distributions of HF and DF from photolysis of CH2 CDF and CD2 CHF are needed to understand the role of H migration. Rates of dissociation for three-center and four-center HBr elimination with energies 318 and 284 kJ mol⫺1 共Ref. 24兲, respectively, at the transition state are calculated to be 1.8 and 0.23⫻1012 s⫺1 , respectively. Accordingly, the branching ratio for formation of HBr following three- and four-center processes is estimated to be 0.88:0.12. The branching ratio for the high-J and low-J components of HBr with 0⭐ v ⭐5 is determined to be 0.74⫾0.04:0.23 ⫾0.04. Considering possible errors and vibrational quenching as discussed in Sec. A, the revised branching ratio of ⬃0.81:⬃0.19 is consistent with that predicted for threecenter and four-center elimination channels with RRKM theory. Based on discussions of Secs. IV D–IV G and similarities in internal energy distributions of HF 共HBr兲 to those of Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7406 HCl from photolysis of CH2CHCl, we conclude that observed high-J and low-J components correspond well with HF 共HBr兲 produced via three-center and four-center elimination, respectively. V. CONCLUSION Rotationally resolved emission from HF and HBr up to v ⫽6 is observed after photolysis of vinyl fluoride and vinyl bromide, respectively, at 193 nm. Similar to the case of CH2 CHCl, all vibrational levels show bimodal rotational distributions with low-J and high-J components corresponding to HX ( v , J兲, X⫽F or Br, produced from four-center and three-center elimination channels, respectively. The SSE statistical model predicts satisfactorily vibrational energy distribution of HX from three-center elimination, but does not explain a rotational energy of HF much smaller than HCl or HBr. An impulse model considering geometries and displacement vectors of transition states during bond breaking predicts the rotational distributions of both channels satisfactorily and provides a possible explanation for rotational excitation of HF less than that of HCl and HBr produced from three-center elimination. The branching ratios determined for three-center:four-center elimination are consistent with predicted rate coefficients for RRKM unimolecular decomposition through these two channels. ACKNOWLEDGMENTS We thank the National Science Council of the Republic of China 共Grant Nos. NSC89-2113-M-007-076 and NSC892119-M-007-003兲 for support and the National Center for High-Performance Computing for computer time. 1 Lin et al. J. Chem. Phys., Vol. 114, No. 17, 1 May 2001 D. A. Blank, W. Sun, A. G. Suits, and Y. T. Lee, J. Chem. Phys. 108, 5414 共1998兲. 2 S.-R. Lin, S.-C. Lin, Y.-C. Lee, Y.-C. Chou, I-C. Chen, and Y.-P. Lee, J. Chem. Phys. 114, 160 共2001兲. 3 A. R. Trobridge and K. R. Jennings, Trans. Faraday Soc. 61, 2168 共1968兲. 4 A. W. Kirk and E. T. Roux, J. Chem. Phys. 53, 1924 共1970兲. 5 M. J. Berry and G. C. Pimentel, J. Chem. Phys. 51, 2274 共1969兲. 6 E. R. Sirkin and G. C. Pimentel, J. Chem. Phys. 75, 604 共1981兲. 7 E. R. Sirkin and G. C. Pimentel, J. Chem. Phys. 77, 1314 共1982兲. 8 E. R. Sirkin and G. C. Pimentel, J. Phys. Chem. 88, 1833 共1984兲. 9 J. F. Caballero and C. Wittig, J. Chem. Phys. 82, 1332 共1985兲. 10 K. Sato, S. Tsunashima, T. Takayanagi, G. Fijisawa, and A. Yokoyama, Chem. Phys. Lett. 242, 401 共1995兲. 11 C. R. Quick and C. Wittig, J. Chem. Phys. 72, 1694 共1980兲. 12 H. Watanabe, H. Horiguchi, and S. Tsuchiya, Bull. Chem. Soc. Jpn. 53, 1530 共1980兲. 13 D. J. Donaldson, D. G. Watson, and J. J. Sloan, Chem. Phys. 68, 95 共1982兲. 14 J. M. Simmie, W. J. Quiring, and E. T. Roux, J. Phys. Chem. 74, 992 共1970兲. 15 V. F. Kochubei, A. P. Gavriliv, F. B. Moin, and Y. A. Pazderskii, Kinet. Katal. 20, 1041 共1979兲. 16 P. Cadman and W. J. Engelbrecht, Chem. Comm. 203 共1970兲. 17 S. Kato and K. Morokuma, J. Chem. Phys. 74, 6285 共1981兲. 18 T. Takayanagi and A. Yokoyama, Bull. Chem. Soc. Jpn. 68, 2245 共1995兲. 19 A. Palma, E. Semprini, F. Stefani, and V. D. Martino, Chem. Phys. Lett. 170, 549 共1990兲. 20 J. G. Johnson and D. Price, Dyn. Mass Spectrom. 3, 183 共1973兲. 21 A. C. Wodtke, E. J. Hintsa, J. Somorjai, and Y. T. Lee, Isr. J. Chem. 29, 383 共1989兲. 22 H. Katayanagi, N. Yonekuira, and T. Suzuki, Chem. Phys. 231, 345 共1998兲. 23 K. Saito, T. Yokubo, T. Fuse, H. Tahara, O. Kondo, T. Higashihara, and I. Murakami, Bull. Chem. Soc. Jpn. 52, 3507 共1979兲. 24 S. A. Abrash, R. W. Zehner, G. J. Mains, and L. M. Raff, J. Phys. Chem. 99, 2959 共1995兲. 25 S. A. Abrash, C. M. Carr, M. T. McMahon, and R. W. Zehner, J. Phys. Chem. 98, 11909 共1994兲. 26 D. M. Paolucci, K. Gunkelman, M. T. McMahon, J. McHugh, and S. A. Abrash, J. Phys. Chem. 99, 10506 共1995兲. 27 G. J. Mains, L. M. Raff, and S. A. Abrash, J. Phys. Chem. 99, 3532 共1995兲. 28 P. M. Agrawal, D. C. Sorescu, L. M. Raff, and S. A. Abrash, J. Phys. Chem. 99, 14959 共1995兲. 29 R. D. Kay and L. M. Raff, J. Phys. Chem. A 101, 1007 共1997兲. 30 P. S. Yeh, G. H. Leu, Y.-P. Lee, and I-C. Chen, J. Chem. Phys. 103, 4879 共1995兲. 31 S. R. Lin and Y.-P. Lee, J. Chem. Phys. 111, 9233 共1999兲. 32 U. K. Sengupta, P. K. Das, and K. N. Rao, J. Mol. Spectrosc. 74, 322 共1979兲. 33 R. S. Ram, Z. Morzi, B. Guo, K.-Q. Zhang, P. F. Bernath, J. V. Auwera, J. W. C. Johns, and S. P. Davis, Astrophys. J., Suppl. Ser. 103, 247 共1996兲. 34 E. Arunan, D. S. Setser, and J. F. Ogilvie, J. Chem. Phys. 97, 1734 共1992兲. 35 J. A. Coxon and P. G. Hajigeorgious, J. Mol. Spectrosc. 150, 1 共1991兲. 36 R. J. Malins and D. W. Setser, J. Chem. Phys. 73, 5666 共1980兲. 37 See EPAPS Document No. EJCPSA6-114-018101 for a complete listing of data and discussion on quenching effects. This document may be retrieved via the EPAPS homepage 共http://www.aip.org/pubservs/ epaps.html兲 or from ftp.aip.org in the directory epaps/. See the EPAPS homepage for more information. 38 A. D. Becke, J. Chem. Phys. 98, 5648 共1993兲. 39 C. Lee, W. Yang, and R. G. Parr, Phys. Rev. B 37, 785 共1988兲. 40 M. J. Frisch, G. W. Trucks, H. B. Schlegel et al., GAUSSIAN 98, Revision A.1, Gaussian Inc., Pittsburgh, PA, 1998. 41 J.-F. Riehl and K Morokuma, J. Chem. Phys. 100, 8976 共1994兲. 42 P. Pechukas and J. C. Light, J. Chem. Phys. 42, 3281 共1965兲; C. E. Kolts, J. Phys. Chem. 75, 1526 共1971兲. 43 M. Hunter, S. A. Reid, D. C. Robie, and H. Reisler, J. Chem. Phys. 99, 1093 共1993兲. 44 C. Wittig, I. Nadler, H. Reisler, M. Noble, J. Catanzarite, and G. Radhakrishnan, J. Chem. Phys. 83, 5581 共1985兲. 45 N.-y. Chang, M.-y. Shen, and C.-y. Yu, J. Chem. Phys. 106, 3237 共1997兲. 46 Y. Huang, Y. A. Yang, G. X. He, S. Hashimoto, and R. J. Gordon, J. Chem. Phys. 103, 5476 共1995兲. 47 K. A. Holbrook, M. J. Pilling, and S. H. Robertson, Unimolecular Reactions, 2nd ed. 共Chichester, New York, 1996兲. Downloaded 15 Nov 2007 to 140.114.72.112. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp
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