Laboratory Studies of VUV CH4 Photolysis and Reactions of the Resulting Radicals Robin Shannon, Mark Blitz, Mike Pilling, Dwayne Heard, Paul Seakins University of Leeds, UK Background to Leeds • Leeds has long background in Laboratory Reaction Kinetics with applications to: – Combustion – Pyrolysis – Atmospheric Chemistry • Additionally field work on OH and HO2 detection (spectroscopic) and hydrocarbons (chromatography) • Development of large models (MCM) • Theory on pressure dependent reactions • New STFC grant on methane photolysis and benzene formation on Titan Outline 1. Methane Photolysis – Previous work – Possible approaches 2. Reactions of 1CH2 – Rare gas collisions – Reaction vs relaxation 3. Reactions of CH 4. Recent studies with Laval expansion system (Heard) 1. Methane Photolysis Gans et al. PCCP Front cover CH4 Photolysis – Background Product Channels: • CH3 + H • 1CH2 + H2 • 3CH2 + 2H • CH + H + H2 Smith and Nash, Icarus, 2006 CH4 Photolysis – Previous Work • C • Gans et al. PCCP 2011 CH4 Photolysis – Previous Work Summary of Previous Results Reference Gans et al. Gans et al. Park et al. Mordaunt et al. Heck et al. Brownswo Wang et al. rd et al. Lodriguito et al. Method Direct determination of CH2 and CH3 Direct determination of CH2 and CH3 Simultaneous photolysis and detection of H atoms by LIF ToF H atom kinetic energy spectroscopy Photofragmen t imaging Determination of H and molecular products Trajectory calculations Date λ/nm 2011 118.2 2011 121.6 2008 121.6 1993 121.6 1996 121.6 nm H atom 105-115 nm H2 Photolysis and H atom detection (vuvLIF) at Lyman α 1997 121.6 2000 118.2 and 121.6 2009 121.6 CH3 + H 0.26 ±0.04 0.42 ± 0.05 0.31 ± 0.05 0.49 0.66 - 0.29 ± 0.07 0.39 ± 0.03 CH2 (a 1A1) 0.17 ± 0.05 + H2 CH2 (X 3B1) 0.48 ± 0.06 + 2H CH + H + H2 0.09 0.48 ± 0.05 0.69 0 0.22 - 0.59 ± 0.10 0.50 ± 0.06 0.03 ± 0.08 - 0 - - 0.066 ± 0.012 0.10 ± 0.02 0.07 - 0.51 0.11 - 0.068 ± 0.013 0.02 ± 0.01 Total H Total H2 0.55 ± 0.17 0.55 ± 0.05 0.31 ± 0.05 0.69 1.0 ± 0.5 0.51 1.31 ± 0.13 0.26 ± 0.05 0.47 ± 0.11 0.47 ± 0.10 0.65 ± 0.10 0.60 ± 0.10 0.51 ± 0.06 CH4 Photolysis – Possible approaches • Repeat of Gans et al. approach (synchrotron photolysis source?) • Direct detection of CH via laser induced fluorescence • Enhanced end product analysis studies – Excimer lamps (e.g. 126 nm) as strong sources (>50 mW cm-2) – Chemical conversion (3CH2 particularly difficult to detect via optical spectroscopy) – Use of PTR-MS for sensitive end-product analysis, H3O+ + RH → RH+ + H2O (soft ionization) 2. 1CH2 Reactions – Temperature Dependence Importance of 1CH2 reactions Wilson and Atreya, JGR 108, E2 5014, 2003 1CH 2 + rare gas 1CH 2 + RG → 3CH2 + RG Gannon et al. JCP 132 2010 Temperature Dependence of 1CH2 removal by C2H2 5 Blitz et al This work Hayes et al Hack et al A(T/298 K)^n 4.5 3.5 -1 10 k 1/cm molecule s -1 4 3 Gannon et al. JPCA 114 2010 10 3 2.5 2 1.5 1 0.5 0 100 Monitor removal of 1CH2 by LIF 1CH + C H → C H + H 2 2 2 3 3 1CH + C H + M → C H + M 2 2 2 3 4 1CH + C H → 3CH + C H 2 2 2 2 2 2 Monitor calibrated production of H by LIF 200 300 400 500 Temperature/K 600 700 800 Product Temperature Dependence k overall k reaction k relaxation relaxation Temperature H Atom Yields ΓH 1CH 2 + 195 K 250 K 298 K 398 K 498 K C2H2 0.28 ± 0.11 0.53 ± 0.15 0.88 ± 0.09 1.1 ± 0.16 1.1 ± 0.42 C2H4 0.35 ± 0.09 0.51 ± 0.13 0.71 ± 0.08 0.86 ± 0.16 1.08 ± 0.19 • Relaxation increases with decreasing temperature • Opposite of rare gas behaviour • Relaxation will be more important for planetary atmospheres – more focus on 3CH2 chemistry ? PES showing surface crossing Crossing is below entrance channel Gannon et al. Faraday Discussions 147 2010 (Glowacki and Harvey, Bristol) 3. CH Reactions CH Chemistry • Reactivity very high – capable of reacting with N2 • Important intermediate for increasing carbon number CH + CH4 → H + C2H4 • Single channel so useful calibration reaction • More usually several open channels CH + CH3OH → HCHO + CH3 CH + CH3OH → H + CH3CHO 4. Product Studies from Laval Reactor (Blitz, Shannon and Heard) Low temperature kinetics of abstraction Reactions OH + CH3COCH3 → H2O + CH2COCH3 Barrier, so activated process – what is happening at low T? Shannon et al. PCCP 16 2014 Product Formation OH + CH3OH → CH3O + H2O Shannon et al. Nature Chem. 5 2013 5. Summary • CH4 photolysis yields are important • Currently uncertainty on CH4 photochemistry • New experiments to be undertaken as part of STFC project building on expertise in atmospheric and combustion studies • 1CH2 chemistry shows interesting T dependence, not always taken into account in models. More focus on 3CH2? • Acceleration in loss rates at low temperatures associated with chemical reaction. Further experiments in Laval systems in progress Reagent and product time profiles Total fluorescence signal/ arbitrary units 0.030 1CH 2 kr = 374000 78000 s-1 0.025 0.020 H 0.015 0.010 0.005 kd = 351000 19000 s-1 0.000 -5 0 5 10 15 Time / s 20 25 30 Experimental • Generate 1CH2 by pulsed photolysis of ketene • Monitor removal of 1CH2 by LIF 1CH + C H → C H + H 2 2 2 3 3 1CH + C H + M → C H + M 2 2 2 3 4 1CH + C H → 3CH + C H 2 2 2 2 2 2 • Monitor calibrated production of H by LIF Master Equation Calculations MESMER (Master Equation Solver for Multi Energy-well Reactions) •K(E)’s calculated from RRKM theory. W (E) k (E) h ( E ) source term kji ni(E) A+B kRi nj(E) kPj kij •Energy transfer calculated an exponential down model Ed ~150 - 450cm-1 Products (infinite sink) n (E) i E n (E) j E Master Equation Results Experimental Pressure 1.2 1 150 K 200 K H atom yield 0.8 250 K 300 K 0.6 0.4 0.2 0 1 10 100 1000 10000 100000 Pressure/Torr Modelling shows no stabilization below 50 Torr Balance of reaction is relaxation Experimental James Lockhart Rotary Pump Exhaust Line / Needle valve Reaction Cell Probe Laser Pulse 282 nm 0.10 Fluorescence Signal / Arbitrary Units Photodiode Flash Photolysis LIF Detection Rhodamine 6G Dye Laser PMT Nd: YAG Laser 0.08 Gas mixture flows in towards the cell 0.06 Photolysis laser pulse 248 nm 0.04 Gas mixing manifold 0.02 Excimer Laser 0.00 0 1000 2000 Time / s Boxcar Averager 3000 4000 5000 MFC C N2 MFC C2H2 MFC (CH3)3COOH MFC O2 II - OH + MEA (monoethanolamine) 4 5x10 4 kobs / s -1 4x10 4 3x10 4 2x10 4 1x10 0 0.0 OH ? PM 14 2.0x10 14 14 4.0x10 [MEA] / molecule cm 6.0x10 -3 k = (7.59 ± 0.31) 10-11 s-1 cm-3 Gas phase oxidation will compete with aerosol uptake Onel, L; Blitz, M. A; Seakins, P. W J.Phys.Chem.Lett 2012, 3, 853−856 II - Recycling OH with Excess Oxygen 100% OH Yield Fluorescence Signal / Arbitrary Units 1.0 0.8 0.6 0.4 Experimental OH Yield 0.2 OH Decay Zero OH Yield in N2 0.0 0 500 1000 1500 2000 Time / s 2500 3000 3500 MESMER • Master Equation Solver for Multi Energy-well Reactions • MESMER 3.0 Released 24th Feb 2014. Contact Robin Shannon (R.Shannon@leeds.ac.uk) for more information.