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Catalytic effect of ice in ozone depletion - a ...

James Finn
October 20, 2011

Catalytic effect of ice in ozone depletion - a first principles study

Presentation given in 2010 as an internal King's College London postgraduate seminar for the physics department. In this seminar we explore the effect that a charged ice interface can have on the dissociation of CFCs in the atmosphere.

James Finn

October 20, 2011
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  1. Catalytic effect of ice in ozone depletion - a first

    principles study James Finn, King’s College London james.fi[email protected] Sunday, 21 March 2010
  2. ➡ Introduction ➡ What is Ozone Depletion ➡ Current models

    ➡ Tools used ➡ Results ➡ Conclusion ➡ Future work Overview Norway, 2008 Benasque Spain, 2010 Sunday, 21 March 2010
  3. What is Ozone Depletion? NASA Ozone Watch O O O

    O3 Cl- Cl Active Chlorine Ozone Sunday, 21 March 2010
  4. Cl Photodissociation Model Molina, Nobel Prize for Chemistry 1985 Cl

    C Cl O O O Cl OCl O O OCl O Cl O O ħυ Self Propagating Reaction Cl Sunday, 21 March 2010
  5. Cl Photo-Heterogeneous Catalysis Model Cl C Cl O O O

    Cl OCl O O OCl O Cl O O ħυ Self Propagating Reaction Cl Ice Sunday, 21 March 2010
  6. Cl Photo-Heterogeneous Catalysis Model Solomon, Nobel Peace Prize 2007 Cl

    C Cl O O O Cl OCl O O OCl O Cl O O ħυ Self Propagating Reaction Cl Ice Sunday, 21 March 2010
  7. Cosmic Rays Potential correlation between the altitude loss of ozone

    loss and the peak CR ionisation rate sics Reports 487 (2010) 141–167 155 b e in the pre-ozone hole (October 1979 for Antarctica and March 1979 for the Arctic) and March 1998 for the Arctic) versus latitude. (b) Cosmic ray ionization rate and ozone loss ntarctica, was obtained by subtracting the altitude distribution curve of the pre-ozone b Physics Reports 487 (2010) 141–167 Contents lists available at ScienceDirect Physics Reports journal homepage: www.elsevier.com/locate/physrep Cosmic-ray-driven electron-induced reactions of halogenated molecules Physics Reports 487 (2010) 141–167 Contents lists available at ScienceDirect Physics Reports journal homepage: www.elsevier.com/locate/physrep Cosmic-ray-driven electron-induced reactions of halogenated molecules adsorbed on ice surfaces: Implications for atmospheric ozone depletion and global climate change Qing-Bin Lu Department of Physics and Astronomy and Departments of Biology and Chemistry, University of Waterloo, Waterloo, ON, N2L 3G1, Canada Sunday, 21 March 2010
  8. Cosmic Rays Potential correlation between the altitude loss of ozone

    loss and the peak CR ionisation rate sics Reports 487 (2010) 141–167 155 b e in the pre-ozone hole (October 1979 for Antarctica and March 1979 for the Arctic) and March 1998 for the Arctic) versus latitude. (b) Cosmic ray ionization rate and ozone loss ntarctica, was obtained by subtracting the altitude distribution curve of the pre-ozone b Physics Reports 487 (2010) 141–167 Contents lists available at ScienceDirect Physics Reports journal homepage: www.elsevier.com/locate/physrep Cosmic-ray-driven electron-induced reactions of halogenated molecules Physics Reports 487 (2010) 141–167 Contents lists available at ScienceDirect Physics Reports journal homepage: www.elsevier.com/locate/physrep Cosmic-ray-driven electron-induced reactions of halogenated molecules adsorbed on ice surfaces: Implications for atmospheric ozone depletion and global climate change Qing-Bin Lu Department of Physics and Astronomy and Departments of Biology and Chemistry, University of Waterloo, Waterloo, ON, N2L 3G1, Canada Polar Stratospheric Clouds Sunday, 21 March 2010
  9. Cosmic Ray Model e- Ice Ice + e- Ice Cl

    Cl C Cl Cl O O O Cl O O O Cl O Cl O O O Cl Cl Cl C Cl Cl Lu, Sanche, PRL 87 (2001) Sunday, 21 March 2010
  10. e- Ice Ice + e- Ice Cl Cl C Cl

    Cl O O O Cl O O O Cl O Cl O O O Cl Cl Cl C Cl Cl Sunday, 21 March 2010
  11. Self Interaction Correction ! ΔEH = -εEH [m(↑) - m(↓)]

    ΔEXC = -α(EXC [m(↑), m(↓)] - EXC [m(↓), m(↓)]) partial SIC α ε LSDA LSDA 1 1 0.1 0.2 0.0 0.2 Force Pairing M. d’Avezac PRB (2005) Sunday, 21 March 2010
  12. Gas Phase Dissociation Calculation AEA [eV] LSDA 0.80 pSIC[0.0,0.2] 2.15

    pSIC[0.1,0.2] 1.75 Experiment ~2.0 Energy Gain 1.24 eV SIC Parameters: α - 0.0 ε - 0.2 Sunday, 21 March 2010
  13. Ice Surface Dissociation Paper in preparation. In agreement with experiments

    by M. Bertin et al. Far. Disc. 141 (2009) 293 Sunday, 21 March 2010
  14. Dissociation Energy 0.00 eV 1.24 eV 2.15 eV Gas Phase

    Gain < Surface Gain Sunday, 21 March 2010
  15. Halogen binding ➡How does the ice surface deform during the

    dissociative process? Sunday, 21 March 2010
  16. Halogen binding Formation of three surface hydrogen bonds ➡How does

    the ice surface deform during the dissociative process? Sunday, 21 March 2010
  17. Electron localisation Formation of a Cl- radical ➡Does this dissociative

    reaction form a “free radical”? Sunday, 21 March 2010
  18. Conclusion ➡ CR deposition of excess electrons on ice surfaces

    within PSC’s have a correlation with ozone depletion ➡ Anionic ice surfaces catalyses the reaction: ➡ CFC’s are more likely to dissociate on a charged ice surface CCl4 - CCl3 + Cl- Sunday, 21 March 2010
  19. Future Work ➡ In depth study of water dimer (H2O)2

    ➡ Using TD-DFT ➡ FIR Optical spectra using fictitious laser pulse ➡ TD Code: Octopus Octopus http://www.tddft.org Sunday, 21 March 2010
  20. Future Work ➡ In depth study of water molecule with

    NO ➡ Using TD-DFT ➡ FIR Optical spectra using fictitious laser pulse ➡ Roles in atmospheric chemistry ➡ Biologically important ➡ Tough molecule to model Sunday, 21 March 2010
  21. Acknowledgements Michel Bockstedte Erlangen University Uwe Bovensiepen Duisburg-Essen, University Angel

    Rubio ETSF, San Sebastian Somesh Battacharya ICTP, Trieste Sandro Scandolo ICTP, Trieste Carlo Cavazzoni (Cineca, Bologna, IT) U. Ndonmouo (Tolouse, France) V. Diep (Perdue Univ. USA) Francesca Baletto KCL, London octopus Sunday, 21 March 2010