1 / 22

Recombination pathways and energy release in H 2 formation on graphitic surfaces

Recombination pathways and energy release in H 2 formation on graphitic surfaces. Liv Hornekær University of Aarhus, Denmark. Interstellar H 2 formation. Dense clouds - Diffuse clouds - PDRs. Efficient recombination from physisorbed states: up to ~20K

topper
Download Presentation

Recombination pathways and energy release in H 2 formation on graphitic surfaces

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Recombination pathways and energy release in H2 formation on graphitic surfaces Liv Hornekær University of Aarhus, Denmark

  2. Interstellar H2 formation Dense clouds - Diffuse clouds - PDRs Efficient recombination from physisorbed states: up to ~20K Above that more tightly bound states are needed Chemisorbed states on graphite (Cazaux & Tielens, Astrophys. J. 604, 222 (2004)) Formation pumping a possible explanation of PDR observations of vibrational state populations (NGC2023, Burton et al., MNRAS 257, 1p (1992))

  3. Binding sites on graphitic surfaces Physisorption Step edges Vacancy Chemisorption Physisorption: Creighan et al, J. Chem. Phys. 124, 114701 (2006) Chemisorption at defects: Sha et al, J. Am. Chem. Soc. 126, 13095 (2004) Güttler et al, Surface Science 570, 218 (2004)

  4. H chemisorbed on HOPG Eva Rauls Sha et al, Surface Science 496, 318 (2002)

  5. H2 formation on graphite dQ = -k0 e- / T Qn EB kB dt n=1 => First order desorption 490 K => 1.4 eV 580 K => 1.6 eV Zecho et al, J. Chem. Phys. 117, 8486 (2002)

  6. STM on graphite 2.46 Å

  7. Hydrogen on graphite –Monomers Zeljko Sljivancanin 155 x 171 Å2, 180 K Vt~ -710mV, It~ -0.16nA

  8. Monomer desorption Flux: 1012 cm-2s-1 STM at ~180 K RT 20% 1030 x 1140 Å2 1030 x 1140 Å2 Experiment: Upper limit: t = 6 min. Theory: Eb= 0.9 eV, n = 1013 s-1 =>t = 130 s

  9. Monomer desorption Flux: 1012 cm-2s-1 STM at ~180 K RT 20% 1030 x 1140 Å2 1030 x 1140 Å2 Flux: 1014 cm-2s-1 STM at ~170 K RT 80% 1030 x 1140 Å2 515 x 570 Å2

  10. 103 x 114 Å2 H-Dimers on graphite Dimer A Dimer B Vt = 884 mV, It = 0.16 nA

  11. Dimers: Theory vs. Experiment Dimer A Dimer B Vt=0.9 V, LDOS=1x10-6 (eV)-1 Å-3 e. f. Vt = 884 mV, It = 0.16 nA

  12. Diffusion Barrier to diffusion for an isolated H atom: 1.14 eV Barrier to desorption for an isolated H atom: 0.9 eV

  13. Dimer formation Eva Rauls

  14. 103 x 114 Å2 H-Dimers on graphite Dimer A Dimer B Vt = 884 mV, It = 0.16 nA

  15. Dimers after Anneal 103 x 114 Å2 80 x 72 Å2 Vt = 884 mV, It = 0.36 nA Vt = 884 mV, It = 0.19 nA

  16. Recombination pathways Hornekaer et al. Phys. Rev. Lett. 96, 156104 (2006)

  17. Measuring the kinetic energy of formed molecules Laser Induced Thermal Desorption (LITD) Alexandrite Laser 4 mJ 100 ns pulse Time of Flight Measurement D Laser QMS D2

  18. Kinetic energy distribution

  19. H on graphitic surfaces under PDR conditions? Tgas ~ 600-1000K => population of the chemisorbed states on graphite Barrier to recombination: 1.4 eV => thermal desorption: 1000 years at 300K Thermal spikes? Localized heating? => Ekin ~ 1.3 eV, Surface + rovibration: 2.1 eV or high coverage of H2 => Eley Rideal

  20. Eley Rideal - Abstraction Chemisorption Sha et al, J. Chem. Phys. 116, 7158 (2002) Zecho et al, Chem. Phys. Lett. 366, 188 (2002)

  21. Outlook PAHs Onions

  22. People involved Laser desorption: Arnd Baurichter Alan Luntz Saoud Baouche Dept. Phys. SDU Thomas Zecho Univ. Bayreuth and MPG Plasma STM group: Wei Xu Roberto Ortero Flemming Besenbacher iNANO and Dept. Phys. and Astron. University of Aarhus Surface Theory: Eva Rauls Bjørk Hammer iNANO and Dept. Phys. and Astron. University of Aarhus Zeljko Sljivancanin EPFL

More Related