1 / 13

Introduction

Introduction. XAFS 12 in Malmö 24. June 2003. High-pressure EXAFS and XRD investigation of unit cell parameters of SnO. Hubertus Giefers. Physics Department, University of Paderborn, D-33095 Paderborn, Germany. Survey.  SnO under pressure

neil
Download Presentation

Introduction

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. Introduction XAFS 12 in Malmö 24. June 2003 High-pressure EXAFS and XRD investigation of unit cell parameters of SnO Hubertus Giefers Physics Department, University of Paderborn, D-33095 Paderborn, Germany

  2. Survey  SnO under pressure  Energy dispersive X-ray diffraction (EDXRD) of SnO  EXAFS of SnO under high pressure  Combination of EXAFS and EDXRD results for determination of z(Sn)  Conclusion & Acknowledgment

  3. SnO under pressure • only a few high pressure (HP) • studies on SnO in the literature • a tetragonal to orthorhombic phase • transition is controversially discussed • no HP study on the atom position • parameter z(Sn) is reported in the • literature c c a a b b N.R. Serebryanaya et al., Dokl. Akad. Nauk SSSR 187, 307 (1969). D.M. Adams et al., Phys. Rev. B46, 11358 (1992). E.V. Kapitanov, E.N. Yakovlev, Phys. Stat. Sol. A51, 641 (1979).

  4. Energy dispersive X-ray diffraction (EDXRD) of SnO High pressure (HP) EDXRD at beamline F3 at HASYLAB/DESY • EDXRD spectra recorded with lN2 cooled Ge-detector • in this case beam: 0.2×0.2 mm2 • diamond anvil cell • liquid N2 as pressure transmitting medium • Gold powder as pressure marker • sample size Ø 0.4 mm2

  5. Energy dispersive X-ray diffraction (EDXRD) of SnO • strong texture with c-axis parallel to load axis • no obvious phase transition with pressure • but: lines (hkl) with h≠k broaden with pressure • the broadening depends on the pressure • transmitting medium • we attribute this line broadening to • nonhydrostatic conditions in the HP cell • SnO is very sensitive to shear stress

  6. Energy dispersive X-ray diffraction (EDXRD) of SnO Birch equation-of-state for SnO: K0 = 33.5(11) GPa K0‘ = 6.1(5) compared to SnO2 with K0 = 205 GPa K0‘ = 3.1 due to the strong preferred orientation of SnO in the HP cell, the free atomic position parameter z(Sn) could not be determined from the diffraction intensities that is the reason why we performed the EXAFS study

  7. EXAFS of SnO under high pressure • versatile high pressure cell with B4C anvils • anvil flat diameter 2.5 mm • sample diameter 1.3 mm • gasket material Cu • polyethylene as pressure transmitting medium • Ag powder as pressure marker • pressure determination with EXAFS of Ag at Ag-K edge (25.5 keV)

  8. EXAFS of SnO under high pressure EXAFS at beamline X1 at HASYLAB/DESY • Si (311) double monochromator • energy resolution of 14 eV at 29 keV • EXAFS at Sn-K edge (29.2 keV) • beam size of 0.8×0.8 mm2

  9. EXAFS of SnO under high pressure EXAFS of: sample SnO and pressure marker Ag together in the HP cell

  10. EXAFS of SnO under high pressure

  11. EXAFS of SnO under high pressure • the Sn-O distance • decreases only by • about 2 % • compressibility of the • Sn-O bonding is quite • small • the decrease is linear • with pressure • the 2nd cumulant • decreases continuously • with pressure → • contradicts a phase • transition to ortho- • rhombic structure

  12. Combination of EXAFS and EDXRD results of SnO - a and c from EDXRD - RSn-O from EXAFS • z(Sn) increases due to the strong compression of the • c-axis and the small reduction of the Sn-O distance • when the Sn-O-Sn layers come closer with pressure • the repulsion increases and the increase of z(Sn) flattens • in the same way as the decrease of the c-axis

  13. Conclusion & Acknowledgment • SnO shows no obvious tetragonal to orthorhombic phase transiton with lN2 • as pressure transmitting medium under pressure • XRD line broadenings are induced by nonhydrostatic conditions in the HP cell • SnO is very sensitive to shear stresses • the combination of XRD and EXAFS reveals all 3 cell parameters (a, c, z(Sn)) • of SnO under pressure • Thanks to • Felix Porsch • Gerhard Wortmann • Edmund Welter and the EXAFS HASYLAB team

More Related