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Pressure-induced dissociation of water molecules in ice VII

  • Scientific Reports 5, Article number: 12551 (2015)
  • doi:10.1038/srep12551
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Abstract

The neutron diffraction pattern of D2O ice was recently measured at pressures up to 52 GPa by Guthrie et al., who proposed an octahedral interstitial model for ice at pressures above 13 GPa to account for the deviation of the observed crystal structure from that of ice VII. In this article, the octahedral interstitial model was re-examined in terms of the interstitial occupancy and X-ray Raman spectroscopy (XRS) spectra. The interstitial occupancy calculated using first-principles molecular dynamics simulations was negligibly small compared to that of the interstitial model. The oxygen K-edge spectra calculated for the interstitial model exhibited two additional low-energy peaks originating from water molecules and hydroxides that are interacting with interstitial protons, respectively, whereas these low-energy peaks were not observed in the experimentally measured spectra. These results suggest that the interstitial model cannot explain the XRS spectra of ice VII at pressures above 13 GPa and that more precise structure measurements and analyses are necessary to reveal the nature of the pressure-induced transition.

Introduction

Water is a simple molecule consisting of two hydrogen atoms and one oxygen atom. However, water exhibits an extremely complex phase diagram that includes more than fifteen phases. Under compression at room temperature, water transforms at 2.2 GPa from ice VI to ice VII, which consists of two interpenetrating sublattices of water molecules forming a bcc oxygen lattice and two random hydrogen-bond networks. As the pressure is increased from 2.2 GPa to 60 GPa, the bcc oxygen lattice remains stable, with reduced lattice constants; however, the hydrogen-bond networks evolve from statically random to dynamically random and eventually to the symmetric state. In this process, ice VII exhibits intricate phenomena originating from the complex proton dynamics, and X-ray diffraction provides very little information about these phenomena.

Although ice VII has been traditionally considered as a single stable phase of water ice, the literature contains several reports on the transition of the structure and properties at approximately 10–20 GPa1. The transition of the electric charge carrier at approximately 10 GPa was observed by impedance spectroscopy2. The maximum dissociation ratio of water molecules irradiated by X-rays was observed3 using X-ray Raman spectroscopy (XRS)4,5. The deviation of the neutron diffraction pattern of deuterated ice at pressures above Pc = 13 GPa from that of the ice VII structure was reported by Guthrie et al.6, who proposed an octahedral interstitial model with substantial deuteron occupancy (~one deuteron/(unit cell)) at the octahedral interstitial voids of the oxygen lattice. Guthrie et al. concluded that some D2O molecules are dissociated at pressures above Pc, and that protonic species begin to localise at the interstitial sites. A new low-frequency Raman band in the metastable region of ice VII has been reported7 to appear at 14 GPa and at 80 K and 10 K but not at 140 K, suggesting8 the existence of a solid-solid critical point (Tc ≈ 100 K, Pc ≈ 14 GPa) as a possible common origin of these anomalies.

Therefore, scrutinising the nature of the transition at Pc, especially the change of the hydrogen position predicted by the octahedral interstitial model6, would be interesting. In this article, the octahedral interstitial model was re-examined in terms of the interstitial occupancy and the XRS spectra. The interstitial occupancy of ice VII was calculated using a first-principles molecular dynamics simulation, and the results were compared to those predicted by the interstitial model. In addition, because some of the water molecules in ice VII should be dissociated to supply protonic species at the octahedral interstitial sites, additional XRS spectral peaks9 should be observed at energies that differ from that of ice VII. Following this idea, the theoretical oxygen K-edge XAS spectrum, which can be directly compared to the XRS spectrum measured in the dipole limit, was calculated for the ice VII model and the octahedral interstitial model; these spectra were subsequently compared with the experimental XRS spectra.

Theoretical and Experimental

First, the occupancy of interstitial hydrogen was evaluated using the trajectories generated by first-principles molecular dynamics simulations. The initial structure was the geometrically optimised ice VII model (Fig. 1(a)) containing 16 water molecules in a cubic unit cell and the experimental lattice constant10,a0, at pressures between 2 GPa and 40 GPa. The molecular dynamics simulations were performed for 100 ps with a time step of 0.1 fs using an NVT ensemble at temperatures of 300 K and 800 K controlled by a Nose-Hoover thermostat11. The occupancy was evaluated for each snapshot by counting the number of protons within the sphere of radius a0/8 at the centre of the octahedral interstitial sites. The first-principles molecular dynamics simulations were performed using the Vienna ab initio simulation package (VASP) code12. Electronic structure calculations were performed with the projector augmented wave potentials13 in the generalised gradient approximation GGA-PW9114. The electron orbitals were represented by plane waves with an energy cutoff of 700 eV and the Gamma k-point.

Figure 1
Figure 1

Unit cell of (a) the ice VII model and (b) the octahedral interstitial model.

Then, the oxygen K-edge XAS spectra were calculated using the 2 × 2 × 2 supercell of the ice VII model (Fig. 1(a)) as well as that of the interstitial model with half of water molecules dissociated into OH at the bcc-site and H+ at the octahedral site (Fig. 1(b)). Both models consist of 16 water molecules in the unit cell and have no total electric dipole moment. The evaluation of the XAS spectra was based on density functional theory as implemented in the WIEN2k code15. The calculations were performed with the GGA-PBE16 exchange-correlation functional, periodic boundary conditions with Brillouin zone integration with 3 × 3 × 3 Monkhorst-Pack k-points, and RmtKmax = 3, where Rmt is the smallest atomic sphere radius and Kmax is the magnitude of the largest K vector in the expansion of the Kohn–Sham equation. These parameters are sufficient for systems with hydrogen atoms. The convergence was tested for selected calculations by increasing the parameters to RmtKmax = 5 and 5 × 5 × 5 Monkhorst-Pack k-points. The XAS spectra were obtained using the Fermi golden rule with transition moments between a core electron and valence and conduction band states17 with the spectrometer broadening S = 1.4 eV and the lifetime broadening of the core excited state GAMMA0 = 0.18 eV18. The electron relaxation and final state interaction between the excited electron and the core hole were modelled by removing one 1s core electron and placing it in the valence band (i.e., a full core-hole approximation).

Finally, XRS spectra of the oxygen K-edge for dense ice were measured at the BL12XU beamline of SPring-8, Japan. X-rays with an energy of 9.887 keV were incident on the target loaded into a Be gasket; the X-rays scattered at an angle of 30° were counted using the backscattering analyser operated at the Si (5 5 5) reflection. Nano-polycrystalline diamonds19 with a culet size of 0.4 mm were used as anvils to obtain a sample with a relatively large volume under high-pressure conditions. The initial diameter of the sample chamber was 0.2 mm. The XRS spectrum was compared with the theoretical XRS spectrum, which is well approximated by the XAS spectrum when the momentum transfer Q is small (Q·r 1) with respect to the radius r of the core wave function. This condition is satisfied in the present measurement where Q = 2.7 Å1 and r = 0.069 Å. XRS is more frequently used in high-pressure experiments for light elements than XAS because XRS uses hard X-rays that can easily penetrate the sample cell.

Results and Discussion

First, the occupancy of the interstitial hydrogen evaluated by the molecular dynamics simulation is shown in Fig. 2. The occupancy of the interstitial proton was less than 10−4 at 300 K and less than 2 × 10−2 even at an elevated temperature of 800 K, implying that no significant water dissociation occurs in the ice in this pressure and temperature range. This result is in contrast to the occupancy of approximately one deuteron/(unit cell) predicted by the interstitial model. Moreover, it was found that the interstitial model is more unstable by 2.0 eV per water molecule in energy compared to the ice VII model.

Figure 2: Interstitial occupancy as a function of pressure evaluated by the first principles molecular dynamics simulation.
Figure 2

Second, to study the effect of water dissociation, the oxygen K-edge XAS spectra averaged over all oxygen atoms (Fig. 3) were calculated using the 2 × 2 × 2 supercell of the normal ice VII model (Fig. 1a) and that of the interstitial model (Fig. 1b). The ice VII model exhibits a typical spectrum of ice VII with the main peak, whereas the interstitial model exhibits two additional low-energy peaks. In order to reveal the origin of these low-energy peaks, the density of states of the interstitial model was calculated and compared with that of the ice VII model (Supplementary Fig. S1). Two unoccupied bands appeared in the band gap, corresponding to the two peaks in the XRS spectrum of the interstitial model. The real-space density of these bands was plotted in Supplementary Fig. S2, from which it is interpreted that the band in the energy range between 0 eV and 4 eV is the unoccupied states due to the interaction between the water molecule and the dissociated proton; the band between 4 eV and 7 eV is the unoccupied states due to the interaction between the OH anion and the dissociated proton.

Figure 3: Oxygen K-edge XRS spectrum of dense ice.
Figure 3

Green circles are the XRS data measured at 53 GPa with energy resolution of 1.4 eV. The error bars are statistical one, i.e., square root of the intensity. Blue solid line and red broken line are the theoretical spectra calculated at 50 GPa for the ice VII model and the octahedral interstitial model, respectively. The main peak of each theoretical spectrum is aligned to the experimental main peak for comparison.

Finally, the oxygen K-edge XRS spectrum (Supplementary Fig. S3) was measured at 53 GPa with energy resolution of 1.4 eV using Double Crystal Monochromator (DCM). The background of the spectrum mostly consists of Compton scattering from the high pressure apparatus and also from the sample itself. It has a maximum around several tens of electron volts in energy loss and a long tail toward the larger energy loss side. The tail was fitted to a function of y = A/(x − B) + C where A = 10000, B = 490 eV and C = 1750 (Supplementary Fig. S3). The experimental spectrum corrected by subtracting the background (Fig. 3) is compared with the theoretical spectra of the ice VII model and the interstitial model. The oxygen K-edge XRS spectra were also collected under various pressures greater than 40 GPa; the features of the resulting spectra were similar to that obtained at 53 GPa. It should be noted that absence of the peaks corresponding to the dissociated species is inconsistent with the interstitial model. The present result is, however, consistent with the report by Fukui et al.3 that the peak due to X-ray-induced water dissociation20, which is expected to appear in the same energy region, was not observed at pressures above 37 GPa.

A distinct pre-edge peak at 534.6 eV, which has been reported for ice VII at 2.2 GPa21 and other lower-pressure phases21,22,23,24,25, was not observed in this measurement, probably due to the insufficient energy resolution of the measurement and the weaker intensity of the peak compared to the low-pressure data. It has been argued24,25 that the pre-edge peak will disappear when hydrogen bonds are symmetrized and ice X is formed. Therefore the XRS spectra of ice VII at pressures from 2 GPa to 50 GPa were calculated with high resolution (0.3 eV) and shown in Supplementary Fig. S4 where the pre-edge is indicated by a solid arrow. The intensity of the pre-edge peak becomes weaker as the pressure increases. At 50 GPa, the pre-edge peak still exists but becomes very weak. With low resolution (1.4 eV), the pre-edge peak was absorbed into the main peak and could not be resolved at all pressures. The oxygen K-edge XRS spectrum with high energy resolution (Supplementary Fig. S3) was also measured at 50 GPa with using a High-Resolution Monochromator in addition to DCM. The statistics of the data was not sufficient to identify the weak pre-edge peak. High resolution XRS measurements with high statistics are demanded to study this pre-edge feature.

In summary, the deviation in the neutron diffraction pattern at pressures above 13 GPa6 from that of ice VII was re-examined. The deviation may indicate a change in the crystal structure of ice VII; however, the octahedral interstitial model proposed by Guthrie et al.6 appears to be inconsistent with the interstitial occupancy obtained by the first-principles molecular dynamics simulation and with the experimental XRS spectra. To identify the structural change observed at pressures above 13 GPa, careful structural analysis based on high-quality neutron diffraction data under high pressures26,27,28 is indispensable.

Additional Information

How to cite this article: Iitaka, T. et al. Pressure-induced dissociation of water molecules in ice VII. Sci. Rep. 5, 12551; doi: 10.1038/srep12551 (2015).

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Acknowledgements

This work was supported by the RIKEN iTHES Project and by KAKENHI (No. 20103001, No. 20103005, No. 24540523 and No. 26106006) from MEXT of Japan and the joint research programme of the Geodynamics Research Center, Ehime University. The computation was performed in the computing facilities at the RICC system and the HOKUSAI-Great Wave system of RIKEN. The XRS measurements were performed with the approval of the National Synchrotron Radiation Research Center, Taiwan (Project No. 2012-3-061) and the Japan Synchrotron Radiation Research Institute (No. 2012B4260).

Author information

Affiliations

  1. Computational Astrophysics Laboratory, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan

    • Toshiaki Iitaka
    •  & Zhi Li
  2. Center for Novel Material Science under Multi-Extreme Conditions, Graduate School of Material Science, University of Hyogo, Kamigori, Hyogo 678-1297, Japan

    • Hiroshi Fukui
  3. School of Materials Science and Engineering, Hefei University of Technology, Hefei, Anhui 230009, China

    • Zhi Li
  4. National Synchrotron Radiation Research Center, Hsinchu 30076, Taiwan

    • Nozomu Hiraoka
  5. Geodynamics Research Center, Ehime University, 2-5 Bunkyo-cho, Matsuyama, Ehime 790-8577, Japan

    • Tetsuo Irifune
  6. Earth-Life Science Institute, Tokyo Institute of Technology, Tokyo 152-8550, Japan

    • Tetsuo Irifune

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Contributions

T. Iiitaka and H.F designed the project. T. Iitaka performed the theoretical analysis and wrote the manuscript. H.F. performed the XRS measurements. Z.L. contributed to the theoretical analysis. N.H. contributed to the XRS measurement. T. Irifune contributed to the use of the nano-polycrystalline diamonds. All the authors discussed the results and commented on the manuscript.

Competing interests

The authors declare no competing financial interests.

Corresponding author

Correspondence to Toshiaki Iitaka.

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