Abstract
Crystallographic preferred orientation (CPO) of post-perovskite (Mg,Fe)SiO3 (pPv) has been believed to be one potential source of the seismic anisotropic layer at the bottom of the lower mantle (D″ layer). However, the natural CPO of pPv remains ambiguous in the D″ layer. Here we have carried out the deformation experiments of pPv-(Mg0.75,Fe0.25)SiO3 using synchrotron radial X-ray diffraction in a membrane-driven laser-heated diamond anvil cell from 135 GPa and 2,500 K to 154 GPa and 3,000 K. Our results show that the intrinsic texture of pPv-(Mg0.75,Fe0.25)SiO3 should be (001) at realistic P–T conditions of the D″ layer, which can produce a shear wave splitting anisotropy of ∼3.7% with VSH>VSV. Considering the combined effect of both pPv and ferropericlase, we suggest that 50% or less of deformation is sufficient to explain the origin of the shear wave anisotropy observed seismically in the D″ layer beneath the circum-Pacific rim.
Similar content being viewed by others
Introduction
Seismological observations have found an anisotropic layer at the bottom of the lower mantle1,2,3, called the D″ layer. The source of shear wave anisotropy in the D″ layer is uncertain, but geophysical models predict large strains along boundaries in the lower mantle. It has been suggested that lower mantle mineral (Mg,Fe)SiO3 post-perovskite (pPv), which is believed to be stable at relevant P–T conditions of the lowermost mantle4,5, may accommodate the large strains by dislocation slip, resulting in crystallographic preferred orientations (CPOs)6,7. The existence of CPO may help explain anisotropic regions in the D″ layer6,7,8, such as those beneath the circum-Pacific rim where a series of seismic studies have shown that shear wave radial anisotropy is 1–3% with horizontally polarized shear waves (VSH) travelling faster than vertically polarized shear waves (VSV)8,9,10,11. Knowledge of the CPO and elasticity of the pPv phase at relevant P–T and compositional conditions of the lowermost mantle is therefore critical for deciphering enigmatic seismic features of the region, which in turn can help our understanding of the geodynamic processes throughout the history of the deep Earth.
The CPO of pPv has been previously investigated both experimentally and theoretically, but many questions remain (Supplementary Table 1). Radial X-ray diffraction (r-XRD) results for Mg0.9Fe0.1SiO3 pPv (pPv10) synthesized from enstatite and deformed to 157 GPa at room temperature show a (100) texture, which is attributed to slip on the (100) and {110} planes6. A subsequent study of MgSiO3 pPv, synthesized from vitreous MgSiO3, over an extended pressure range from 148 to 185 GPa shows (001) textures, which is attributed to slip on (001)[100] and (001)[010]7. It has been suggested that the (100) texture results from transformation of bridgmanite (bgm), while the (001) texture results from stress-induced slip7. These different results raise the question as to whether the experimentally observed textures are a result of the bgm-to-pPv phase transformation, or are stress-induced12,13. Theoretical simulations of MgSiO3 pPv at high pressures and 0 K demonstrate a diversity of possible slip systems, including (010), {110} and (001)14,15,16,17. On the other hand, elastic anisotropy of D″ layer predicted from global models of mantle flow indicates that the most probable slip of MgSiO3 pPv is on the (010) or (001) plane18,19. MgSiO3 pPv is stable only at high pressures (>125 GPa) and high temperatures (>2,000 K) that are challenging for experimental CPO studies. Thus, analogue pPv minerals that are stable at ambient conditions or relatively low P–T conditions, such as CaIrO3, MgGeO3, MnGeO3 and NaNiF3, have been investigated to aid our understanding of the CPO in pPv-structured minerals for interpreting seismic anisotropy of the D″ layer12,13,20,21. However, these analogue minerals may not have the same slip systems and indeed do not show systematic CPO patterns in the pPv structure, and thus may not be suitable for understanding the CPO of MgSiO3 pPv at lowermost mantle conditions.
Besides disagreement among existing studies, there is also a lack of information for CPO development in Fe-bearing pPv at the lowermost mantle conditions. pPv in the D″ layer is expected to contain iron, where both temperature and iron content affect dislocation slip and texture evolution of materials at high pressure22. For example, deformation studies of lower mantle mineral phase ferropericlase (fp) (Mg,Fe)O at high pressures indicate that the slip system dominates at room temperature, whereas {100}<110> becomes equally active at high temperatures23,24,25. Slip on {100}<110> is also more active in (Mg0.1,Fe0.9)O at room temperature, producing a weaker texture compared with MgO, and therefore demonstrating that iron content affects CPO as well25.
Here we have investigated the deformation of Fe-bearing pPv (Mg0.75Fe0.25SiO3; pPv25) using synchrotron r-XRD in a membrane-driven laser-heated diamond anvil cell from 135 GPa and 2,500 K to 154 GPa and 3,000 K. Analysis of the high P–T diffraction images shows dominant (001) textures, suggesting slip on (001)[100] and (001)[010] or on (001)<110>. Geophysical models of subducting slabs predict that Fe-bearing pPv with slip on (001) would produce a shear wave splitting anisotropy of ∼3.7% with VSH>VSV. Our results thus support geodynamic modelling for the mantle flow-induced CPO in pPv that is reflected in seismic observations of the D″ layer beneath the circum-Pacific rim.
Results
Texture of Fe-bearing pPv
Figure 1 demonstrates schematics of synchrotron r-XRD in a laser-heated diamond anvil cell and experimental P–T pathway in two independent runs (seen Methods for details). Analysis of the r-XRD patterns of the temperature-quenched pPv25 synthesized from enstatite (run 1) at 129 GPa and 300 K (right after the phase transformation) show a crystallographic pole density maximum (texture) near {102} in the inverse pole figures (IPFs) with 2.2 multiples of a random distribution (m.r.d.) (m.r.d.=1 indicates random orientation) and weak secondary maxima at (100) and (001) (Fig. 2a). Upon laser heating of pPv25 to 2,500 K for at least 5 min, the secondary maximum at (001) increased to 3.3 m.r.d (Fig. 2b) and the maximum near {102} became weaker and the secondary maximum at (100) disappeared. The pole densities at (001) and near {102} remained mostly unchanged upon further compression from 135 GPa to 150 GPa at a simultaneous high temperature of 2,500 K. Even at 156 GPa and 3,000 K conditions, there was little change in texture. The larger grain size in these samples, as exhibited from the spotty diffraction patterns, may more readily adopt a deformation texture13 with the small increase in differential stress seen in the sample chamber due to thermal expansion during heating. Upon temperature quenching at 156 GPa, the (001) texture became much weaker and the maximum near {102} became dominant again (Supplementary Fig. 1a). Differential stress of the pPv samples at 132 GPa and 2,500 K was relatively low at 0.25 GPa compared with measurements taken at lower temperature6,7, but increased to 1.50 GPa at 150 GPa (Fig. 2c). In run 2, we were unable to completely transform from bgm to pPv, despite 4 h of laser heating at 133 GPa and 2,500 K. Thus, we analysed textures of both bgm25 and pPv25 during continuous compression and laser heating at 2,500 K. At 133 GPa and 2,500 K, bgm25 displayed no significant texture, whereas pPv25 exhibited a {102} texture maximum (Supplementary Fig. 1), in contrast to the (001) texture maximum seen at 135 GPa and 2,500 K in the run 1. These results suggest that the evolution of texture of pPv25 at high pressures may be sensitive to grain size, differential stress from thermal expansion in the sample chamber, temperature and the degree of phase transformation.
Our observation of a pole density maximum near {102} and a secondary maximum at (100) in pPv25 at 129 GPa, 300 K and differential stress 0.25 GPa following conversion to pPv at 2,000 K for 270 min is similar to that observed for (Mg0.9Fe0.1)SiO3 pPv10 at 145 GPa, 300 K and a differential stress of 7.2–8.5 GPa after conversion to pPv at 1,700–2,000 K for 15–20 min (ref. 6). The (001) texture we observed at 150 GPa, 2500 K and differential stress 1.5 GPa is similar to that of MgSiO3 pPv at 148–185 GPa, 300 K and differential stress of 5.3–10.9 GPa after conversion to pPv at 3,500 K for 10 min (ref. 7) (Supplementary Table 1) and to that of analogue MnGeO3 pPv at 63–105 GPa, 2,000 K and differential stress 2.4–7.3 GPa (ref. 12). In contrast to previous results, we see a change in texture from {102} at room temperature to (001) upon laser heating, and interestingly this (001) texture is not quenchable from high temperature. Differences in textural evolution between earlier studies and our study may be explained by the differences in (1) temperature and duration of heating during sample synthesis and subsequent deformation (Supplementary Table 1) and (2) use or lack of a pressure medium. Both of these factors affect grain size and differential stress and may slightly influence slip system activity. Most notably, our results taken at simultaneously high pressure and temperature on pPv25 show a much lower differential stress of 0.25–1.5 GPa that is still sufficient to induce deformation by dislocation slip. The much lower differential stress is likely to be due to the combined effects of in situ high temperature, a lower experimental pressure range and an NaCl pressure medium.
Slip systems of Fe-bearing pPv
We have performed viscoplastic self-consistent (VPSC)26 polycrystal plasticity simulations to estimate probable slip systems responsible for the observed (001) texture in pPv25. Models are based on previously suggested slip systems listed in Supplementary Table 1. A compressive strain was applied in 1% increments up to 20% strain to 2,000 grains represented as ellipsoids inside of an anisotropic homogenous medium. Summary of relative CRSS and slip system activities for VPSC models are listed in Supplementary Table 2, and IPFs showing texture are shown in Supplementary Fig. 2. We suggest that the texture near {102} is a result of the phase transformation to pPv, whereas the (001) texture is a deformation-induced slip. Thus, we assigned grains an initial preferred orientation similar to our observed {102} transformation texture (Supplementary Fig. 2). The best match to experimental deformation texture (Fig. 2b,c) favours slip on the (001) planes along either the [100] and [010] directions or the <110> direction (Fig. 2d and Supplementary Fig. 2). Thus, slip on (001) should be more representative of the deformation behaviour of pPv in the lowermost mantle.
Discussion
Based on recent geodynamic modelling of the lower mantle, subducting slabs probably sink to the lowermost mantle where the bgm phase is expected to transform to a Fe-bearing pPv phase4,5,8. Seismic velocities resulting from slip on (001)[100] and (001)[010] or on (001)<110> alone in a slab descending to the bottom of the mantle were predicted with a three-dimensional geophysical model27, which assumes deformation is accommodated by dislocation slip. Tracers in the model record temperature and strain history as the slab descends. Grain rotations and resulting CPO are calculated from incremental strain recorded by the tracer, relative critical resolved shear stress of slip systems and starting grain orientations. The transformation texture (Fig. 2a) was assigned as the initial texture in the slab. Texture results for one tracer at the bottom of the slab and ∼100 km above the core-mantle boundary (CMB) were combined with single-crystal elastic constants of pPv at 130 GPa and 3,000 K (ref. 28) to calculate P- and S-wave velocities. The path of the tracer and CPO evolution are shown in Fig. 3. Results show that slip on (001)[100] and (001)[010] or on (001)<110> alone produces a fast horizontal polarization direction with 3.7% shear wave radial anisotropy (the inset of Fig. 3, dVs), consistent with seismic observations of VSH>VSV in D″ layer beneath the circum-Pacific rim7,10,11.
Previous investigations of the source of anisotropy in the D″ have shown that the expected texture of bmg in D″ layer does not produce a seismic signature consistent with seismic observations and thus is not expected to contribute significantly to the observed seismic anisotropy in the region27. (Mg,Fe)O fp with high Vs anisotropy of ∼40% and abundance of ∼25% volume in the D″ layer, has been suggested as a source for the observed anisotropy in D″ (ref. 23). Here we also ran the simulation with 75 vol.% pPv and 25 vol.% fp to investigate the effect of (Mg,Fe)O on seismic velocities in D″ and found that the fastest shear wave polarization directions are tilted subparallel to the CMB with a shear wave radial anisotropy of 3.42% with VSH>VSV (Supplementary Fig. 3), which is similar to that of the pPv (Fig. 3). Thus, our results would suggest that pPv is mostly responsible for the seismic signature observed in the D″ with possibly some contribution from (Mg,Fe)O. However, results here do not take into account grain–grain interactions between stronger pPv grains and presumably weaker (Mg,Fe)O grains, as they are deformed together, which has been shown to affect CPO (for example, Kaercher et al.29).
Selected regions of the D″ layer beneath the circum-Pacific rim are denoted in the set of Supplementary Fig. 4, where the shear wave splitting anisotropy of Caribbean (1), North West Pacific (3) and Antarctic ocean (5) are about 1–1.5%, and others (2,4) are about 0.5% from the literature after 2000 (Supplementary Table 2). Shear wave splitting anisotropy values for deformation accommodated entirely by dislocation slip (Fig. 3 and Supplementary Fig. 3) are larger than those of geophysics observations, meaning that not all deformation may be accommodated by dislocation slip in these regions. Thus, we also ran a simulation with only 50% of deformation accommodated by dislocation slip for pPv and pPv+fp (Fig. 4), where the shear wave radial anisotropy reduces to 2.65% and 2.07%, respectively, consistent with previous results30. This suggests that 50% or less of deformation accommodated by slip is enough to explain the source of shear wave anisotropy in the D″ layer beneath the circum-Pacific rim (Supplementary Fig. 4). Future experimental studies on elastic constants and CPO of FeAl-bearing pPv and fp at relevant P–T conditions of the D″ layer are necessary to further confirm the origin of the shear wave splitting in the region.
Methods
High-pressure synchrotron r-XRD experiments
Polycrystalline (Mg0.75,Fe0.25)SiO3 enstatite was used as the starting material for the synthesis of bgm and pPv at high P–T conditions31. A modified symmetric diamond anvil cell (DAC) with two large side openings of 2θ=30° was integrated with a helium-driven membrane unit to apply pressure for in situ r-XRD experiments. A pair of beveled diamond anvils with a culet size of 100–300 μm in diameter was used to pre-indent a Be gasket of 3 mm in diameter with an initial central thickness of ∼100 μm to ∼30 μm-thick. Subsequently, a hole of 120 μm was drilled in the pre-indented area and filled with a cubic boron nitride (cBN) gasket insert. This assemblage was further compressed to 25 GPa, compressing the cBN gasket insert to 25 μm thickness, and a hole of 80 μm was drilled in the cBN. The sample was sandwiched between two 5 μm platelets of NaCl (run 1: for synthesis of pPv25 directly from enstatite) or KCl (run 2: for synthesis of pPv25 from bgm following conversion of bgm from enstatite) for thermal insulation and pressure calibration (the pressure uncertainty is estimated to be about 2–4 GPa based on their well-known P–T–V equation of states32,33) and inserted into the cBN sample chamber. Samples were ∼15 μm thick and 40 μm in diameter.
High P–T r-XRD experiments were conducted at beamline 13-ID-D (GSECARS) of the Advanced Photon Source (APS) at Argonne National Laboratory. The double-sided laser heating system was modified to accommodate in situ collection of r-XRD patterns of bgm and pPv25 at simultaneous high P–T (ref. 34) (Fig. 1). To avoid contamination of the diffraction peaks from Be gasket, an incident X-ray beam with a monochromatic wavelength of 0.3344 Å was focused down to 3 μm in diameter (full-width at half maximum) onto the sample at an angle of 67.5° from the compression axis of the DAC. To ensure the diffraction images were taken only from the heated area of the sample, X-ray-induced fluorescence from the NaCl or KCl layers was used to align the X-ray spot of ∼3 μm with the laser heating spot of ∼15 μm on both sides of the sample. Temperatures of the heated samples were derived from fitting the grey-body thermal radiation to Planck’s radiation function34, where we adjusted the laser power to keep the peak temperatures within ∼50 K on each side. XRD patterns were recorded using a MarCCD detector with an exposure time of 20–30 s. Instrument parameters of the CCD (charge-coupled device) were calibrated with a LaB6 standard.
In run 1, the enstatite sample assemblage was slowly compressed to 132 GPa where it became amorphous and then laser-heated to 2,000 K, to synthesize the pPv phase directly. Upon temperature quenching after laser heating, analysis of the XRD patterns confirmed the occurrence of the pPv25 phase without other unknown diffraction peaks at 129 GPa and 300 K. We intentionally kept the heating temperature at 2,500 K for the synthesis relatively low, to avoid potential strong grain, growth-induced spotty diffraction patterns that can affect the analysis of the textures. The pPv25 sample at 129 GPa and 300 K was then laser heated to 2,500 K and eventually compressed to 150 GPa, while maintaining the high temperature. At 150 GPa, the sample was further heated up to 3,000 K where the pressure increased to 156 GPa. In run 2, enstatite was compressed to 103 GPa at 300 K and then laser-heated to 1,500 K, to synthesize bgm crystals. The sample was further heated to 2,500 K and consequently compressed from 105 GPa to 133 GPa in 3–5 GPa intervals, to simulate the transformation of bgm to pPv and to understand how the bgm to pPv transformation affects the textures of the pPv phase at high P–T (Fig. 1). These experiments confirm the conclusions of dominant (001) slip in pPv (refs 7, 13) and also help explain the relative texture intensity between bmg and pPv at lowermost mantle conditions. Results differ from conclusions of dislocation simulations ref. 35.
Data analysis and viscoplastic simulations
Experimental r-XRD images were initially processed using the Fit2D36 software to mask saturated diffraction spots and produce unrolled diffraction patterns. As the bottom of the tilted DAC blocked some of the diffraction patterns, ∼180° of Debye rings were collected and analysed, which is still sufficient for textural analysis as only 90° is needed. The unrolled patterns were sliced into 36 spectra at every 5° along the azimuthal angle η and integrated for each slice. The spectra were then refined using the Rietveld method as implemented in the MAUD software package37. We followed the same steps as Wenk et al.37 to extract available information. Together with theoretical elastic constants of pPv-MgSiO3 (ref. 28), the moment pole stress model38 was used to calculate elastic lattice strains from sinusoidal variations in peak position. One typical refinement of pPv25 at 150 GPa and 2,500 K in run 1 is shown in Supplementary Fig. 5. Texture is represented in IPFs that were processed in the software BEARTEX39. VPSC polycrystal plasticity simulations were performed to estimate probable slip systems responsible for the development of the experimentally observed textures26 and are discussed in more detail in the Supplementary Information (Supplementary Fig. 2 and Supplementary Table 2).
Data availability
The data sets generated and/or analysed during the current study are available from the corresponding authors.
Additional information
How to cite this article: Wu, X. et al. Seismic anisotropy of the D″ layer induced by (001) deformation of post-perovskite. Nat. Commun. 8, 14669 doi: 10.1038/ncomms14669 (2017).
Publisher’s note: Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
References
McNamara, A. K., van Keken, P. E. & Karato, S. Development of anisotropic structure in the Earth’s lower mantle by solid-state convection. Nature 416, 310–314 (2002).
Garnero, E. J. & McNamara, A. K. Structure and dynamics of Earth’s lower mantle. Science 320, 626–628 (2008).
Ammann, M. W., Brodholt, J. P., Wookey, J. & Dobson, D. P. First principles constraints on diffusion in lower mantle minerals and a weak D″ layer. Nature 465, 462–465 (2010).
Murakami, M., Hirose, K., Kawamura, K., Sata, N. & Ohishi, Y. Post-perovskite phase transition in MgSiO3 . Science 304, 855–858 (2004).
Oganov, A. R. & Ono, S. Theoretical and experimental evidence for a post-perovskite phase of MgSiO3 in the Earth’s D″ layer. Nature 430, 445–448 (2004).
Merkel, S. et al. Deformation of (Mg,Fe)SiO3 post-perovskite and D″ anisotropy. Science 316, 1729–1732 (2007).
Miyagi, L., Kanitpanyacharoen, W., Kaercher, P., Lee, K. K. M. & Wenk, H. R. Slip systems in MgSiO3 postperovskite: Implications for D″ anisotropy. Science 329, 1636–1638 (2010).
Nowacki, A., Wookey, J. & Kendall, J. M. Deformation of the lowermost mantle from seismic anisotropy. Nature 467, 1091–1096 (2010).
Wookey, J. & Kendall, J. M. in Post-Perovskite: The last Mantle Phase Transition (eds Hirose, K. et al.) 171–189 (American Geophysical Union, 2007).
Panning, M. & Romanowicz, B. Inferences on flow at the base of earth's mantle based on seismic anisotropy. Science 303, 351–353 (2004).
Panning, M. & Romanowicz, B. A three-dimensional radially anisotropic model of shear velocity in the whole mantle. Geophys. J. Int. 167, 361–379 (2006).
Hirose, K., Nagaya, Y., Merkel, S. & Ohishi, Y. Deformation of MnGeO3 post-perovskite at lower mantle pressure and temperature. Geophys. Res. Lett. 37, L20302 (2010).
Miyagi, L., Kanitpanyacharoen, W., Stackhouse, S., Militzer, B. & Wenk, H. R. The enigma of post-perovskite anisotropy: deformation versus transformation texture. Phys. Chem. Minerals 38, 665–678 (2011).
Tsuchiya, T., Tsuchiya, J., Umemoto, K. & Wentzcovitch, R. M. Phase transition in MgSiO3 perovskite in the earth’s lower mantle. Earth Planet. Sci. Lett. 224, 241–248 (2004).
Oganov, A. R., Martonak, R., Laio, A., Raiteri, P. & Parrinello, M. Anisotropy of Earth’s D″ layer and stacking faults in the MgSiO3 post-perovskite phase. Nature 438, 1142–1144 (2005).
Metsue, A. & Tsuchiya, T. Shear response of Fe-bearing in MgSiO3 post-perovskite at lower mantle and pressure. Proc. Jpn Acad. Ser. B89, 51–57 (2013).
Goryaeva, A., Carrez, P. & Cordier, P. Modeling defects and plasticity in MgSiO3 postperovskite: Part 2—screw and edge [100] distance locations. Phys. Chem. Miner. 42, 793–803 (2015).
Nowacki, A., Walker, A. M., Wookey, J. & Kendall, J. M. Evaluating post-perovskite as a cause of D″ anisotropy in regions of palaeosubduction. Geophys. J. Int. 192, 1085–1090 (2013).
Ford, H. A. & Long, M. D. A regional test of global models for flow, rheology, and seismic anisotropy at the base of the mantle. Phys. Earth Planet. Interior 245, 71–75 (2015).
Dobson, D. P. et al. Strong inheritance of texture between perovskite and post-perovskite in the D″ layer. Nat. Geosci. 6, 575–578 (2013).
Yoneda, A. et al. Elastic anisotropy of experimental analogues of perovskite and post-perovskite help to interpret D″ diversity. Nat. Commun. 5, 3453 (2014).
Mao, W. L., Meng, Y. & Mao, H. K. Elastic anisotropy of ferromagnesian post-perovskite in Earth’s D″ layer. Phys. Earth Planet. Interiors 180, 203–208 (2010).
Marquardt, H. et al. Elastic shear anisotropy of ferropericlase in Earth’s lower mantle. Science 324, 224–226 (2009).
Stretton, I., Heidelbach, F., Mackwell, S. & Langenhorst, F. Dislocation creep of magnesiowustite (Mg0.80Fe0.2O). Earth Planet. Sci. Lett. 194, 229–240 (2001).
Tommaseo, C. C., Devine, J., Merkel, S., Speziale, S. & Wenk, H. R. Texture development and elastic stresses in magnesiowűstite at high pressure. Phys. Chem. Miner. 33, 84–97 (2006).
Lebensohn, R. A. & Tomé, C. N. A self-consistent anisotropic approach for the simulation of plastic-deformation and texture development of polycrystals-application to zirconium alloys. Acta Metal. Mater. 41, 2611–2624 (1993).
Cottaar, S., Li, M., McNamara, A. K., Romanowicz, B. & Wenk, H. R. Synthetic seismic anisotropy models within a slab impinging on the core-mantle boundary. Geophys. J. Int. 199, 164–177 (2014).
Wentzcovitch, R. M., Tsuchiya, T. & Tsuchiya, J. MgSiO3 post perovskite at D″ conditions. Proc. Natl Acad. Sci. USA 103, 543–546 (2006).
Kaercher, P. et al. Two-phase deformation of lower mantle analogs. Earth Planet. Sci. Lett. 456, 134–145 (2016).
Wenk, H. R., Cottaar, S., Tomé, C. N., McNamara, A. K. & Romanowicz, B. Deformation in the lowermost mantle: From polycrystal plasticity to seismic anisotropy. Earth Planet. Sci. Lett. 306, 33–45 (2011).
Mao, Z. et al. Electronic spin and valence states of Fe in CaIrO3-type silicate post-perovskite in the lowermost mantle. Geophys. Res. Lett. 37, L22304 (2010).
Fei, Y. et al. High-pressure geoscience special feature: toward an internally consistent pressure scale. Proc. Natl Acad. Sci. USA 104, 9182–9186 (2007).
Dewaele, A. et al. High-pressure-high-temperature equation of state of KCl and KBr. Phys. Rev. B 85, 214105 (2012).
Prakapenka, V.B. et al. Advanced flat top laser heating system for high pressure research at GSECARS: application to the melting behavior of germanium. High Pressure Res. 28, 225–235 (2008).
Goryaeva, A. M., Carrez, P. & Cordier, P. Low viscosity and high attenuation in MgSiO3 post-perovskite inferred from atomic-scale calculations. Sci. Rep. 6, 34771 (2016).
Hammersley, A. P., Svensson, S. O., Hanfland, M., Fitch, A. N. & Hausermann, D. Two-dimensional detector software: from real detector to idealised image or two-theta scan. High Pressure Res. 14, 235–248 (1996).
Wenk, H. R. et al. Rietveld texture analysis from synchrotron diffraction images: II. Complex multiphase materials and diamond anvil cell experiments. Powder Diffract. 29, 220–232 (2014).
Matthies, S., Priesmeyer, H. G. & Daymond, M. R. On the diffractive determination of single-crystal elastic constants using polycrystalline samples. J. Appl. Cryst. 34, 585–601 (2001).
Wenk, H. R., Matthies, S., Donovan, J. & Chateigner, D. BEARTEX: a Windows-based program system for quantitative texture analysis. J. Appl. Cryst. 31, 262–269 (1998).
Tateno, S., Hirose, K., Sata, N. & Ohishi, Y. Determination of post-perovskite phase transition boundary up to 4400 K and implications for thermal structure in D″ layer. Earth Planet. Sci. Lett. 277, 130–136 (2009).
Acknowledgements
X.W. acknowledges financial support from the National Science Foundation of China (U1232204 and 41473056). J.F.L. acknowledges financial support from the US National Science Foundation and Center for High Pressure Science and Technology Advanced Research. High-pressure experiments were performed at GeoSoilEnviroCARS of the APS, Argonne National Laboratory. GeoSoilEnviroCARS operations are supported by the National Science Foundation-Earth Sciences (EAR-1128799) and Department of Energy Geosciences (DE-FG02-94ER14466). A.P.S. is supported by DOE-BES, under contract number DE-AC02-06CH11357. H.R.W. is appreciative for support from NSF EAR-1343908, CSEDI 1067513 and CDAC. We thank J.L. for supporting some test experiments in Beijing Synchrotron Radiation Facility, China, and also thank Dr Kirill Zhuravlev for his kindly help in the experiments. We are very grateful to Sanne Cottaar for the three-dimensional geophysical model code, and M.L. and A.M. for tracers used in the code.
Author information
Authors and Affiliations
Contributions
J.F.L. and V.B.P. designed the experiments. J.F.L. and X.W. conceived and designed the research. J.F.L., X.W., Z.M., J.L. and V.B.P. conducted the experiments. X.W. and P.K. analysed the experimental data. P.K. carried out the simulations. X.W., P.K. and J.F.L. wrote the paper. All authors contributed intellectually to the paper.
Corresponding authors
Ethics declarations
Competing interests
The authors declare no competing financial interests.
Supplementary information
Supplementary Information
Supplementary Figures, Supplementary Tables and Supplementary References (PDF 948 kb)
Rights and permissions
This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/
About this article
Cite this article
Wu, X., Lin, JF., Kaercher, P. et al. Seismic anisotropy of the D″ layer induced by (001) deformation of post-perovskite. Nat Commun 8, 14669 (2017). https://doi.org/10.1038/ncomms14669
Received:
Accepted:
Published:
DOI: https://doi.org/10.1038/ncomms14669
This article is cited by
-
Thermal equation of state of phase egg (AlSiO3OH): implications for hydrous phases in the deep earth
Contributions to Mineralogy and Petrology (2021)
-
Elasticity and Anisotropy of the Pyrite-Type FeO2H-FeO2 System in Earth’s Lowermost Mantle
Journal of Earth Science (2019)
-
Prediction of Mechanical Twinning in Magnesium Silicate Post-Perovskite
Scientific Reports (2017)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.