Abstract:Bridgmanite, the dominant mineral in the Earth’s lower mantle, crystallizes in the perovskite structure and transforms into post-perovskite at conditions relevant for the D layer. This transformation affects the dynamics of the Earth’s lowermost mantle and can explain a range of seismic observations. The thickness over which the two phases coexist, however, can extend over 100 km, casting doubt on the assignment of the observed seismic boundaries. Here, experiments show that the bridgmanite to post-perovskite … Show more
“…Post‐perovskite should be predominant above the CMB including such areas away from the circum‐Pacific high‐velocity regions. Our results do not preclude the bridgmanite/post‐perovskite transition in pyrolite from generating D” reflections; stress‐induced re‐equilibration within the two‐phase region can produce high amplitude seismic reflections, even when the transition region is thick (Langrand et al., 2019). Additionally, development of the lattice‐preferred orientation of post‐perovskite may generate sharp reflectors within a broad two‐phase region (Ammann et al., 2010; Pisconti et al., 2019).…”
Both experiments and theory have shown that a phase transition between bridgmanite (perovskite-type structure) and post-perovskite occurs in the MgSiO 3 end-member under the lowermost mantle conditions (∼120 GPa and
“…Post‐perovskite should be predominant above the CMB including such areas away from the circum‐Pacific high‐velocity regions. Our results do not preclude the bridgmanite/post‐perovskite transition in pyrolite from generating D” reflections; stress‐induced re‐equilibration within the two‐phase region can produce high amplitude seismic reflections, even when the transition region is thick (Langrand et al., 2019). Additionally, development of the lattice‐preferred orientation of post‐perovskite may generate sharp reflectors within a broad two‐phase region (Ammann et al., 2010; Pisconti et al., 2019).…”
Both experiments and theory have shown that a phase transition between bridgmanite (perovskite-type structure) and post-perovskite occurs in the MgSiO 3 end-member under the lowermost mantle conditions (∼120 GPa and
“…However, dynamic compression occurs on a timescale that largely prevents diffusive processes that change bulk alloy concentrations like those used to form steels. Recent studies in other materials have revealed diffusive phase transformations active on timescales as fast as tens of nanoseconds using dynamic compression 43 and can evolve with characteristic times on the order of hundreds of seconds or more using static compression 44 , highlighting a broad range of possible behaviors. In our case, the rapid stabilization of the hcp structure for iron and for Fe-Si 8.5wt% , but not for Fe-Si 16wt% , may imply that in this latter case the formation of hcp phase may require non-Martensitic action like diffusive de-mixing.…”
The extreme pressures achievable with dynamic compression holds great promise for studying planetary interiors. Phase stability of Fe-Si alloys, which are complex to address, is particularly relevant to understanding telluric planetary cores due to the widely varying properties produced by small changes in Si concentration. Here we report the study of phase stability of pure iron and Fe-Si alloys by x-ray diffraction measurements carried out on shocked samples using an x-ray free electron laser (XFEL). Our setup combined with the brilliance of the XFEL allows us to observe the rapid onset of high-pressure solid-solid phase transformation in Fe and Fe-Si8.5wt%; we observe no such evidence in Fe-Si16wt% up to 110 GPa on the nanosecond timescale. Density Functional Theory calculations provide the conceptual framework to rationalize these observations. Taken together our experiments and calculations support recent dynamic compression measurements and shed light on conflicting static compression results. Our work highlights the need to properly consider the differing intrinsic timescales of the static and dynamic experiments when comparing results, and the complementarity of the techniques in assessing phase diagram and transition mechanisms.
“…PETRA III serves a broad user community, covering a very broad range of scientific fields, from physics [1][2][3][4], chemistry [5,6], and biology, to medicine [7,8], materials [9][10][11], geo- [12][13][14][15] and environmental [16,17] science, archaeometry [18], and nanotechnology [19,20]. With this, it makes an important contribution to solving the grand societal challenges, e.g.…”
PETRA III at DESY is one of the brightest synchrotron radiation sources worldwide. It serves a broad international multidisciplinary user community from academia to industry at currently 25 specialised beamlines. With a storage-ring energy of 6 GeV, it provides mainly hard to high-energy X-rays for versatile experiments in a very broad range of scientific fields. It is ideally suited for an upgrade to the ultra-low emittance source PETRA IV, owing to its large circumference of 2304 m. With a targeted storage ring emittance of $$20 \times 5\,\textrm{pm}^{2}\,\textrm{rad}^{2},$$
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PETRA IV will reach spectral brightnesses two to three orders of magnitude higher than today. The unique beam parameters will make PETRA IV the ultimate in situ 3D microscope for biological, chemical, and physical processes helping to address key questions in health, energy, mobility, information technology, and earth and environment.
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