Abstract:Structural transition in amorphous oxides, including glasses, under extreme compression above megabar pressures (>1 million atmospheric pressure, 100 GPa) results in unique densification paths that differ from those in crystals. Experimentally verifying the atomistic origins of such densifications beyond 100 GPa remains unknown. Progress in inelastic X-ray scattering (IXS) provided insights into the pressure-induced bonding changes in oxide glasses; however, IXS has a signal intensity several orders of magnitu… Show more
“…The detailed analysis of the O K ‐edge IXS features of MgSiO 3 glasses combined with the ab initio MD simulations revealed the densification of the depolymerized silicate magmas at the lowermost mantle. Recent IXS studies on simple oxide crystals and glasses have revealed that overall shifts in the O K ‐edge features, particularly shifts in the edge onset energy serve as structural proxies of the interatomic distances and bulk densities (Lee et al, , ; Yi & Lee, , ). For the MgSiO 3 glasses, Figure a presents the systematic shifts in the edge energy at the center of gravity ( E c ) values of the MgSiO 3 crystals (Yi & Lee, , ), glasses (Lee et al, ), and liquids with increasing density.…”
Section: Resultsmentioning
confidence: 99%
“…The IXS spectra were collected by scanning the X‐ray energy relative to the analyzer energy of 9.9045 keV. Scattered photons were collected at a scattering angle of 25° with a polycapillary post sample collimator, together with a single spherical Si(555) analyzer operating in a backscattering geometry (Chow et al, ; Lee et al, ). The O K ‐edge IXS spectra for MgSiO 3 glasses with varying pressures up to 130 GPa were collected with the step size and the energy loss (incident energy − analyzed energy) range of 0.5 eV and from 530 to 565 eV, respectively.…”
Section: Methodsmentioning
confidence: 99%
“…The presence of partial melts denser than the lower mantle silicate crystals in ULVZ near the bottom of the mantle has mainly been attributed to the potential partitioning of iron in the melts rather than in crystals, accounting for the observed density contrast (Caracas et al, ; Rost et al, ). In addition to such densification through iron enrichment, a dense packing of oxygen atoms, unique to compressed silicate melts above megabar pressures, may account for the presence of melts at the CMB (Lee et al, , ). Probing of bonding environments around oxygen is, therefore, crucial to understanding the nature of densification of silicate melts at the CMB.…”
Section: Introductionmentioning
confidence: 99%
“…Synchrotron inelastic X‐ray scattering (IXS) reveals otherwise hidden information on the direct bonding environments around target low‐z elements at high pressure (e.g., Lee et al, , ; Lin et al, ; Lin et al, ; Sternemann & Wilke, , and references therein) (see Text S1 in the supporting information). Indeed, oxygen K ‐edge IXS has been applied to explore the densification of MgSiO 3 glasses up to ~40 GPa (Lee et al, ).…”
Section: Introductionmentioning
confidence: 99%
“…However, the pressure condition of the earlier study was not sufficient to fully account for the changes in melt properties at CMB (Text S1). While the inefficiency of IXS poses challenges for probing structures above 100 GPa, recent experimental advances in X‐ray optics involving the postcollimation of scattered X‐rays enabled collection of oxygen K ‐edge IXS signals for simple oxides, such as B 2 O 3 and SiO 2 above megabar pressures (Chow et al, ; Lee et al, ; Lee et al, ). These studies offer opportunities to study transitions in oxygen environments in complex glasses.…”
The structural adaptation in MgSiO 3 melts under compression up to 130 GPa is the key to revealing the origins of the pronounced negative buoyancy of the melts at the core-mantle boundary (CMB). A full understanding of the melt densification requires study of the pressure-induced changes in the bonding configuration around oxygen at the CMB, which has proven to be difficult to measure. Here, the experimental breakthrough in O K-edge inelastic X-ray scattering enables collection of the spectra of MgSiO 3 glasses up to~130 GPa, along with ab initio molecular dynamics simulations, revealing the electronic bonding transitions around heavily compressed oxygen. The spectral results indicate the emergence of denser network structures around oxygen, stemming from contractions in the Mg-O and O-O distances associated with flexible topological and short-range rearrangements around Si. The results unveil the electronic structure and thus the nature of densification in dense partial melts at the CMB.Plain Language Summary A thin ultralow velocity zone at the bottom of mantle is characterized by reduced seismic wave velocities and enhanced density, suggesting the possible presence of molten silicates at a depth of~2,850 km (~130 GPa of pressure). How the melts densify near the core-mantle boundary is unclear. Because oxygen occupies the major volume fraction of silicates, the melt densification is dominated by the reorganization of oxygen during compression. However, the oxygen bonding environments in MgSiO 3 melt-a model mantle melt-near the core-mantle boundary are unknown. Here, the inelastic X-ray scattering spectra of MgSiO 3 glasses and liquids up to~130 GPa revealed the electronic bonding transitions around compressed oxygen that are not observed at low pressures and substantially differ from those in the crystalline MgSiO 3 bridgmanite. The spectral results indicate the pressure-induced emergence of denser network structures around oxygen, stemming from gradual contractions in the Mg-O and O-O distances associated with flexible topological and short-range rearrangements around Si. The densification around oxygen near megabar pressures potentially contributes to the gravitational stabilization of the complex partial melts in the deeper part of the mantle toward ultralow velocity zone.
“…The detailed analysis of the O K ‐edge IXS features of MgSiO 3 glasses combined with the ab initio MD simulations revealed the densification of the depolymerized silicate magmas at the lowermost mantle. Recent IXS studies on simple oxide crystals and glasses have revealed that overall shifts in the O K ‐edge features, particularly shifts in the edge onset energy serve as structural proxies of the interatomic distances and bulk densities (Lee et al, , ; Yi & Lee, , ). For the MgSiO 3 glasses, Figure a presents the systematic shifts in the edge energy at the center of gravity ( E c ) values of the MgSiO 3 crystals (Yi & Lee, , ), glasses (Lee et al, ), and liquids with increasing density.…”
Section: Resultsmentioning
confidence: 99%
“…The IXS spectra were collected by scanning the X‐ray energy relative to the analyzer energy of 9.9045 keV. Scattered photons were collected at a scattering angle of 25° with a polycapillary post sample collimator, together with a single spherical Si(555) analyzer operating in a backscattering geometry (Chow et al, ; Lee et al, ). The O K ‐edge IXS spectra for MgSiO 3 glasses with varying pressures up to 130 GPa were collected with the step size and the energy loss (incident energy − analyzed energy) range of 0.5 eV and from 530 to 565 eV, respectively.…”
Section: Methodsmentioning
confidence: 99%
“…The presence of partial melts denser than the lower mantle silicate crystals in ULVZ near the bottom of the mantle has mainly been attributed to the potential partitioning of iron in the melts rather than in crystals, accounting for the observed density contrast (Caracas et al, ; Rost et al, ). In addition to such densification through iron enrichment, a dense packing of oxygen atoms, unique to compressed silicate melts above megabar pressures, may account for the presence of melts at the CMB (Lee et al, , ). Probing of bonding environments around oxygen is, therefore, crucial to understanding the nature of densification of silicate melts at the CMB.…”
Section: Introductionmentioning
confidence: 99%
“…Synchrotron inelastic X‐ray scattering (IXS) reveals otherwise hidden information on the direct bonding environments around target low‐z elements at high pressure (e.g., Lee et al, , ; Lin et al, ; Lin et al, ; Sternemann & Wilke, , and references therein) (see Text S1 in the supporting information). Indeed, oxygen K ‐edge IXS has been applied to explore the densification of MgSiO 3 glasses up to ~40 GPa (Lee et al, ).…”
Section: Introductionmentioning
confidence: 99%
“…However, the pressure condition of the earlier study was not sufficient to fully account for the changes in melt properties at CMB (Text S1). While the inefficiency of IXS poses challenges for probing structures above 100 GPa, recent experimental advances in X‐ray optics involving the postcollimation of scattered X‐rays enabled collection of oxygen K ‐edge IXS signals for simple oxides, such as B 2 O 3 and SiO 2 above megabar pressures (Chow et al, ; Lee et al, ; Lee et al, ). These studies offer opportunities to study transitions in oxygen environments in complex glasses.…”
The structural adaptation in MgSiO 3 melts under compression up to 130 GPa is the key to revealing the origins of the pronounced negative buoyancy of the melts at the core-mantle boundary (CMB). A full understanding of the melt densification requires study of the pressure-induced changes in the bonding configuration around oxygen at the CMB, which has proven to be difficult to measure. Here, the experimental breakthrough in O K-edge inelastic X-ray scattering enables collection of the spectra of MgSiO 3 glasses up to~130 GPa, along with ab initio molecular dynamics simulations, revealing the electronic bonding transitions around heavily compressed oxygen. The spectral results indicate the emergence of denser network structures around oxygen, stemming from contractions in the Mg-O and O-O distances associated with flexible topological and short-range rearrangements around Si. The results unveil the electronic structure and thus the nature of densification in dense partial melts at the CMB.Plain Language Summary A thin ultralow velocity zone at the bottom of mantle is characterized by reduced seismic wave velocities and enhanced density, suggesting the possible presence of molten silicates at a depth of~2,850 km (~130 GPa of pressure). How the melts densify near the core-mantle boundary is unclear. Because oxygen occupies the major volume fraction of silicates, the melt densification is dominated by the reorganization of oxygen during compression. However, the oxygen bonding environments in MgSiO 3 melt-a model mantle melt-near the core-mantle boundary are unknown. Here, the inelastic X-ray scattering spectra of MgSiO 3 glasses and liquids up to~130 GPa revealed the electronic bonding transitions around compressed oxygen that are not observed at low pressures and substantially differ from those in the crystalline MgSiO 3 bridgmanite. The spectral results indicate the pressure-induced emergence of denser network structures around oxygen, stemming from gradual contractions in the Mg-O and O-O distances associated with flexible topological and short-range rearrangements around Si. The densification around oxygen near megabar pressures potentially contributes to the gravitational stabilization of the complex partial melts in the deeper part of the mantle toward ultralow velocity zone.
Complex oxide heterointerfaces contain a rich playground of novel physical properties and functionalities, which give rise to emerging technologies. Among designing and controlling the functional properties of complex oxide film heterostructures, vertically aligned nanostructure (VAN) films using a self‐assembling bottom‐up deposition method presents great promise in terms of structural flexibility and property tunability. Here, the bottom‐up self‐assembly is extended to a new approach using a mixture containing a 2Dlayer‐by‐layer film growth, followed by a 3D VAN film growth. In this work, the two‐phase nanocomposite thin films are based on LaAlO3:LaBO3, grown on a lattice‐mismatched SrTiO3001 (001) single crystal. The 2D‐to‐3D transient structural assembly is primarily controlled by the composition ratio, leading to the coexistence of multiple interfacial properties, 2D electron gas, and magnetic anisotropy. This approach provides multidimensional film heterostructures which enrich the emergent phenomena for multifunctional applications.
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