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The combination of double-sided laser heating in the diamond anvil cell and detailed chemical analysis of the recovered samples is a promising approach to explore the chemistry of the Earth’s deep interior from the lower mantle to the core. Routine recovery of laser-heated samples coupled with chemical and textural characterization at the submicron scale is the key to expand knowledge of chemical interactions and melting at extreme conditions, particularly in complex systems. Recent technical developments have allowed us to investigate element partitioning and melting relations at pressures approaching the Earth’s inner-core boundary. In this chapter, we review the techniques used for recovering tiny laser-heated samples and analyzing their chemical compositions and quenched textures, while highlighting key experiments that address silicate–metal element partitioning during mantle–core differentiation, silicate melting relations with applications to early magma ocean crystallization and deep mantle melting, and melting relations in iron-alloy systems relevant to the core. The results have drastically expanded our understanding of element redistribution at deep chemical boundaries and the chemical evolution of the deep mantle and the inner core. Finally, we emphasize the need for standardized protocols to obtain consistent, reproducible results and streamlined procedures to promote good practice and increase productivity. A broad collaboration with a systematic approach would further advance the field of high-pressure geochemistry.
The combination of double-sided laser heating in the diamond anvil cell and detailed chemical analysis of the recovered samples is a promising approach to explore the chemistry of the Earth’s deep interior from the lower mantle to the core. Routine recovery of laser-heated samples coupled with chemical and textural characterization at the submicron scale is the key to expand knowledge of chemical interactions and melting at extreme conditions, particularly in complex systems. Recent technical developments have allowed us to investigate element partitioning and melting relations at pressures approaching the Earth’s inner-core boundary. In this chapter, we review the techniques used for recovering tiny laser-heated samples and analyzing their chemical compositions and quenched textures, while highlighting key experiments that address silicate–metal element partitioning during mantle–core differentiation, silicate melting relations with applications to early magma ocean crystallization and deep mantle melting, and melting relations in iron-alloy systems relevant to the core. The results have drastically expanded our understanding of element redistribution at deep chemical boundaries and the chemical evolution of the deep mantle and the inner core. Finally, we emphasize the need for standardized protocols to obtain consistent, reproducible results and streamlined procedures to promote good practice and increase productivity. A broad collaboration with a systematic approach would further advance the field of high-pressure geochemistry.
Recent years have been witness to advances in our understanding of the high-pressure behavior of crystalline and amorphous silica. Experimental developments made possible by new diffraction techniques have generated new findings to megabar pressures (i.e., above 100 GPa). Theoretical advances, including increasingly accurate first-principles methods and interatomic potentials such as those first proposed by Yoshito Matsui and co-workers, have provided predictions and new understanding of experimental data. We review these theoretical developments in the context of recent experimental findings. Our analyses provides a basis for understanding the extensive metastablity of high-pressure crystalline structures, the nature of the short- and intermediate-range order of the high-pressure amorphous material, and both equilibrium and nonequilibrium transformations. Such study also provides insight into the structural basis of anomalous transport properties of the liquid predicted at high pressure.
Introduction
The nature of silica under pressure is a textbook example of the intersection of condensed-matter physics and mineralogy [1]. Silica is of obvious importance in mineralogy, as SiO2 is abundant in the Earth's crust and plays a major role in the deep interior, both as a product of chemical reactions and as an important secondary phase. From the point of view of condensed-matter physics, SiO2 presents an important system for investigating pressure-induced polymorphism, providing examples of first-order reconstructive transitions [2], displacive (soft-mode-driven) transitions [3], pressure-induced amorphization [4, 5], and polymorphism and polyamorphism [4–6]. Silica is also of great technological interest in both its crystalline and glassy forms.
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