Core-Mantle Co-Evolution: An Interdisciplinary Approach

"Earth's interior consists of the rocky mantle and metallic core. They are the most remarkable layers in terrestrial planets. However, detailed composition of the lower mantle and core, particularly, the light elements in the core, physical and chemical state of silicate minerals as well as metallic phases in the core-mantle boundary region and material transport between core and mantle through time and space have not been studied in detail. Seismological observations have suggested that strong heterogeneous features exist, as a result of vigorous convective dynamics at the core-mantle boundary region, which seems to be in contrast with geochemical views suggesting the presence of stable regions. These, so called as primordial reservoirs, are supposed tohold the geochemical signature of early Earth's accretion and differentiation at around 4.6 billion years ago. Moreover, the abundance of radioactive elements in the deep Earth that act as the primary heat sources that drive the dynamic behaviors of the deep Earth are greatly uncertain and unexplored. Recent technological advances in seismological observations, experimental knowhow, analytical resolution and computational network has revolutionized our understanding on deep Earth processes. In seismology, dense observational networks in Thailand, Pacific and USArray are simultaneously available, which can access much finer resolution of seismic imaging of heterogeneous structure in the deep Earth. In particular, the origin of anomalous structure in the uppermost outer core could be resolved. Experimental physicists have achieved record pressures of multi megabars that can ideally help to understand even exoplanetary and Super-Earth interiors. The advances in analytical precision and accuracy and application in geochemistry and cosmochemistry has been well documented in examples such as those in Hayabusa returned "dust" samples. The accessibility of supercomputers for simulations on convective processes in metallic core and silicate mantle and material properties finding first principle computations have also revolutionized our understanding of deep planetary interior. Therefore, it is imminent that it is high time for experts from all these communities to come under a single umbrella and work together."--
New insights into interactions between the core and mantle. The Earth’s deep interior is difficult to study directly but recent technological advances have enabled new observations, experiments, analysis, and simulations to better understand deep Earth processes. Core-Mantle Co-Evolution: An Interdisciplinary Approach seeks to address some of the major unsolved issues around the core-mantle interaction and co-evolution. It provides the latest insights into dynamics, structure, and evolution in the core-mantle boundary region. Volume highlights include: Latest technological advances in high pressure experiments and their application to understanding the mineral physical properties and stability of phases in deep Earth Recent progress in observational seismology, geochemical analysis, geoneutrino experiments, and numerical modeling for understanding the heterogeneity of the lower mantle Theoretical investigations on thermal-chemical evolution of Earth’s mantle and core Exploring thermal-chemical-mechanical-electromagnetic interactions in the core-mantle boundary regions The American Geophysical Union promotes discovery in Earth and space science for the benefit of humanity. Its publications disseminate scientific knowledge and provide resources for researchers, students, and professionals.