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Review of Electrical Resistivity Measurements and Calculations of Fe and Fe-Alloys Relating to Planetary Cores

MetadataDetails
Publication Date2021-09-10
JournalFrontiers in Earth Science
AuthorsMeryem Berrada, Richard A. Secco
InstitutionsWestern University
Citations25
AnalysisFull AI Review Included

Technical Documentation & Analysis: MPCVD Diamond for Planetary Core Research

Section titled “Technical Documentation & Analysis: MPCVD Diamond for Planetary Core Research”

6CCVD specializes in providing high-quality, custom MPCVD diamond materials essential for extreme high-pressure/high-temperature (HPHT) research, particularly in geophysics and planetary science. The reviewed paper highlights the critical role of diamond-based apparatus (DAC, MAP) in determining the electrical resistivity ($\rho$) and thermal conductivity ($k$) of Fe and Fe-alloys under conditions relevant to planetary cores (Earth, Moon, Mercury, Mars, Ganymede).


  • Core Research Focus: Review of electrical resistivity ($\rho$) measurements and calculations for Fe and Fe-alloys (Ni, Si, S, O, P) under extreme HPHT conditions (up to 365 GPa and 7000 K) relevant to terrestrial and icy planetary cores.
  • Methodological Reliance: Experimental data relies heavily on static HPHT techniques, primarily the Diamond-Anvil Cell (DAC) and Multi-Anvil Press (MAP), which necessitate high-purity, robust diamond components.
  • Key Finding (Earth Core): Average $\rho$ values for pure Fe at Earth’s Core-Mantle Boundary (CMB) and Inner-Core Boundary (ICB) cluster around $1.07 \mu\Omega$m and $0.97 \mu\Omega$m, respectively, though significant discrepancies exist between theoretical and experimental results (e.g., DAC outliers up to $3.7 \mu\Omega$m).
  • Material Sensitivity: The electrical resistivity of Fe-alloys is highly sensitive to light element content (Si, S, O, P), requiring extremely precise control over sample composition and purity to accurately model core thermal evolution and dynamo sustenance.
  • Diamond Necessity: The paper confirms that Single Crystal Diamond (SCD) is indispensable for DAC experiments, enabling the attainment of pressures up to 365 GPa required for Earth’s ICB and future super-Earth exoplanet studies.
  • Experimental Challenges: Discrepancies in reported $\rho$ values are often attributed to experimental artifacts, including sample geometry errors, temperature gradients (especially in laser-heated DAC), and shunting effects, underscoring the need for ultra-high precision materials and assembly.

The following hard data points were extracted from the review, highlighting the extreme conditions SCD and PCD materials must withstand or enable:

ParameterValueUnitContext
Maximum Pressure Achieved365GPaEarth ICB conditions (Theoretical/Calculated)
Maximum Temperature (Laser Heating)Up to 7000KDAC experiments
Sommerfeld Lorenz Number (L0)2.44 $\times$ 10-8W $\cdot$ $\Omega$ $\cdot$ K-2Standard value for Wiedemann-Franz Law (WFL) conversions
Earth CMB Resistivity (Fe, Avg)1.07$\mu\Omega$mAverage reported value (4,000 K, 136 GPa)
Earth ICB Resistivity (Fe, Avg)0.97$\mu\Omega$mAverage reported value (5,000 K, 330 GPa)
Fe-Si/S Alloy Content Range1.8 to 35.5wt%Range of light element content investigated
Lunar CMB Pressure Range4.5 to 7GPaMulti-anvil press conditions
Martian CMB Temperature Range1,770 to 2,106KRelevant for Fe and Fe-alloy measurements

The research relies on advanced HPHT techniques that utilize diamond materials for pressure generation, sample containment, and measurement access:

  1. Diamond-Anvil Cell (DAC) Experiments: Used opposing Single Crystal Diamond (SCD) anvils to generate ultra-high pressures (up to 365 GPa) on small samples ($\sim$10-4 mm3).
  2. High-Temperature Generation: Achieved primarily through laser heating (up to 7000 K) or internal resistive heating, requiring SCD’s high thermal stability and optical transparency.
  3. Multi-Anvil Press (MAP) Experiments: Utilized tungsten carbide (WC) anvils compressing octahedral cells (often MgO) to achieve lower pressures (up to $\sim$24 GPa) but over larger sample volumes.
  4. Electrical Resistivity Measurement: Conducted using the four-wire method (MAP) or the Van der Pauw method (DAC) on sheet or foil samples, necessitating precise electrode patterning and placement.
  5. Insulation and Shunting Mitigation: High-purity insulating materials (e.g., Al2O3) are required in DAC assemblies to prevent electrical shunting between the sample and the metal gasket, a known source of error in HPHT resistivity measurements.
  6. First-Principles Calculations (DFT/DMFT): Theoretical models (Kubo-Greenwood, Bloch-Grüneisen) are used in conjunction with experimental data to extrapolate $\rho$ values from laboratory P/T to relevant planetary core conditions.

The research reviewed underscores the need for highly specialized, high-purity diamond materials to conduct reliable HPHT electrical resistivity measurements. 6CCVD is uniquely positioned to supply the necessary custom MPCVD diamond solutions to replicate and advance this research.

Research Requirement6CCVD Solution & Value PropositionTechnical Specification Match
Ultra-High Pressure AnvilsOptical Grade Single Crystal Diamond (SCD): Essential for DAC experiments requiring pressures up to 365 GPa. Our SCD offers superior purity and mechanical strength compared to natural diamonds, ensuring reliable pressure generation and minimal optical interference for laser heating/XRD.Materials: Single Crystal Diamond (SCD). Polishing: Ra < 1 nm (critical for anvil culet quality).
HPHT Substrates & Heat SinksHigh-Purity Polycrystalline Diamond (PCD) Wafers: Ideal for use as high-thermal-conductivity substrates in MAP or DAC setups, ensuring uniform temperature distribution and minimizing thermal gradients (a major source of error cited in the paper).PCD Dimensions: Plates/wafers up to 125 mm diameter. Thickness: 0.1 $\mu$m to 500 $\mu$m.
Precision Electrode PatterningCustom Metalization Services: Accurate resistivity measurements (four-wire, Van der Pauw) require precise electrode placement. We offer internal metalization capabilities for depositing thin-film electrodes directly onto diamond surfaces or sample foils.Metalization Options: Au, Pt, Pd, Ti, W, Cu (Internal capability).
Conductive Reference MaterialsBoron-Doped Diamond (BDD): Can be utilized as a stable, conductive reference material or as a component in complex electrode assemblies for high-precision electrical measurements under pressure.Materials: Boron-Doped Diamond (BDD).
Custom Geometry & AssemblyPrecision Laser Cutting and Shaping: We provide custom dimensions and shaping of diamond plates and wafers to fit specific DAC culet sizes (e.g., 50-250 $\mu$m diameter) and MAP cell geometries, ensuring optimal sample alignment and minimizing shunting artifacts.Custom Dimensions: Plates/wafers up to 125 mm. Substrates: Up to 10 mm thickness.

6CCVD’s in-house PhD team possesses deep expertise in MPCVD diamond properties under extreme conditions. We can assist researchers in selecting the optimal diamond grade (e.g., high-purity SCD for optical access, or specific PCD grades for thermal management) and designing custom geometries for similar HPHT Electrical Resistivity and Thermal Transport projects, ensuring maximum experimental fidelity and minimizing the parasitic effects noted in the literature.

For custom specifications or material consultation, visit 6ccvd.com or contact our engineering team directly.

View Original Abstract

There is a considerable amount of literature on the electrical resistivity of iron at Earth’s core conditions, while only few studies have considered iron and iron-alloys at other planetary core conditions. Much of the total work has been carried out in the past decade and a review to collect data is timely. High pressures and temperatures can be achieved with direct measurements using a diamond-anvil cell, a multi-anvil press or shock compression methods. The results of direct measurements can be used in combination with first-principle calculations to extrapolate from laboratory temperature and pressure to the relevant planetary conditions. This review points out some discrepancies in the electrical resistivity values between theoretical and experimental studies, while highlighting the negligible differences arising from the selection of pressure and temperature values at planetary core conditions. Also, conversions of the reported electrical resistivity values to thermal conductivity via the Wiedemann-Franz law do not seem to vary significantly even when the Sommerfeld value of the Lorenz number is used in the conversion. A comparison of the rich literature of electrical resistivity values of pure Fe at Earth’s core-mantle boundary and inner-core boundary conditions with alloys of Fe and light elements (Si, S, O) does not reveal dramatic differences. The scarce literature on the electrical resistivity at the lunar core suggests the effect of P on a wt% basis is negligible when compared to that of Si and S. On the contrary, studies at Mercury’s core conditions suggest two distinct groups of electrical resistivity values but only a few studies apply to the inner-core boundary. The electrical resistivity values at the Martian core-mantle boundary conditions suggest a negligible contribution of Si, S and O. In contrast, Fe-S compositions at Ganymede’s core-mantle boundary conditions result in large deviations in electrical resistivity values compared to pure Fe. Contour maps of the reported values illustrate ρ( P , T ) for pure Fe and its alloys with Ni, O and Si/S and allow for estimates of electrical resistivity at the core-mantle boundary and inner-core boundary conditions for the cores of terrestrial-like planetary bodies.

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