Magnetic Materials

Rare-Earth Permanent Magnets

Nd2Fe14B and SmCo5 intermetallics whose 4f-3d exchange coupling yields the strongest permanent magnets known — and one of the most strategically concentrated supply chains in clean energy.

At a glance

Class Statistics

Compounds Tracked
20,957
Multi-Source DFT
0
With Synthesis Routes
14
Avg. Agreement
0.97 / 1.00
Overview

What are Rare-Earth Permanent Magnets?

Rare-earth permanent magnets represent the pinnacle of magnetic material performance, characterized by their exceptional energy products and high coercivity. These materials are primarily intermetallic compounds that leverage the unique electronic structure of rare-earth elements, specifically the 4f electron orbitals, which provide high magnetocrystalline anisotropy. When combined with transition metals like iron or cobalt, these elements facilitate strong 3d-4f exchange coupling, resulting in magnets that can maintain high magnetic flux densities even in compact geometries. The two most prominent classes are Neodymium-Iron-Boron (Nd2Fe14B) and Samarium-Cobalt (SmCo5 or Sm2Co17). Neodymium magnets are favored for their superior magnetic strength and cost-effectiveness in ambient temperature applications, such as electric vehicle motors and wind turbine generators. Conversely, Samarium-Cobalt magnets are prized for their remarkable thermal stability and resistance to oxidation, making them the preferred choice for high-temperature environments like aerospace and defense systems. The strategic importance of these materials cannot be overstated; they are foundational components in the global transition toward electrification and renewable energy. However, their production is characterized by a highly concentrated supply chain, involving complex extraction and refining processes that present significant geopolitical and environmental challenges. As the demand for high-efficiency motors grows, research is increasingly focused on reducing heavy rare-earth content, such as dysprosium or terbium, which are often added to enhance thermal performance, while simultaneously exploring recycling pathways to mitigate supply volatility.

Members

Top Rare-Earth Permanent Magnets

Ranked by data richness — literature synthesis coverage, multi-source DFT corroboration, and patent activity.

FormulaBand GapBest EAH (eV/atom)StabilityDFT SourcesRecipes
CeFe4Sb120.23 eV0.0000On hull (stable)—4
Ce2Fe17Metallic / not reported0.0412Metastable12
CeFe2Metallic / not reported0.0000Stable11
DyCoSi1.39–2.29 eV0.0000Stable10
DyCoSn2.44 eV0.0000Stable10
TbCoSi1.36–2.36 eV0.0000Stable10
TbCoSn2.62 eV0.0000Stable10
Ce(FeSb3)4Metallic / not reported0.0000On hull (stable)—4
NdFeSi1.54 eV0.0000Stable10
TbCo0.26 eV0.1539Unstable10
SmFeP0.09 eV0.0906Unstable10
CeFe4P120.46–0.52 eV0.0000Stable10
Dy4FeSe70.04–0.17 eV0.0847Unstable10
Dy8Ga3Co0.03 eV0.0000Stable10
Pr3AlFeS70.45 eV0.0273Metastable10
Sm3AlFeS70.40 eV0.0000Stable10
CeCoGeMetallic / not reported0.0000Stable10
CeFe4As120.32 eV0.0000Stable10
Dy3GaFeS70.39 eV0.0499Metastable10
Dy8In3Co0.10 eV0.0000Stable10
Nd3GaFeS70.46 eV0.0484Metastable10
Pr3InFeS70.57 eV0.0725Metastable10
Sm4FeS70.02 eV0.0768Metastable10
Tb7CoI120.18 eV0.0000Stable10
CeCo2Metallic / not reported0.0000Stable10
CeCoGe2Metallic / not reported0.0000Stable10
CeCoF61.33 eV0.0856Metastable—0
FeI12Pr70.19 eV0.0000On hull (stable)—0
Sm2Co17Metallic / not reported0.0000On hull (stable)—3
Co17Sm2Metallic / not reported0.0000On hull (stable)—3
Dy3FeGaS70.44 eV0.0621Metastable—0
FeGaNd3S70.02 eV0.0392Metastable—0
FeGaNd3Se70.13 eV0.0271Metastable—0
FeGaS7Sm30.08 eV0.0416Metastable—0
FeGaS7Tb30.07 eV0.0518Metastable—0
FeInPr3S70.29 eV0.0627Metastable—0
CeCoSiMetallic / not reported0.0000Stable10
CeCo3Metallic / not reported0.0054Stable10
CeFeSiMetallic / not reported0.0000Stable10
CeCo0.34–0.72 eV0.0217Near hull (likely stable)—0
SmCo0.74 eV0.0701Metastable—0
DyCo0.28 eV0.0000On hull (stable)—0
NdCo0.35–0.69 eV0.1233Above hull—0
PrCo0.37–0.67 eV0.1426Above hull—0
CeCoRhMetallic / not reported0.0000Stable10
CeCoGeHMetallic / not reported0.0000Stable10
TbUFe13.22 eV0.3110Above hull—0
AcTbFe10.52 eV0.5206Above hull—0
CeCoTe0.82 eV0.3236Above hull—0
DyCoTe0.88 eV0.1216Above hull—0
Reference

Frequently Asked Questions

How many rare-earth permanent magnets are in the database?

20,957 rare-earth permanent magnets are tracked, of which 0 have multi-source DFT validation and 14 have documented synthesis routes.

More questions
What is the most data-rich rare-earth permanent magnet?
CeFe4Sb12 is the most thoroughly characterized, with 1 reported structures.
Which rare-earth permanent magnet has the widest band gap?
Among the top compounds, TbUFe has the widest reported DFT band gap (13.22 eV).
Why are rare-earth magnets stronger than conventional ferrite magnets?
Rare-earth magnets possess significantly higher magnetic anisotropy and saturation magnetization due to the interaction between the 4f electrons of rare-earth elements and the 3d electrons of transition metals, allowing them to store much more magnetic energy in a smaller volume.
What is the primary difference between Neodymium and Samarium-Cobalt magnets?
Neodymium magnets offer the highest magnetic strength for general applications, while Samarium-Cobalt magnets are specifically engineered to maintain their magnetic properties at elevated temperatures and in corrosive environments.
Why is the supply chain for rare-earth magnets considered a strategic concern?
The extraction and processing of rare-earth elements are geographically concentrated, creating dependencies that can lead to market volatility and supply disruptions, which poses risks to industries reliant on clean energy technologies.
Can rare-earth magnets be recycled effectively?
Yes, recycling technologies are being developed to recover rare-earth elements from end-of-life magnets, though the process remains technically challenging due to the complex coatings and assembly methods used in modern devices.
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