Class Statistics
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.
Top Rare-Earth Permanent Magnets
Ranked by data richness — literature synthesis coverage, multi-source DFT corroboration, and patent activity.
| Formula | Band Gap | Best EAH (eV/atom) | Stability | DFT Sources | Recipes |
|---|---|---|---|---|---|
| Al2Dy6Fe2S14 | 0.21 eV | 0.0560 | Metastable | 2 | 0 |
| Dy6Fe2Ga2S14 | 0.44 eV | 0.0621 | Metastable | 2 | 0 |
| CeCoGe2 | Metallic / not reported | 0.0000 | On hull (stable) | 3 | 0 |
| Co2Nd8S14 | 0.09 eV | 0.1942 | Above hull | 1 | 0 |
| Fe2P2Sm2 | 0.10 eV | 0.0905 | Metastable | 1 | 0 |
| Co1I12Tb7 | 0.28 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Dy3GaFeS7 | 0.44 eV | 0.0621 | Metastable | 1 | 0 |
| Dy4FeSe7 | 0.17 eV | 0.0847 | Metastable | 1 | 0 |
| Fe2Ga2Nd6S14 | 0.02 eV | 0.0392 | Metastable | 1 | 0 |
| Fe2S14Sm8 | 0.52 eV | 0.1694 | Above hull | 1 | 0 |
| Nd3GaFeS7 | 0.02 eV | 0.0392 | Metastable | 1 | 0 |
| Nd4FeS7 | 0.48 eV | 0.1658 | Above hull | 1 | 0 |
| Pr12Co6Pb | 0.05 eV | 0.0439 | Metastable | 1 | 0 |
| Pr3InFeS7 | 0.29 eV | 0.0627 | Metastable | 1 | 0 |
| Pr4FeS7 | 0.32 eV | 0.1675 | Above hull | 1 | 0 |
| Sm12Co6Sn | 0.03 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Sm3AlFeS7 | 0.19 eV | 0.0357 | Metastable | 1 | 0 |
| Sm4FeS7 | 0.52 eV | 0.1694 | Above hull | 1 | 0 |
| SmFeP | 0.10 eV | 0.0905 | Metastable | 1 | 0 |
| Tb7CoI12 | 0.28 eV | 0.0000 | On hull (stable) | 1 | 0 |
| CeCo2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CeCoSi | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CeCoGe | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CeFeSi | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CeCo3 | Metallic / not reported | 0.0278 | Metastable | 2 | 0 |
| CeFe2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CoDySi2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| Ce2Fe17 | Metallic / not reported | 0.0412 | Metastable | 3 | 0 |
| Ce2Co17 | Metallic / not reported | 0.0119 | Near hull (likely stable) | 3 | 0 |
| Ce2FeSi3 | Metallic / not reported | 0.1069 | Above hull | 3 | 0 |
| Co4Dy2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| Ce2Co4 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| Co4Dy4Sn4 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| BCoDy | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| BCoTb | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| NdFe2 | Metallic / not reported | 0.0809 | Metastable | 2 | 0 |
| Co2Ge2Pr2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| CoDySi | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| Co2Dy2Si4 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| Co2Dy4Si4 | Metallic / not reported | 0.0081 | Near hull (likely stable) | 2 | 0 |
| FeNdSi2 | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| BCoPr | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| C4Ce2Co2 | Metallic / not reported | 0.0000 | On hull (stable) | 2 | 0 |
| Co2Nd | Metallic / not reported | 0.0766 | Metastable | 1 | 0 |
| Fe2Si4Tb4 | Metallic / not reported | 0.0200 | Near hull (likely stable) | 2 | 0 |
| CeCoFe | Metallic / not reported | 0.0050 | Near hull (likely stable) | 1 | 0 |
| CeCoGeH | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| CeCoRh | Metallic / not reported | 0.0374 | Metastable | 1 | 0 |
| CoDySn | Metallic / not reported | 0.0000 | On hull (stable) | 1 | 0 |
| CoNiPr | Metallic / not reported | 0.0848 | Metastable | 1 | 0 |
Frequently Asked Questions
How many rare-earth permanent magnets are in the database?
What is the most data-rich rare-earth permanent magnet?
Which rare-earth permanent magnet has the widest band gap?
Why are rare-earth magnets stronger than conventional ferrite magnets?
What is the primary difference between Neodymium and Samarium-Cobalt magnets?
Why is the supply chain for rare-earth magnets considered a strategic concern?
Can rare-earth magnets be recycled effectively?
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