Cuprate Superconductors
Layered copper-oxide superconductors — YBCO, BSCCO — with critical temperatures above liquid nitrogen. Coated-conductor tapes now feed compact fusion magnets and power transmission.
Class Statistics
What are Cuprate Superconductors?
Cuprate superconductors represent a transformative class of ceramic materials characterized by their complex, layered crystal structures containing copper-oxide planes. These materials are defined by their ability to exhibit superconductivity—the total absence of electrical resistance—at temperatures significantly higher than those achieved by traditional metallic superconductors. The chemistry typically involves rare-earth elements, alkaline earth metals, and copper, arranged in repeating units that facilitate the movement of charge carriers. The discovery of these materials was a landmark event in condensed matter physics because it pushed the transition temperature above the boiling point of liquid nitrogen, a milestone that drastically reduced the cost and complexity of cooling systems required for practical applications. Notable members of this family include Yttrium Barium Copper Oxide (YBCO) and Bismuth Strontium Calcium Copper Oxide (BSCCO). Beyond their theoretical significance in understanding non-conventional electronic states, cuprates are currently at the forefront of industrial engineering. They are manufactured into flexible, high-performance coated-conductor tapes that carry immense current densities. These tapes are now integral to the development of next-generation technologies, including compact, high-field magnets for fusion energy reactors, advanced medical imaging systems, and efficient power transmission grids. As researchers continue to refine the synthesis and grain boundary engineering of these ceramics, cuprates remain the primary candidate for achieving robust, high-temperature superconducting devices that operate outside of specialized cryogenic laboratories.
Top Cuprate Superconductors
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 |
|---|---|---|---|---|---|
| La2CuO4 | 0.06 eV | 0.0000 | On hull (stable) | 2 | 8 |
| BaCuO2 | 0.19–0.28 eV | 0.0000 | On hull (stable) | 2 | 1 |
| CaCuO2 | 0.03–0.67 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Ca4Cu4O8 | 0.03–0.67 eV | 0.0000 | On hull (stable) | 2 | 0 |
| LaCuO2 | 2.52 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Cu2La4O8 | 0.06 eV | 0.0000 | On hull (stable) | 2 | 0 |
| TlCuO2 | 0.43 eV | 0.0248 | Near hull (likely stable) | 2 | 0 |
| YCuO2 | 0.02–2.65 eV | 0.0000 | On hull (stable) | 2 | 0 |
| CuBiO2 | 0.63–0.84 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Cu8O20Y8 | 0.09–0.33 eV | 0.0403 | Metastable | 2 | 0 |
| Sr2CuClO2 | 2.38 eV | 0.0000 | On hull (stable) | 2 | 0 |
| As4Cu4O16Tl8 | 1.44–1.61 eV | 0.0062 | Near hull (likely stable) | 2 | 0 |
| BaNd2CuO5 | 0.58 eV | 0.0210 | Near hull (likely stable) | 2 | 0 |
| BaPr2CuO5 | 0.43 eV | 0.0205 | Near hull (likely stable) | 2 | 0 |
| Y4Cu2O7 | 1.57 eV | 0.1043 | Above hull | 2 | 0 |
| Ba2ClCuO2 | 2.30 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Ba8Cu4I4O8 | 2.26 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Ca4Cu2Fe2O6S2 | 0.68 eV | 0.0673 | Metastable | 2 | 0 |
| Cl2Cu6Nd2O16Se4 | 0.02 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Cu2O12Te2Tl8 | 0.47 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Cu4La12O8S12 | 0.97 eV | 0.0000 | On hull (stable) | 2 | 0 |
| Ca1Cu1O2 | 0.03–0.67 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Ca2CuO3 | Metallic / not reported | 0.0018 | Near hull (likely stable) | 2 | 2 |
| Cu1Nd1O2 | 2.41 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu4La4O8 | 2.52 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cl1Cu1La1Nb2O7 | 0.31 eV | 0.0397 | Metastable | 1 | 0 |
| Cu18La18O36 | 2.52 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu1La1O2 | 2.52 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu1La2O4 | 0.06 eV | 0.0000 | On hull (stable) | 1 | 0 |
| NdCuO2 | 2.41 eV | 0.0000 | On hull (stable) | 1 | 0 |
| As4Ca4Cu4H4O20 | 0.29 eV | 0.0147 | Near hull (likely stable) | 1 | 0 |
| As8Ba4Cu4O28 | 0.68 eV | 0.0000 | On hull (stable) | 1 | 0 |
| H8Ba4Cu8O36P8 | 0.18 eV | 0.0093 | Near hull (likely stable) | 1 | 0 |
| Ba2Cu2O4 | 0.19–0.28 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Ca2Cu2O5 | 0.99 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu4La8O16 | 0.06 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Ba2Cu1O6U1 | 0.07 eV | 0.0085 | Near hull (likely stable) | 1 | 0 |
| Cu2O4Y2 | 0.02–2.65 eV | 0.0000 | On hull (stable) | 1 | 0 |
| LiLa4CuO8 | 0.02–0.77 eV | 0.0157 | Near hull (likely stable) | 1 | 0 |
| Mg14CuBiO16 | 1.66–1.94 eV | 0.1252 | Above hull | 1 | 0 |
| SrMg14CuO16 | 0.06–0.70 eV | 0.1046 | Above hull | 1 | 0 |
| YMg14CuO16 | 0.22 eV | 0.0959 | Metastable | 1 | 0 |
| Ba2Cu2Nd4O10 | 0.58 eV | 0.0210 | Near hull (likely stable) | 1 | 0 |
| Bi16Cu16O32 | 0.63–0.84 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Bi2Cu2O4 | 0.63–0.84 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Br4Cu4La4Nb8O28 | 0.23 eV | 0.0404 | Metastable | 1 | 0 |
| Ca4Cu4O28P8 | 0.03–0.69 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu1O2Y1 | 0.02–2.65 eV | 0.0000 | On hull (stable) | 1 | 0 |
| Cu4O8Y4 | 0.02–2.65 eV | 0.0000 | On hull (stable) | 1 | 0 |
| CuO2Y | 0.02–2.65 eV | 0.0000 | On hull (stable) | 1 | 0 |
Frequently Asked Questions
How many cuprate superconductors are in the database?
2,024 cuprate superconductors are tracked, of which 99 have multi-source DFT validation and 9 have documented synthesis routes.
What is the most data-rich cuprate superconductor?
Which cuprate superconductor has the widest band gap?
What makes cuprate superconductors different from conventional superconductors?
Why is the liquid nitrogen threshold important for these materials?
Are cuprate superconductors easy to manufacture into wires?
What are the primary applications for cuprate-based coated conductors?
Related Material Classes
Screen cuprate superconductors computationally
Evaluate stability, supply-chain risk, and patent whitespace before committing lab resources.
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