Ag1Au1K2
Ag1Au1K2 is a semiconducting ternary intermetallic compound currently being explored in the context of perovskite-related material research.

About Ag1Au1K2
Ag1Au1K2 is a semiconducting material composed of silver, gold, and potassium. It is categorized within the broad research landscape of halide perovskite-related structures, where researchers investigate unique electronic configurations for potential optoelectronic applications.
Despite its inclusion in structural databases, this compound is considered thermodynamically unstable, as it sits above the stability hull. Its existence as a reported structure highlights the ongoing effort to map the complex phase space of ternary and quaternary metallic systems.
Key Properties
Cross-validated computational properties for Ag1Au1K2, aggregated across 2 databases.
Band GapEnergy needed to move an electron from the valence band to the conduction band. Lower or zero values tend to behave more metallic; larger gaps are more insulating or semiconducting.
Energy Above HullThermodynamic distance from the most stable set of competing phases. 0 eV/atom is on the convex hull; small positive values may still be experimentally accessible.
StabilityA plain-language summary of the best reported energy-above-hull result. It reflects whether the lowest-energy structure is on, near, or far from the stability hull.
StructuresCount of reported calculated crystal structures for this formula, including alternate polymorphs, source databases, and observed space groups.
Reported Structures
Lowest-energy structures reported for Ag1Au1K2, ranked by energy above hull.
| Space GroupSymmetry classification of the crystal arrangement. The number is the international space-group index. | Crystal SystemBroad lattice family, such as cubic, tetragonal, monoclinic, or triclinic, derived from unit-cell symmetry. | Band Gap (eV)Electronic gap calculated for this specific reported structure, measured in electronvolts. | E above hull (eV/atom)Thermodynamic distance from the convex hull for this structure, normalized per atom. Lower is generally more stable. | E/atom (eV)Computed total energy normalized per atom. Use energy above hull, not this value alone, when comparing stability. | Density (g/cm³)Mass per relaxed crystal volume, reported in grams per cubic centimeter. |
|---|---|---|---|---|---|
| Immm (No. 71) | orthorhombic | 2.00 | 0.4923 | -20.658 | 0.44 |
| P2/m (No. 10) | — | — | — | — | — |
| P4/mmm (No. 123) | — | — | — | — | — |
| Pm (No. 6) | — | — | — | — | — |
| Cmmm (No. 65) | — | — | — | — | — |
| P4mm (No. 99) | — | — | — | — | — |
| Amm2 (No. 38) | — | — | — | — | — |
| C2/m (No. 12) | — | — | — | — | — |
| P4/mmm (No. 123) | — | — | — | — | — |
| Fm-3m (No. 225) | — | — | — | — | — |
| P4/mmm (No. 123) | — | — | — | — | — |
| P4/mmm (No. 123) | — | — | — | — | — |
Applications
Where Ag1Au1K2 is used.
Frequently Asked Questions
Common questions about Ag1Au1K2, answered from cross-validated data.
What is Ag1Au1K2?
Ag1Au1K2 is a semiconducting ternary intermetallic compound currently being explored in the context of perovskite-related material research.
What is Ag1Au1K2 used for?
What is the band gap of Ag1Au1K2?
Is Ag1Au1K2 a metal, semiconductor, or insulator?
Is Ag1Au1K2 thermodynamically stable?
What is the crystal structure of Ag1Au1K2?
What is the density of Ag1Au1K2?
How many polymorphs of Ag1Au1K2 are known?
What elements does Ag1Au1K2 contain?
Where does the data for Ag1Au1K2 come from?
How It Compares
Within the halide perovskite photovoltaics class.
Unlike the highly stable and widely utilized halide perovskite CsPbBr3, which serves as a benchmark for photovoltaic performance, Ag1Au1K2 represents a more exotic and less stable structural arrangement within the broader class of perovskite-related materials.
Related Compounds
Other Halide Perovskite Photovoltaics in the database.
Data sources & attribution
- materials_project — Data from the Materials Project. Cite: Jain et al., APL Materials 1, 011002 (2013).
- aflow — Data from AFLOW. Cite: Curtarolo et al., Comp. Mater. Sci. 58, 218 (2012).
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