Iron in Iron Selenide: How an Impurity That Kills Superconductivity Became Its Booster express

Original: "Superconductivity of 30.4 K and its Reemergence under Pressure in Fe1.11Se Synthesized via Ion-exchange and De-intercalation Reaction"
arXiv:2602.06312 · 2026-02-06 · CC BY 4.0 · 2 min
A crystal with excess iron, which usually destroys superconductivity, showed a record 30.4 K under pressure.

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In the crystal lattice of iron selenide, iron and selenium atoms alternate like bricks in a wall. But sometimes extra iron atoms sneak into the voids between them, like uninvited guests squeezing into the gaps between bricks. Just 3% of such 'guests' and superconductivity vanishes: the material stops conducting electricity without resistance. In the new study, researchers grew a crystal with 11% extra iron — three times the 'lethal' dose. And it still became a superconductor, with a transition temperature of 30.4 K — higher than many other iron-based superconductors.

The secret lies in the synthesis method. Usually, such crystals are made at high temperatures, when atoms have time to settle into the most comfortable positions, like passengers taking seats in an empty bus. Here, they used hydrothermal ion exchange: a solution under pressure washes out some atoms and inserts others, not letting the lattice 'relax'. As a result, the extra iron is trapped in unusual positions that are impossible at equilibrium. It's as if passengers were forced to stand in the aisle, even though there are free seats.

Under pressure, the superconducting temperature of the new crystal behaves unusually: it first drops to a minimum at 2–2.6 GPa, then rises again, forming a 'V'-shaped curve. Such behavior was previously seen only in FeSe intercalates — compounds where other atoms are inserted between the iron selenide layers.

Upon further compression, a magnetic order appears in the crystal, which was previously observed only in pure FeSe under pressure. So, the extra iron doesn't just not interfere, but actually helps 'switch on' new states of matter. The authors believe that non-equilibrium synthesis opens the door to materials with properties unattainable under ordinary conditions, as if we learned to build buildings not from a standard blueprint, but by assembling them from ready-made blocks in any order.

Original abstract

as written by the authors arXiv:2602.06312

Binary stoichiometry FeSe (s-FeSe) is a well-known parent of high-temperature unconventional superconductors owing to its charge-neutral layer, highly tunable structure and electronic properties, and rich interplays among multiple electronic phases. Yet the s-FeSe synthesized via high-temperature equilibrium reactions bears the notorious interstitial Fe,where merely 3% of them is sufficient to kill the superconductivity. Here, we successfully synthesized a new non-stoichiometric Fe1.11Se single crystal with a superconducting onset temperature (Tconset) of 30.4 K through a hydrothermal ion-exchange and de-intercalation route. 11% interstitial Fe ions exceed the equilibrium phase diagram limit. Intriguingly, under physical pressure, the Tconset of exhibits a "V"-shaped evolution with a minimum at 2-2.6 GPa, and then upturning into a second superconducting region, reminiscent of the behaviors in FeSe intercalates. Furthermore, a pressure-induced possible magnetic order, previously only observed in pressurized s-FeSe, shows up. These results offer fresh insights into the role of interstitial Fe in governing superconducting and transport properties under non-equilibrium synthesis and tuning strategies.

A temperature of 30.4 K is about -243°C, colder than the surface of Pluto, but for iron-based superconductors, it's a fairly 'warm' temperature.

Scientists
Wolfgang PauliSubrahmanyan ChandrasekharEnrico FermiLeo EsakiAugustin-Louis CauchyChristiaan Huygens
Concepts
high temperature superconductivity superconductivity dome nickelate high temperature superconductor silicon carbide superconducting gap gallium arsenide superconducting electronics cuprate faraday constant bcs theory niobium niobium nitride room temperature superconductivity transition temperature superconducting wire strain induced superconductivity magnetic flux quantum