Can Superconductivity Be Achieved at Room Temperature and Ambient Pressure?

The core insight

No one knows whether there exists a stable material, at ordinary pressure, in which electrons pair up and flow without resistance at room temperature — because we do not yet have a complete theory of why some materials superconduct at unexpectedly high temperatures at all.

The question, precisely

Strip away the popular-science shimmer and the question splits into two, tightly linked.

First: is there a fundamental physical limit on the superconducting transition temperature TcT_c for a material stable at ambient pressure, and if so, what sets it? Is room temperature (roughly 293–300 K) achievable in principle, or does something in the physics of chemical bonding, lattice stability, and electron correlation cap TcT_c well below that, forcing high pressure as the only route past a few hundred kelvin?

Second, and more fundamental: what is the actual pairing mechanism responsible for high-temperature superconductivity in the copper-oxide (cuprate) superconductors and their cousins — the iron-based superconductors, the nickelates — discovered since 1986? BCS theory explains conventional superconductors with great precision. It does not obviously explain why cuprates superconduct at temperatures four to five times higher than BCS physics comfortably allows. Thirty-eight years after their discovery, there is still no theory of cuprate superconductivity commanding the kind of consensus BCS commands for simple metals.

These two questions are entangled because engineering our way to room-temperature ambient-pressure superconductivity — rather than stumbling onto it by luck — requires knowing what actually causes high TcT_c in the first place. Without a predictive theory, the search is closer to alchemy than to design: synthesize a candidate, cool it, measure, hope. A real answer would look like this: a microscopic theory that takes a material's chemical formula and crystal structure and predicts TcT_c to within experimental error — for cuprates, for hydrides, for anything — the way BCS theory predicts TcT_c for lead or niobium from measurable phonon spectra. Short of that gold standard, even a settled, evidence-backed identification of the pairing glue in cuprates — spin fluctuations, some other purely electronic mechanism, or something stranger — would count as answering half the question. And a material that superconducts above 273 K at 1 atmosphere, reproduced independently in multiple laboratories, would answer the other half outright, whether or not we fully understood why.

What we know — a century of pairing up

Superconductivity's first sixty years were a triumph of patient empiricism chasing an increasingly frustrating theoretical gap. Onnes found it in mercury in 1911; over the following decades, physicists found it in lead, tin, niobium, and dozens of alloys, always at temperatures near absolute zero, always seemingly capped somewhere below 25 K no matter what was tried. Meissner and Ochsenfeld showed in 1933 that a superconductor doesn't just carry current with zero resistance — it actively expels magnetic field from its interior, the Meissner effect, a fact that turned out to be as fundamental as zero resistance itself and signaled that superconductivity was a genuine new phase of matter, not merely "very good conductivity."

The theoretical breakthrough came in 1957, when John Bardeen, Leon Cooper, and John Robert Schrieffer published what is simply called BCS theory. Its central insight is almost impertinent in its simplicity: two electrons, which repel each other ferociously through the bare Coulomb force, can nonetheless form a weakly bound pair — a Cooper pair — through the mediation of the crystal lattice itself. An electron moving through a lattice of positive ions tugs them slightly inward as it passes, leaving a trailing wake of enhanced positive charge; a second electron, arriving slightly later, feels an attraction to that wake rather than to the first electron directly. The attraction is retarded, indirect, and weak — but at low enough temperature, it is enough. Cooper had shown in 1956 that in a filled Fermi sea, any attractive interaction, however feeble, causes electrons near the Fermi surface to bind into pairs; BCS then showed that the whole electron gas condenses collectively into a coherent quantum state built from such pairs, all sharing one macroscopic wavefunction with a single phase. Resistance vanishes because scattering a single electron out of that state costs a finite energy — the superconducting gap Δ\Delta — and at low temperature there simply isn't enough thermal energy lying around to pay the toll.

This is phonon-mediated coupling: the lattice vibrations, quantized as phonons, serve as the glue. BCS theory produces a startlingly successful formula,

kBTc≈1.13 ℏωD e−1/N(0)V,k_B T_c \approx 1.13\, \hbar\omega_D \, e^{-1/N(0)V},

relating TcT_c to the Debye frequency ωD\omega_D (how stiff and how light the lattice is), the density of electron states at the Fermi level N(0)N(0), and the pairing interaction strength VV. It correctly predicts the isotope effect — that TcT_c shifts when you swap an element for a heavier isotope, exactly as you'd expect if lattice vibrations were doing the work. It explains the energy gap seen in tunneling experiments, the specific heat jump at TcT_c, the exponential suppression of TcT_c at weak coupling. For conventional superconductors — mercury, lead, niobium, and the workhorse niobium-titanium alloy inside every MRI magnet on Earth — BCS theory is not a rough guide; it is, essentially, exact.

But the same formula that explains BCS superconductors also explains why physicists spent decades assuming a hard ceiling existed. Because TcT_c depends exponentially on the pairing strength, and because stronger electron-phonon coupling also tends to destabilize the crystal lattice itself (a lattice that couples too strongly to its electrons is prone to structural distortion or collapse), reasonable estimates through the 1960s and 70s suggested phonon-mediated superconductivity could not plausibly exceed roughly 30–40 K. For a while it looked like nature's answer to "how hot can a superconductor be" was simply: not very.

Then, in 1986, Georg Bednorz and K. Alex Müller, working at IBM Zürich, found superconductivity at 35 K in a brittle, black ceramic — a layered copper-oxide compound, lanthanum barium copper oxide — a material class nobody expected to superconduct at all, since ceramics are usually insulators. Within a year, Paul Chu's group had pushed a related compound, YBa₂Cu₃O₇ (YBCO), to 92 K — above the boiling point of liquid nitrogen, a genuinely cheap, genuinely accessible coolant. The <span class="wiki-link-missing">cuprate high-Tc superconductors</span> had arrived, and the supposed BCS ceiling was shattered within eighteen months.

What makes cuprates strange is not just the temperature — it's the starting material. Undoped, a cuprate like La₂CuO₄ is not a good metal at all; it's a Mott insulator, a material that band theory says should conduct but which is instead insulating because the electrons repel each other too strongly to move freely, each one locked to its own copper site by Coulomb repulsion, spins forming an antiferromagnetic checkerboard. Superconductivity emerges only once you dope this Mott insulator — chemically substitute atoms to inject or remove electrons from the copper-oxide planes — carving out a rich, strange phase diagram as a function of doping and temperature.

The Resistance That Won't Die

In a basement laboratory in Leiden in April 1911, Heike Kamerlingh Onnes watched the electrical resistance of a thread of frozen mercury vanish—not fade, not diminish, but drop to a value indistinguishable from zero—the moment his thermometer crossed 4.2 kelvin. He wrote the observation in his lab notebook with the flat understatement of a man who did not yet know he'd found a hole in the fabric of solid-state physics: kwik nagenoeg nul — "mercury practically zero." Practically zero was, it turned out, actually zero. A current started circulating in a superconducting ring can, in principle, run for longer than the age of the universe without measurable decay.

More than a century later, we still cannot make that happen in a wire on your desk at room temperature, in open air, for free. We can get superconductivity at temperatures that would have stunned Onnes—above the boiling point of liquid nitrogen, even flirting with the temperature of a chilly day outside—but only in materials squeezed to pressures found near the center of the Earth, or in compounds too delicate and expensive to wind into a magnet coil. The dream that has haunted condensed matter physics for a hundred years is deceptively simple to state: a material that carries electricity with zero resistance, at 20°C, at one atmosphere of pressure, cheaply and stably enough to rewire civilization. It remains, stubbornly, a dream.

This is one of the great open problems of matter and energy, not because we lack superconductors — we have thousands — but because we do not fully understand, even now, what rules govern how high the transition temperature can go, and whether nature permits it to go all the way to room temperature without extreme pressure as the toll for admission.

svg[The generic cuprate phase diagram: doping away from the parent antiferromagnetic insulator opens a superconducting dome, but the region above it — the pseudogap and the "strange metal" — remains only partly understood.] hole doping p → temperature T → antiferro- magnet superconducting dome pseudogap strange metal Fermi liquid optimal doping

That diagram — antiferromagnetic insulator on the left, an underdoped pseudogap region whose electronic structure is only partly gapped for reasons still argued over, a dome of superconductivity peaking near "optimal doping," and a mysterious strange metal phase overhead where resistivity rises linearly with temperature all the way from near-zero to room temperature and beyond, defying ordinary metal physics — is the central object that any theory of cuprates has to explain. It connects directly to the modern physics of correlated electron systems: materials where the electron-electron interaction is not a small correction to free-electron behavior but the dominant physics, and where phases of matter — magnetism, superconductivity, charge order, exotic "strange" metallicity — compete and intertwine on nearly equal energetic footing.

Where it breaks down

The trouble is this: BCS theory, in its original form, has no room for a Mott insulator as the parent compound of a superconductor, and no obvious mechanism to produce transition temperatures near 100 K from phonons alone in these materials. The electron-phonon coupling in cuprates, measured directly by various spectroscopic probes, appears too weak by most estimates to produce BCS pairing at the observed TcT_c through phonons doing all the work. And more tellingly, the symmetry of the pairing is wrong for a straightforward BCS story: conventional superconductors pair electrons into an isotropic, "s-wave" state, the gap is roughly the same magnitude in every direction on the Fermi surface, but cuprates pair into a d-wave state — the superconducting gap has four lobes, changes sign around the Fermi surface, and actually vanishes entirely along certain crystal directions. This was established with remarkable clarity through phase-sensitive Josephson junction experiments in the 1990s (notably by Dale Van Harlingen, Donald Ginsberg, and collaborators, and independently confirmed by tricrystal SQUID experiments led by Chang Tsuen and John Kirtley's collaborators at IBM). D-wave pairing is exactly what you'd expect if the pairing glue were not phonons but spin fluctuations — electrons scattering off the fluctuating antiferromagnetic spin correlations left over from the parent Mott insulator. That is suggestive, but suggestive is not proof: three and a half decades of increasingly sophisticated numerical and analytical work have failed to close the case.

The strange metal phase compounds the puzzle. In an ordinary metal, resistivity from electron-phonon scattering rises linearly with temperature at high TT, then saturates or drops toward a residual value at low TT, following the physics of Fermi-liquid quasiparticles — well-defined, long-lived electron-like excitations that are the bedrock assumption of almost all of standard solid-state physics. In the strange metal phase of cuprates, resistivity is linear in TT from a few kelvin all the way past room temperature, with no sign of saturation, and — most disturbingly — the scattering rate implied by that resistivity approaches a universal bound, roughly ℏ/τ∼kBT\hbar/\tau \sim k_B T, called the Planckian limit, as if the electrons are scattering as fast as quantum mechanics will allow. There may be no well-defined quasiparticles at all in this regime — the entire conceptual scaffolding of "electrons as particles that occasionally bump into things" may simply not apply. If the normal state you're pairing from isn't even a normal Fermi liquid, then extending BCS's Cooper-pairing logic — built on the premise of a well-defined Fermi surface with sharp electron and hole excitations — becomes conceptually shaky at its foundation, not just quantitatively.

Add to this the discovery, from 2015 onward, of hydrogen-rich compounds — hydrogen sulfide, then lanthanum hydride (LaH₁₀), then a series of others — that superconduct at temperatures rivaling or exceeding the cuprates, in some cases above 250 K, tantalizingly close to room temperature. These hydride superconductors appear, on current evidence, to be conventional BCS superconductors after all: hydrogen's extreme lightness gives an enormous phonon frequency (recall TcT_c scales with ωD\omega_D in the BCS formula), and under the crushing pressures used to synthesize them — over a million atmospheres, achieved by squeezing tiny samples between the tips of two diamonds in a diamond anvil cell — hydrogen atoms are forced into dense metallic lattices with exceptionally strong electron-phonon coupling. It's BCS theory, vindicated and pushed to its extreme, rather than refuted. But the achievement comes at a brutal price: those pressures are far beyond anything usable in a wire, a magnet, or a power line. The samples are microscopic, often unstable outside the anvil cell, and difficult even to characterize with full confidence. So the hydride story simultaneously reinforces BCS theory's power and underscores how far we remain from a practical room-temperature superconductor: we may know how to reach the temperature, but not yet how to do it without a diamond anvil doing the equivalent of a small planet's gravity on your sample.

And the field has also had to reckon, painfully, with the credibility of some of its own claimed breakthroughs. A 2020 paper reporting room-temperature superconductivity near 15°C in a carbonaceous sulfur hydride under extreme pressure was retracted by Nature in 2022 after concerns about data processing methods, and follow-up work by other groups failed to reproduce the result. The 2023 sensation around "LK-99," a copper-doped lead apatite claimed by a South Korean team to superconduct at ambient pressure and room temperature, ignited a frenzy of replication attempts within days — and collapsed within weeks, as multiple independent laboratories showed the observed effects (partial levitation, resistance drops) were consistent with ferromagnetic impurities and sample inhomogeneity rather than superconductivity. These episodes are worth naming plainly, not as gossip but as data about the field itself: the prize is so large, and the phenomenon so exacting to verify correctly (you need zero resistance, the Meissner effect, and a sharp specific-heat anomaly all coinciding at the same temperature, ideally in more than one lab, before you believe it), that both honest error and motivated overreach are recurring hazards on this frontier.

The contenders

No single accepted theory yet explains cuprate high-TcT_c superconductivity, but there are several serious, actively pursued research programs, and it's worth laying out their appeal and their trouble honestly.

Spin-fluctuation mediated pairing. The leading phenomenological picture treats the cuprates as doped Mott insulators where residual antiferromagnetic spin correlations, rather than phonons, provide the pairing glue — an electron moving through the lattice disturbs the local spin arrangement, and a second electron is attracted to that disturbance. This naturally produces d-wave pairing, matches a great deal of neutron scattering data showing a magnetic resonance mode that tracks superconductivity, and connects cuprates conceptually to other unconventional superconductors — heavy-fermion compounds, some iron-based superconductors, even certain organic superconductors — that also sit near antiferromagnetic instabilities and also pair with sign-changing gaps. Its trouble is that "spin-fluctuation theory" is really a family of related approaches (the fluctuation-exchange approximation, various renormalization-group treatments, slave-boson mean-field theories of the resonating-valence-bond idea originally proposed by Philip Anderson in 1987) rather than one sharp, universally agreed calculation, and getting from the qualitative picture to a quantitatively correct TcT_c from first principles has proven extraordinarily hard, because the physics is at strong coupling — precisely the regime where the mathematical tools that work beautifully for BCS (perturbation theory in a small coupling constant) break down.

Numerically exact and quasi-exact simulations of the Hubbard model. Much of the theoretical cuprate literature reduces the problem to the Hubbard model — a deliberately minimal toy model of electrons hopping between lattice sites with a single number, UU, encoding the Coulomb repulsion cost of two electrons sharing a site. It's a caricature of real cuprate chemistry, but a caricature many physicists believe captures the essential physics. Over the last decade, large international collaborations pooling several numerical methods — dynamical mean-field theory, density-matrix renormalization group, determinant quantum Monte Carlo, tensor-network methods — have cross-checked each other's results on this same model with unprecedented rigor. The verdict, as of the mid-2020s, is genuinely double-edged: these calculations do find a superconducting phase with d-wave pairing symmetry in the doped Hubbard model, at least in some parameter regimes and geometries, which is an important consistency check on the spin-fluctuation picture. But they also find that the model's superconductivity competes closely — sometimes losing — to stripe phases (coexisting charge and spin density modulations) and other competing orders, and the results depend sensitively on details (next-nearest-neighbor hopping, the precise value of UU, ladder geometry versus full two-dimensional lattices) in ways that make some researchers doubt whether the single-band Hubbard model, however faithfully simulated, truly contains all essential cuprate physics, or whether real cuprates need additional ingredients — longer-range interactions, the specific role of apical oxygen atoms, multi-band effects — left out of the minimal model.

Quantum criticality and the strange metal. A different, complementary research program focuses less on the mechanism of pairing itself and more on the strange metal phase from which superconductivity emerges, arguing that the superconductivity might be almost a secondary phenomenon — a low-temperature instability of an even stranger, more fundamental "parent" quantum state. This program draws on the idea of a quantum critical point hidden under the superconducting dome, a zero-temperature phase transition (perhaps involving the pseudogap's mysterious partial gapping, or a hidden order parameter never directly observed) whose quantum fluctuations, fanning out to finite temperature, would naturally produce both the linear-in-TT Planckian resistivity and an enhanced, non-phonon pairing glue. This connects, intriguingly and at a deep conceptual level, to ideas from a completely different corner of physics: string-theory-inspired holographic duality techniques (the AdS/CFT correspondence) have been used by theorists including Subir Sachdev, Sean Hartnoll and others to construct toy "holographic superconductors" and strange-metal models that reproduce Planckian scattering, offering a strange, unexpected bridge between gravitational physics and correlated electron matter. It's a beautiful and mathematically rich program, but its critics note, fairly, that it has so far produced qualitative, universal-scaling insight more than material-specific, falsifiable predictions — it can explain that Planckian behavior is natural near quantum criticality, but has not yet nailed down which cuprate compound should have which TcT_c.

Phonon revival and multi-channel pairing. It would be a mistake to write phonons out of the cuprate story entirely. Some researchers argue the mainstream narrative has been too quick to dismiss electron-phonon coupling, pointing to strong isotope effects observed in underdoped cuprates and to angle-resolved photoemission spectroscopy (ARPES) data showing "kinks" in the electron dispersion consistent with coupling to specific optical phonon modes, particularly involving the apical oxygen atoms above and below the copper-oxide planes. The likeliest resolution many researchers now favor is not "phonons versus spin fluctuations" as a binary choice but some cooperative combination — spin fluctuations providing the dominant pairing glue while phonons contribute a supporting, non-negligible boost, the two channels reinforcing each other in a way genuinely new theoretical tools are only beginning to disentangle.

The materials-design program for hydrides and beyond. Running in parallel to the theoretical arguments over cuprates is a distinct, more empirical research program: use machine-learning-accelerated crystal structure search and density functional theory to predict which hydrogen-rich (or boron-, or other light-element-rich) compounds should have the strongest possible electron-phonon coupling, then attempt synthesis under high pressure. This program is squarely built on trusting BCS/Migdal-Eliashberg theory (the more sophisticated, strong-coupling extension of BCS developed by Gerasim Eliashberg) as essentially correct for these hydrides, and using it predictively — an approach that has scored real, independently verified successes, notably the 2015 prediction and subsequent 2019 confirmation of near-room-temperature superconductivity in LaH₁₀ near 250 K under roughly 170 gigapascals. Its central open challenge is not "does the theory work" but "can chemistry be found that keeps this behavior at lower, eventually ambient, pressure" — whether some clever combination of chemical pre-compression (using a cage of other atoms to squeeze hydrogen internally, without needing external mechanical pressure) can substitute for the diamond anvil.

Figure
Two roads to high T_c: cuprates rely on a doped Mott insulator and a contested electronic glue; hydrides rely on conventional phonon glue pushed to its extreme by pressure — neither yet reaches room temperature at one atmosphere.
Cuprates Hydrides Mott insulator (parent) doping → spin fluctuations? d-wave pairing, T_c ≈ 90–130 K ambient pressure ✓ mechanism: contested light element (H) metal extreme pressure ~100–200 GPa s-wave (BCS) pairing, T_c up to ≈250 K mechanism: understood (BCS) ambient pressure: ✗ (so far)

What would settle it

Answering the mechanism question and answering the room-temperature-at-ambient-pressure question require different kinds of evidence, and it's worth separating them.

For the mechanism of cuprate superconductivity, the decisive evidence would most likely come from convergence, not a single knockout experiment: numerical simulations of increasingly realistic multi-band models (going beyond the single-band Hubbard model to include the specific orbital physics of real copper-oxide planes) that reproduce not just d-wave pairing but the correct TcT_c, the correct doping dependence, and the correct connection to the pseudogap and strange-metal phases, cross-validated against ever more precise spectroscopic measurements — resonant inelastic x-ray scattering (RIXS), which can now map spin excitations with a precision unavailable a decade ago, and ARPES with ever finer energy and momentum resolution. Quantum simulators — ultracold atoms trapped in optical lattices engineered to mimic the Fermi-Hubbard model exactly, an approach pursued by groups including Markus Greiner's and Waseem Bakr's laboratories — offer another route: build a defect-free, fully controllable analog of the theorist's toy model in the lab, using actual atoms instead of solving equations on a computer, and simply measure whether it superconducts and how. This sidesteps the approximations of any numerical method, though reaching temperatures cold enough (in units of the relevant hopping energy) to see pairing directly has been a persistent technical struggle, one that has seen real recent progress. A firm, quantitative match between such a "quantum simulation" and real cuprate behavior — or a clear demonstration that the minimal Hubbard model cannot reproduce cuprate TcT_c's, forcing theorists to admit missing ingredients — would each, in its own way, be genuinely decisive.

For the practical goal of ambient-pressure room-temperature superconductivity, the criterion for "settled" is unambiguous and has been for decades: independent replication, in at least two or three separate laboratories, of a material showing all three simultaneous fingerprints — zero DC resistance below some Tc≥293T_c \geq 293 K, the Meissner effect (magnetic field expulsion, ideally shown via both magnetization measurements and direct imaging), and a sharp thermodynamic anomaly (a jump in specific heat) at that same temperature — measured on a sample stable at one atmosphere of pressure. Any claim lacking Meissner data, or resting on unusual single-lab measurements of partial resistance drops or anomalous magnetic susceptibility alone, should be treated as provisional at best, exactly the lesson of the retracted 2020 hydride claim and the LK-99 episode. Given how thoroughly and how fast the community now mobilizes to check extraordinary claims — LK-99 was checked, debated, and substantially debunked within roughly a month, an extraordinary pace for materials science — the infrastructure for verification is arguably in a healthier state now than at any earlier point in the field's history, even though the underlying physics remains as hard as ever.

As for timing: honest researchers in the field decline to give a confident date, and that reticence is itself informative — this is a problem that has resisted focused effort by thousands of very capable physicists for decades. Machine-learning-guided materials discovery, increasingly sophisticated correlated-electron simulation on both classical and early quantum computers, and continued high-pressure hydride chemistry are all active, well-funded, rapidly moving fronts; each could plausibly produce a surprise within the next decade. But "plausibly within a decade" has been said, honestly, for several decades running, and there is no guarantee nature has left room-temperature ambient-pressure superconductivity available at all outside of exotic pressure conditions.

Why it matters

The stakes are not abstract. Roughly five to ten percent of all electricity generated worldwide is lost to resistive heating in transmission and distribution before it ever reaches a light bulb or a factory floor — a bill of hundreds of billions of dollars and a proportional slice of humanity's carbon output, paid every single year simply because copper and aluminum wires are not perfect conductors. A cheap, stable, ambient-pressure room-temperature superconductor would let that loss largely vanish. It would make today's cumbersome liquid-helium-cooled superconducting magnets — the ones inside every MRI scanner, every large particle accelerator, every design for a compact fusion reactor pursuing the goals discussed under controlled nuclear fusion — into simple, cheap, uncooled components, radically shrinking the size and cost of high-field magnets and potentially accelerating the timelines of fusion devices that depend on ever-stronger magnetic confinement. It would transform electric motors, generators, maglev transport, and quantum computing hardware, much of which already depends on superconducting circuits (the superconducting qubits in current quantum processors are themselves a direct descendant of Cooper pairing physics) that currently require dilution refrigerators reaching millikelvin temperatures.

But the deeper stakes are intellectual, and they connect to one of the largest live questions in all of physics: how collections of many strongly interacting quantum particles organize themselves into qualitatively new behavior that cannot be predicted just by knowing the rules governing any one particle. Cuprates are a flagship example of emergence — Mott insulators, antiferromagnets, strange metals and d-wave superconductors all arising from what is, at bottom, simply electrons and ions obeying the ordinary rules of quantum electrodynamics at low energy. Understanding how that emergence works, precisely and predictively, would be a triumph on the scale of BCS theory itself, and the tools built to attack it — the numerical methods for strongly correlated systems, the classification of unconventional pairing symmetries, the study of quantum criticality and Planckian transport — bleed directly into neighboring frontiers, including the study of exotic topological quantum matter, where some of the same correlated-electron machinery is used to hunt for Majorana modes, fractionalized excitations, and other states of matter with no classical analog at all. Solving the cuprate mechanism problem would very likely hand physics a general theory of strongly correlated quantum matter — a prize whose value would extend far past superconductivity itself.

The people chasing it

Origins · 1 minHeike Kamerlingh Onnes and how this was discovered
HK
Heike Kamerlingh Onnes
1853–1926 · Discovered superconductivity in mercury in 1911 at his Leiden cryogenics laboratory, the first place on Earth able to liquefy helium; won the 1913 Nobel Prize in Physics.

physicist[John Bardeen|1908–1991|Co-developed BCS theory with Cooper and Schrieffer in 1957, becoming the only person ever to win the Nobel Prize in Physics twice — the first for the transistor, the second for superconductivity.]

Origins · 1 minJ. Georg Bednorz and K. Alex Müller and how this was discovered
JG
J. Georg Bednorz and K. Alex Müller
Bednorz b. 1950; Müller 1927–2023 · IBM Zürich researchers who discovered superconductivity above 30 K in a lanthanum-copper-oxide ceramic in 1986, opening the cuprate era and earning the Nobel Prize the following year — an unusually fast recognition.

physicist[Philip W. Anderson|1923–2020|Proposed the resonating-valence-bond theory of cuprates in 1987, arguing the physics of the doped Mott insulator, not phonons, was the key to high-TcT_c superconductivity — a still-influential, still-contested framework.]

Origins · 1 minMikhail Eremets and how this was discovered
ME
Mikhail Eremets
b. 1955 · Max Planck Institute for Chemistry researcher whose high-pressure diamond-anvil-cell experiments produced the landmark hydrogen sulfide (2015) and lanthanum hydride (2019) superconductivity results, establishing conventional phonon-mediated pairing near 200–250 K under extreme pressure.

Beyond these names stand thousands of working physicists, chemists, and materials scientists: the numerical collaborations (the "Simons Collaboration on the Many-Electron Problem" pooled a dozen competing computational methods on the Hubbard model specifically to force honest cross-validation); the ARPES and RIXS spectroscopists mapping electronic structure photon by photon; the high-pressure chemists racing to find hydride compounds stable at ever-lower pressure; and, notably, the community of skeptical replicators — the labs around the world that dropped what they were doing to test LK-99 within days of its announcement, exemplifying a peer-review process happening in real time, in public, faster than any journal could referee it.

history 1911 — Onnes discovers superconductivity in mercury at 4.2 K. 1957 — Bardeen, Cooper, and Schrieffer publish BCS theory. 1986 — Bednorz and Müller discover cuprate superconductivity above 30 K. 2015 — Eremets and colleagues report superconductivity near 203 K in compressed hydrogen sulfide.

The open frontier

Stand back from the details and a strange, humbling picture emerges. We have superconductors that work near room temperature and we have superconductors that work at ambient pressure — we have simply never had both at once in the same material, verified beyond doubt. It is one of the few genuinely open frontiers in physics where the basic experimental fact — does a working device exist — is as uncertain as the theory behind it, and where the theory of the best-known high-temperature examples, the cuprates, has resisted forty years of extraordinarily talented effort without full resolution. That combination of empirical accessibility (anyone with access to a decent lab could in principle be the one to find the next surprise) and theoretical depth (the problem sits at the genuine edge of what many-body quantum mechanics lets us calculate) is part of why this question exerts such a pull on physicists and public alike. It is not a question awaiting one clever experiment so much as a question awaiting the maturation of an entire toolkit — better simulations, better spectroscopy, better materials chemistry, and perhaps a genuinely new theoretical idea nobody has had yet.

What remains unresolved, stated plainly:

  • Is the dominant pairing glue in cuprates spin fluctuations, a cooperative mix of spin fluctuations and phonons, or something not yet identified — and can any theory predict cuprate TcT_c quantitatively from first principles?
  • What is the strange metal phase, physically — is it evidence of a hidden quantum critical point, a breakdown of the quasiparticle concept altogether, or something else entirely?
  • Can chemical pre-compression or entirely new light-element compounds deliver hydride-like TcT_c values without needing hundred-gigapascal external pressure?
  • Is there a fundamental thermodynamic or structural reason no stable ambient-pressure material can superconduct above roughly 250–300 K, or is this simply a materials-search problem still awaiting its answer?
  • Could a fundamentally new class of pairing mechanism — engineered through synthetic quantum matter, twisted two-dimensional materials, or ideas from topological physics — sidestep the whole cuprate/hydride dichotomy?

Ask the tutor: If spin fluctuations really are the glue holding Cooper pairs together in the cuprates, why has that idea, unlike BCS theory, never produced an equally precise formula for predicting a material's transition temperature — and what would it take to get one?