(the heaviest Schrödinger's cat so far 🐈), yet its two states were only 1/800 of a proton apart.
In 2023, physicists in Zurich made a sliver of sapphire vibrate two opposite ways at once: a lab version of a cat that is both alive and dead. How heavy the vibration is depends on how you count. Its two states were far closer together than a proton is wide, and the double state lasted about 10 millionths of a second. Here's why distance is the hard part, and where gravity comes in.
In 1935 he imagined a cat shut in a steel box with a speck of radioactive material and a flask of poison. If one atom decays, the flask breaks. Quantum physics describes that atom as decayed and not decayed at once, until something checks. So the cat would be alive and dead at once. Absurd. That was his point.
Ninety years later, physicists build real "cats" on purpose, from atoms, light and even sound, and race to make them bigger. The heaviest so far weighs about as much as a fine grain of sand. Sort of.
🐈Chapter 1
16 micrograms
In April 2023, a team at ETH Zurich in Switzerland reported a new kind of cat: a sound wave inside a crystal.
In a small chip of sapphire, they trapped a vibration in a sliver about as wide as a hair. It rings like a tiny bell, about 6 billion times a second. They made it ring two opposite ways at once: in one version the atoms swing forward while, in the other, they swing back.
The vibration has an effective mass of 16 micrograms (Chapter 5 explains "effective"), and roughly 100 million billion atoms take part. As of 24 October 2026, we could find no heavier cat made of moving matter.
Three twists follow: the weight depends on how you count; the two states were astonishingly close; and Roger Penrose's idea that gravity itself ends such states would, by our rough estimate, give this cat millions of years. It is also about three quarters of a Planck mass, a natural unit we'll meet in Chapter 11.
📦Chapter 2
A quite ridiculous case
Schrödinger introduced his cat with the words "One can even set up quite ridiculous cases." (That's John Trimmer's 1980 translation.) He wasn't claiming cats are alive and dead. He meant that a strangeness harmless in one atom can be passed along, step by step, to something as big as a cat, where it plainly makes no sense.
So what is a "both at once" state, a superposition? It's not "secretly one or the other, we just don't know which". It's both possibilities together, locked in step, and they can interfere, like ripples on a pond that add up in some places and cancel in others. Interference is how physicists tell a real superposition from a coin toss nobody has looked at.
Two famous lab "cats" arrived in 1996: in the US, a single atom in two places at once; in Paris, a faint microwave field that the team watched lose its quantum strangeness as it leaked information to its surroundings. Today a "cat state" is any superposition of two clearly different states.
🗺️Chapter 3
A picture of two states at once
To draw something doing two things at once, physicists use a map: left to right is how far the vibrating atoms have swung, up and down is how fast they move.
In Nº 2, a state was a single dot on a map like this. Quantum physics doesn't allow a sharp dot. Even the calmest vibration is a round smudge, blurred by a quantum jitter that never goes away. A cat is two smudges with a row of stripes between them.
Here's the magic. The map works almost like a chart of chances, but the stripes dip below zero, and no ordinary chance can be less than zero. No mix of everyday vibrations can do that; only a true "both at once" can. The negative stripes are the cat's fingerprint.
Make the cat bigger and watch the stripes get finer. Then guess which fades first, the hills or the stripes, and press ▶ Watch it fade 👇
The stripes go first, and fast: for ETH's biggest cat, about 5 times faster than the energy leaks away, and bigger cats lose them faster still (Chapter 6 explains why). Now shrink the cat to zero and pick "Odd cat": a single quantum of sound, a ring on the map, and even that dips below zero in the middle. The map is an ideal version; the real cats faded a little faster.
🔔Chapter 4
A cat made of sound
The cat lives in a sandwich of two chips, in a fridge far colder than deep space.
One chip is sapphire, topped with a thin disc that turns electric pulses into squeezes. It sits face to face with a chip carrying a qubit, a tiny superconducting circuit that can itself be in two states at once. Through the disc, the qubit sends sound into the sapphire, where it bounces between the faces like a note in an organ pipe. Then:
Ring the crystal gently with a microwave pulse.
Put the qubit into a "both at once" state.
Let them trade energy. After about 3 millionths of a second the qubit almost lets go, leaving the sound ringing two opposite ways at once.
To read the cat, the qubit asks the sound one question, thousands of times: is the number of sound quanta even or odd? The answers rebuild the whole map, negative stripes and all.
The circuit has famous ancestors: the 2025 Nobel Prize in Physics went to John Clarke, Michel Devoret and John Martinis for showing, in 1984 and 1985, that a circuit far bigger than any atom can tunnel, slipping through an energy barrier it is too weak to climb, and take in energy only in fixed steps, like a single quantum object.
⚖️Chapter 5
Which 16 micrograms?
So what exactly weighs 16 micrograms? Not the chip, which is far heavier, and not a lump of crystal moving as one. In a ringing crystal every atom moves a different amount: neighbouring slabs move in opposite directions, and the middle of the beam moves most. To give such a vibration one "mass", physicists compare it with a weight on a spring, and for that they must choose which wiggle to count.
Count the average wiggle: 16 micrograms, with the two states 1/800 of a proton apart. Count the biggest wiggle, in the middle: the same state is just 1 microgram, with its two states 4 times farther apart. Both are honest.
Pick a way of counting, or drag the dot along the line, and watch mass and distance trade places 👇
The "weight" changed 16 times over, the distance 4 times, and one thing not at all: mass × distance² (mass times the distance times itself). That's the number that both Penrose's gravity clock (Chapter 9) and most of the world's eavesdropping (Chapter 6) count. The physics doesn't care which ruler you pick, even if the headline does.
The paper's own down-to-earth unit is one thin slab of crystal, about 30 nanograms, that moves almost as one body. And nobody saw the cat: it was pieced together from thousands of measurements.
🔬Chapter 6
1/800 of a proton
A proton is tens of thousands of times smaller than an atom. Slice its width into 800 pieces: that's the gap between the cat's two states.
The crystal itself never went anywhere. The vibration as a whole was in two states at once: in one, the atoms in the vibrating part sat a touch forward; in the other, a touch back. The two settings were closer together than a proton is wide. That still counts: for the vibration as a whole, the gap is about 7 times its own quantum blur, so a measurement could, in principle, tell the two states apart.
Why so close? Because the world keeps eavesdropping. Anything that could tell the two states apart, from flaws in the crystal to the qubit itself, carries off a tiny record of which one, even if nobody reads it, and each record wipes out some of the stripes. The farther apart the states, the faster the world notices: twice the distance, 4 times faster.
ETH's sound lasted about 84 millionths of a second, but the stripes faded in about 10. Split the same crystal by a proton's width and they'd last about 20 trillionths of a second; by an atom's width, about 6 billionths of a trillionth of a second.
Heavy, or far apart.
Every "both at once" experiment has to choose. (Eavesdropping explains why the stripes vanish, not why we see one outcome; that puzzle is open. The same idea is behind one argument that empty space may never jiggle into anything at all: see Nº 3.)
🏆Chapter 7
Biggest by which ruler?
Is the heaviest cat also the biggest? Its main rival fires particles through gratings, combs of tiny slits (in the newest machines, combs made of laser light): a pattern appears at the far end only if each particle went through several slits at once.
On 21 January 2026, a team in Vienna reported this with sodium clusters of more than 7,000 atoms, each about 8 nanometres across. The crystal outweighs one cluster about 57 million million times. But each cluster was spread over more than 10 times its own size, a stretch tens of billions of times wider than the crystal's gap, and stayed that way about 1,000 times longer: 12 thousandths of a second against 10 millionths.
Every solid dot below is a real experiment. Tap one for its story, switch on Penrose's band (where gravity might end a superposition within a second, as Chapter 9 explains), then switch to the score and watch the winner change 👇
The score, macroscopicity, measures how hard an experiment tests quantum physics. It rewards mass and time, but only for states far enough apart, and it counts in powers of ten. The 2026 clusters hold the record: 15.5. An ETH crystal vibration like the cat's, holding a single quantum of sound, scored 11.3; we found no published score for the cat itself. Schrödinger's cat, kept in two states for a second, would score about 57.
Heaviest and highest score are different titles, and as of 24 October 2026 different experiments hold them.
⛰️Chapter 8
A size limit for quantum physics?
Maybe big things can't stay in two states at all. Some physicists propose a tiny new rule: now and then, at random, each particle gets pinned to one place. For one particle that's about once every 300 million years. But in a speck of a hundred thousand billion billion particles, less than a gram, one gets pinned every ten-millionth of a second. Because the particles are all tied together, that one pin snaps the whole speck into one state, as long as its two versions are more than about a ten-thousandth of a millimetre apart. These are collapse models; the best known dates from 1986.
There's a side effect: each pinning kicks a particle, and kicked charged particles give off light, so ordinary matter should glow very faintly with X-rays. Spotting that needs no cat, just a very quiet detector deep underground.
The strongest test so far came from a dark-matter detector, XENONnT, in an underground lab beneath Italy's Gran Sasso mountain. On 23 March 2026 its team reported no such glow, ruling out the original 1986 settings (once every 300 million years, a ten-thousandth of a millimetre) for the simplest version of the idea. Other versions survive, and more data are in hand. The ideas that care most about cats are the ones that blame gravity.
🕰️Chapter 9
Penrose's clock
Lajos Diósi and Roger Penrose, working separately, suggested that gravity sets the clock. Every mass bends space and time a little, so a mass in two arrangements at once would bend it two ways at once, and nobody knows how to make sense of that. Penrose's guess: nature puts up with it only for a while. Heavier means sooner; farther apart means sooner.
Underground detectors have ruled out the simplest version, the one with nothing left to adjust. Versions with one adjustable size survive, so "Penrose has been proved wrong" goes too far.
For the crystal, the clock counts mass × distance², just like the eavesdropping. By our rough estimate it reads 3 to 70 million years. The cat lasted 10 millionths of a second. Gravity never got a turn.
Pick an object and slide its split. Watch for the only one whose gold band lands before its violet flag 👇
Nothing made so far comes near Penrose's clock. Vienna's clusters: 80 to 2,100 years, against 12 thousandths of a second. A dust speck 10 micrometres wide, split by its own width, would be forced to pick one place within 0.4 to 10 millionths of a second, by coincidence about as long as the crystal cat lasted; nobody has made one. A real test needs mass and distance.
🏀Chapter 10
Gravity's quantum ladder
Gravity already shapes quantum waves at the light end of the scale. Take neutrons slowed to a crawl, a few metres per second: slow enough to bounce off a polished glass mirror.
Above such a mirror, quantum physics lets a neutron bounce only to certain heights, like the rungs of a ladder. The lowest rung reaches 13.7 micrometres, less than the thickness of even a fine human hair, and no neutron can bounce any lower. The rungs aren't evenly spaced. A team in Grenoble, France, saw the steps in 2002.
Pick a rung above the first, then shake the mirror until the neutrons jump. Then try the Moon 👇
Each jump has its own sharp note: shake the mirror at just the right frequency and neutrons get kicked up a rung. On the Moon, weaker gravity makes taller rungs and lower notes. A team from TU Wien uses these notes to measure gravity and to hunt for hidden forces that some dark-energy and dark-matter ideas predict.
Is this quantum gravity? No. The neutron is quantum, but the gravity is the ordinary pull that drops an apple.
🤝Chapter 11
Meeting in the middle
Physics has a natural unit of mass, built from the constants of quantum physics, light and gravity: the Planck mass, about 22 micrograms. It's a unit, not a wall: nothing known says quantum physics changes there.
But two races meet near it. The heaviest cat is about three quarters of a Planck mass. From the other side, the lightest object whose own gravity has been measured (as far as we know, as of 24 October 2026) is a 90-milligram gold ball, in Vienna in 2021: 5,600 times the cat.
A dream experiment, proposed in 2017, would join them: put two specks of diamond each in two places at once, a quarter of a millimetre apart, and let them fall side by side for about 2.5 seconds, touching only through gravity. If they come out entangled, linked in the quantum way, that would be strong evidence that gravity itself is quantum.
How strong that evidence would be is still argued: in June 2025 two physicists showed that even Penrose's kind of model, where gravity is not quantum, can make such links at short range; in May 2026 two of the proposers and a colleague replied that the test still works. In October 2025 two other physicists argued that even ordinary, non-quantum gravity can link quantum objects, though in a different pattern, so the test must check the pattern, not only the link; that claim is disputed too.
And the twist: by our rough estimate, Penrose's clock would end each diamond's double state in 0.5 to 12 thousandths of a second, long before the 2.5 seconds are up. So the same experiment, not yet done, would test Penrose too.
🔭Chapter 12
Bigger cats
Bigger cats are on their way. As of 24 October 2026:
🔦Floating glass beads, held by laser light in a vacuum. In August 2025 a team let one bead's quantum blur grow more than three times wider: still far smaller than the bead; matching the bead's size is the goal.
⚛️Heavier clusters. Vienna aims for clusters of millions of atomic mass units (one unit is about the mass of a hydrogen atom; the 2026 clusters were about 172,000), and an upright machine that could gain about 100 times in mass and in time.
🧲New ideas, like a July 2026 proposal for superconducting specks heavier than a picogram, floating in magnetic traps.
Nobody has yet claimed that gravity linked two objects in the quantum way. Let's add it up. 🧾
🧾 One cat, itemised
Effective masscounted by the average wiggle16 µg
Same cat, counted differentlyby the biggest wiggle1 µg
Atoms humming alongroughly1017
Gap between its two statesin proton widths1/800
Stripes lastedETH, 2023~10 µs
Penrose's clockour rough estimate3–70 million yr
Share of a Planck massa unit, not a wall0.74
Heavier cats sinceas far as we could find, as of 24 October 20260
heavy is easy ✦ far is hard ✦ gravity hasn't had its turn
In a fridge colder than deep space, a sliver of sapphire rang two opposite ways at once.
Its two ways of ringing were closer together than a proton is wide.
For about 10 millionths of a second, the world didn't quite find out which.
Then it did, the way it always does, and the stripes faded.
Gravity, if Penrose is right, would have noticed too. In millions of years.
The heaviest cat so far was split by 1/800 of a proton. Heavy is easy. Far is hard.
Nº 10 · ∫ Full version
Sixteen micrograms
In April 2023 a team at ETH Zurich put a vibration of a sapphire crystal into a Schrödinger cat state: the same sound wave ringing two opposite ways at once. The vibration had an effective mass of sixteen micrograms, about three quarters of a Planck mass, and, as far as we can find, no heavier cat state of motion has been reported since. Yet its two states were only 2.1 × 10−18 m apart, about one eight-hundredth of a proton's diameter, and their quantum fingerprint faded in about ten microseconds. That is not a weakness of the experiment. It is the physics. The same state can honestly be called one microgram split four times farther apart, because only mass times distance squared is fixed, and that product is what destroys cats: the environment's eavesdropping grows with it, and so does the collapse that Roger Penrose suggested gravity itself might cause. For this cat, on this page's estimate, Penrose's clock would read three to seventy million years. Heavy turns out to be easy. Far is hard.
This page explains what a cat state is and how to picture one, how ETH made a cat out of sound and read it with a superconducting qubit, what "effective mass" means and why "sixteen micrograms" is a choice of ruler, why big cats die young, how the crystal compares with the matter-wave record of January 2026, how collapse models are tested with a dark-matter detector, what Penrose's gravitational clock says about every superposition made so far, how neutrons sit on gravity's quantum ladder, and which proposed experiment would finally put gravity itself to the test.
This is the ∫ Full version, with the equations, caveats and sources. New to the idea? Start with the ✨ Simple version.
Numbers marked "this page's arithmetic" or "this page's estimate" were computed for this page from the cited inputs; they are not published results. Penrose's collapse times are given as ranges, because published conventions for the gravitational self-energy differ by a factor of up to about 25. "Effective mass" follows the paper: 16.2 µg is defined with the root-mean-square displacement of the vibrating atoms.
Records, limits and preprints are as of 24 October 2026.
Part IA cat made of sound
Chapter 1Sixteen micrograms
On 20 April 2023 a team at ETH Zurich (Marius Bild, Matteo Fadel, Yiwen Chu and colleagues) reported in Science that they had put a vibration of a sapphire crystal into a Schrödinger cat state.1 The vibration is sound: a standing wave near 6 GHz, trapped in a sliver of crystal about as wide as a hair. For about ten microseconds it rang two opposite ways at once. The paper's title calls the system "a 16-microgram mechanical oscillator". More precisely, the vibration has an effective mass of sixteen micrograms (16.2 µg), and about 1017 atoms take part in it, in the authors' estimate.
Three more numbers set the scene. The two states the crystal held at once differed by 2.1 × 10−18 m, about one eight-hundredth of a proton's diameter (this page's arithmetic, with the CODATA 2022 proton radius).2 The quantum fingerprint of the superposition lasted about 10 µs. And 16.2 µg is 0.74 of the Planck mass, the unit of mass built from ħ, c and G (this page's arithmetic). As of 24 October 2026 we found no heavier cat state of motion reported anywhere.
The page follows three twists. First, "sixteen micrograms" is a choice of ruler: the same state can honestly be given a different mass, and only one combination of mass and distance is fixed (Chapter 5). Second, the distance, not the mass, is the hard part, and the reason is the same combination (Chapters 6 to 8). Third, Roger Penrose proposed that gravity itself ends superpositions, and his proposal counts that combination too; for this cat his clock reads millions of years (Chapter 10). The two frontiers, quantum objects getting heavier and sources of gravity getting lighter, meet near the Planck mass (Chapter 12).
Chapter 2A quite ridiculous case
In late 1935 Erwin Schrödinger published a long essay in three parts, "Die gegenwärtige Situation in der Quantenmechanik" ("The present situation in quantum mechanics").3 In its fifth section he introduced a cat. In John Trimmer's 1980 translation the passage opens: "One can even set up quite ridiculous cases."4 A cat is shut in a steel chamber with a Geiger counter and a tiny bit of radioactive substance, so little that in the course of an hour perhaps one atom decays, and with equal probability perhaps none. A decay sets off a hammer that shatters a flask of hydrocyanic acid. After an hour, the wavefunction of the whole system would contain the living and the dead cat "mixed or smeared out in equal parts".
Schrödinger meant this as an absurdity. His point was that an indefiniteness that seems harmless while it is confined to an atom can be passed, by an ordinary chain of cause and effect, to something as large as a cat, where it plainly makes no sense. He was not claiming that cats are in superpositions; he was saying that the theory's description could not simply be read as a picture of reality.
A superposition is not "secretly one or the other, we just don't know which". It is a state that contains both possibilities together with a definite relation between them, a phase, and that relation has consequences: it makes the two possibilities interfere, like two overlapping sets of waves. Interference is what tells a superposition apart from a mere coin toss, which is why every superposition experiment on this page is an interference experiment of one kind or another.
Two landmark laboratory "cats" came in 1996. At NIST, Christopher Monroe, David Wineland and colleagues put a single trapped atom into a superposition of two separated positions.5 In Paris, Serge Haroche's group made a superposition of two phases of a weak microwave field in a cavity and watched it progressively lose its quantum character as it leaked information to its surroundings.6 Since then, "cat state" has become a working term: a superposition of two states that are clearly distinguishable. For a vibrating object, the natural choice is a superposition of two coherent states:
|cat⟩ ∝ |α⟩ ± |−α⟩|α⟩ is a coherent state: the quantum version of a definite oscillation with complex amplitude α, blurred only by the zero-point motion that even the ground state has. |α|² is its mean number of quanta. |−α⟩ is the same oscillation in the opposite phase. The + sign gives an "even" cat, the − sign an "odd" one.
The ETH cat is exactly this: one vibration of the crystal, in two opposite phases at once. "Clearly distinguishable" has a precise meaning here. The two oscillations must differ by more than their own quantum blur, so that a single measurement could, in principle, tell them apart.1
Chapter 3A portrait of two states at once
To see a cat state you need a map with two directions: where the vibrating thing is (position, horizontally) and how fast it is moving (momentum, vertically). Physicists call it phase space. Nº 2 pictured a state as a single dot in an imaginary map with one axis per quantity. For a classical oscillator the dot circles the origin once per vibration. In quantum mechanics the uncertainty principle forbids a dot: the calmest possible state, the ground state, is a round smudge as wide as the zero-point motion (squeezing can narrow it one way only by widening it the other), and a cat is two smudges with stripes between them.
The map is the Wigner functionW, introduced by Eugene Wigner in 1932.7 It behaves almost like a probability distribution over phase space: adding it up along the momentum direction gives the probability of each position, and adding it up along the position direction gives the probability of each momentum. A coherent state is a single round hill. A cat state of the kind ETH made has the form
W(β) = [e−2|β−α|² + e−2|β+α|² ± 2e−2|β|²cos(4α Im β)] / [π(1 ± e−2α²)]For real α. β is a point of phase space: Re β measures position and Im β momentum, in the oscillator's natural units; the ground state is a round hill of height 2/π. Bild et al. 2023, supplement, eq. S33, at the moment the cat is made.
The first two terms are two hills, at +α and −α: the two oscillations. The third term is the interference between them, a set of stripes across the middle of the map. Its cosine swings below zero. A probability can never be negative, so no mixture of ordinary oscillations, no classical uncertainty about which way the crystal is ringing, can produce those negative stripes. They are the fingerprint of a genuine superposition, and the quantity ETH measured.1,8 The stripes have a period of π/(2α) along the momentum direction, so bigger cats have finer stripes.
Figure 1 draws this map for the ETH cat. Grow the cat from nothing to α = 3, switch between the even and odd cat, then press Play: the cat loses energy at the crystal's measured rate. Before you do, guess which fades first, the hills or the stripes.
Figure 1🗺️ Try it
A portrait of two states at once
Grow the cat, then let it fade
α, the size of each of the two vibrations; the mean number of phonons is about α².
Which fades first?
Average phononsQuanta of sound, on average
Stripes left
Deepest dip below zero
Split, in the real crystal
Stripes left, e−2α²(1−η²)Energy left, η²
The Wigner function of an ideal cat state |α⟩ ± |−α⟩ of one vibration mode, losing energy at the measured rate T1 = 84 µs (Bild et al. 2023): W(β) = [e−2|β−ηα|² + e−2|β+ηα|² ± 2e−2|β|²e−2α²(1−η²)cos(4ηα Im β)] / [π(1 ± e−2α²)], η = e−t/2T1 (their supplement, eq. S33), normalised so the ground state peaks at 2/π. Horizontal: position (Re β); vertical: momentum (Im β), on equal scales. Brass is positive, violet negative; the strip is the slice along the dashed line. The interference term fades 2α² times faster than the energy; under pure energy loss any negativity is gone once half the energy has leaked out (t = T1 ln 2 ≈ 58 µs). The split converts α into the crystal's displacement with the paper's rms definition, 2√(2(1 + 2α²)) xzpf, xzpf = 2.95 × 10−19 m for the 16.2 µg effective mass at 5.96 GHz (this page's arithmetic). The real states had 66% fidelity to an ideal cat and extra dephasing, so their negativity faded in about 10 µs, a little faster than this ideal model (whose negative volume falls to 1/e in about 14 µs at α = 1.61).A map of the crystal's vibration: left to right is how far the atoms have swung, up and down is how fast they move. Two hills mean two opposite vibrations at once. The violet stripes between them dip below zero, and only a true "both at once" can do that; the strip beside the map is a slice through the middle. Make the cat bigger and watch the stripes get finer; then press play and see how much faster the stripes fade than the hills.
The stripes go first, and fast. While the hills have barely drifted towards the centre, the interference term is gone. In the model, the stripes fade 2α² times faster than the energy leaks away: about five times faster for the biggest ETH cat, and the bigger the cat, the bigger the factor. Chapter 7 explains why. Two other things are worth noticing. At α = 0 the even cat is just the ground state, one hill; the odd cat is a single phonon, a ring whose centre dips below zero, so even one quantum of sound is a state no classical vibration can imitate. And the real states were not ideal: their fidelity to an ideal cat was 66%, with extra loss of phase, so their negativity faded a little faster than in this model.1
Chapter 4A cat made of sound
The device is a sandwich of two sapphire chips. One carries a thin disc of aluminium nitride, a piezoelectric material that turns an oscillating electric field into a mechanical strain and back. It is flip-chip bonded face to face over a second chip that carries a superconducting transmon qubit.1,9 The qubit's microwave field squeezes the disc, the disc launches sound into the sapphire, and the sound bounces between the chip's two faces as standing waves, a ladder of overtones about 12 MHz apart. The qubit is tuned into resonance with one of them, near 6 GHz.
That one mode is a standing wave about 500 half-wavelengths long across the 435 µm thickness of the chip, and confined sideways to a Gaussian beam with a waist of 27 µm. It fills a sliver about 54 µm wide, roughly the width of a hair, with a volume of about 0.001 mm³ (this page's arithmetic for the width and volume). One quantum of sound in it, one phonon, carries hf ≈ 25 µeV, about 0.29 K in temperature units (this page's arithmetic). The experiment runs at a small fraction of that, far colder than the 2.7 K of deep space, so the mode starts in its quantum ground state.
The recipe has three steps.1 First, a microwave pulse displaces the mode into a coherent state with α = 1.75. Second, the qubit is put into a superposition of its two states. Third, qubit and sound are left to exchange energy resonantly. Because the exchange runs at a different rate for each phonon number, the qubit's oscillation washes out after about 0.9 µs and comes back at about 6.7 µs. In between, at about 2.9 µs, the qubit almost disentangles from the sound and leaves the mode in a superposition of two coherent states turning in opposite directions. That is the cat.
Reading it out uses the same qubit. In this device the qubit's frequency depends on the number of phonons, so a short sequence of qubit pulses can ask a single question: is the number of phonons even or odd?10 The average answer, after the state has been shifted by a chosen amount in phase space, gives the Wigner function at one point. Repeated thousands of times over a grid of shifts, it rebuilds the whole portrait, negative stripes included. The team made cats of three sizes, which the paper labels D = 1.09, 1.43 and 1.61, where D² is the mean number of phonons: 2.6 for the largest. The measured states matched the state expected from the protocol with 76% fidelity, and an ideal two-component cat with 66%.1
The platform has a short lineage. In 2010 a team at the University of California, Santa Barbara, with Andrew Cleland and John Martinis as senior authors, put a human-made mechanical resonator into its quantum ground state and controlled it one phonon at a time.11 In 2017 Chu and colleagues coupled a qubit to bulk sound in a crystal, the design ETH uses.9 The parity readout followed in 2022,10 and in 2024 the same ETH group turned a crystal vibration into a qubit of its own.12 The deeper ancestry is the superconducting circuit itself. The 2025 Nobel Prize in Physics went to John Clarke, Michel Devoret and Martinis for experiments in 1984 and 1985 showing that an electrical circuit built from superconductors, far larger than any atom, could tunnel through a barrier and absorb energy only in discrete amounts, as a single quantum object would.13 The ETH cat is made and read with a descendant of that circuit.
Chapter 5Which sixteen micrograms?
What, exactly, has a mass of sixteen micrograms? Not the chip, which is far heavier. Not a piece of crystal moving as one body either. In a standing wave, neighbouring half-wavelength slabs of crystal move in opposite directions; the amplitude is largest on the axis of the beam and falls off sideways like a Gaussian; and the centre of mass of the crystal hardly moves at all. Every atom in the sliver moves a different amount.
To compare such a mode with the textbook picture of a mass on a spring, you have to choose a reference displacement xeff, then define the effective mass Meff so that the energy comes out right:
E = ½ Meff ω² xeff² ⇒ Meffxeff² = 2E/ω²The energy E and the angular frequency ω are fixed by the physics. How the product is split between a mass and a displacement is a convention.
The paper's supplement gives two choices.1 Take xeff as the root-mean-square displacement of the atoms in the mode and the effective mass is 16.2 µg; the two states of the largest cat then differ by 2.1 × 10−18 m. Take xeff as the maximum displacement, on the beam axis, and the effective mass is 1.0 µg, with the two states 8.4 × 10−18 m apart. The naive mass of the mode's cylinder, density × πw0² × length, is 4.0 µg, in between. Both definitions are honest; the analysis of the same platform by Schrinski and colleagues used the 1.0 µg one.14 What they agree on is the product: 16.2 µg × (2.1 × 10−18 m)² = 1.0 µg × (8.4 × 10−18 m)² = 7.1 × 10−44 kg m² (this page's arithmetic).
Figure 2 draws a few of the sliver's half-waves frozen at full swing, every dot (a parcel of atoms) drawn twice, once for each branch of the cat. Pick a ruler, or drag the handle along the line, and watch the mass and the split trade places.
Figure 2⚖️ Try it
Which sixteen micrograms?
Pick a ruler
Effective mass
Split between the two statesDistance between the two states
As a slice of a proton
Mass × split²Mass × distance²
A standing longitudinal wave in the sapphire, u ∝ cos(mπz/L) e−r²/w₀², with waist w₀ = 27 µm through the L = 435 µm chip (Bild et al. 2023, supplement). Only a few of the roughly 500 half-wavelengths are drawn; each dot stands for a parcel of atoms and is drawn in both branches of the cat; the displacement is exaggerated about ten billion times relative to the drawing's scale along the beam, and the beam is drawn far narrower than it is. Because the mode is not a centre-of-mass motion, its mass is defined only together with a reference amplitude through ½Meffω²xeff² = E: the rms displacement gives 16.2 µg and a split of 2.1 × 10−18 m, the maximum displacement 1.0 µg and 8.4 × 10−18 m. The chart interpolates between them on logarithmic axes; Meffd² = 7.1 × 10−44 kg m² either way (this page's arithmetic). The paper estimates that a half-wavelength slab, about 30 ng, approximates a centre-of-mass mode; it gives no split for it. Proton fractions use the CODATA 2022 radius, 0.84075 fm.The sliver of crystal, ringing two opposite ways at once: every dot (a little bunch of atoms) is drawn twice, once for each way. Most of it moves a little and the middle moves most, so its "weight" depends on where you hold the ruler. Pick a way of counting, or drag the dot along the line: the mass and the distance trade places, but mass × distance² never changes.
The "weight" changes sixteen-fold, the split four-fold, and mass × split² not at all. That is more than a curiosity. Anything that depends on the energy of the motion, or on the mass-weighted squared displacement of the atoms, gives the same answer on either ruler: decoherence by most mechanisms (Chapter 7) and Penrose's gravitational collapse for smooth matter (Chapter 10). The physics of this page does not depend on the definition, even though its headline does.
The paper also offers a third, more physical unit. A single half-wavelength slab, the authors write, "approximates a center-of-mass mode", and they estimate its mass at about 30 ng; they call it "by far the most massive object that has been placed into a cat state". That is the authors' claim, and a reasonable one, but it uses a different object from the 16.2 µg of the title. And none of it was seen. The chip is visible to the eye; the mode is a 0.001 mm³ sliver inside it, and the superposition was inferred from thousands of qubit measurements. Headlines that called the cat visible to the naked eye were describing the chip. ETH's own press release compared the 16 micrograms to a fine grain of sand: a comparison of masses, not a picture of what moved.
Part IIHeavy, but barely apart
Chapter 6One eight-hundredth of a proton
How far is 2.1 × 10−18 m? The proton's root-mean-square charge radius is 0.84075 fm (CODATA 2022),2 so its diameter is about 1.68 × 10−15 m. The split is about 1/800 of that, and one fifty-millionth of a hydrogen atom (this page's arithmetic). On the 1.0 µg ruler it is 1/200 of a proton. Either way it is far smaller than a proton.
Small is not the same as meaningless. The relevant yardstick is the crystal's own quantum blur, its zero-point motion:
xzpf = √(ħ / 2Meffω) ≈ 2.95 × 10−19 m split = 2√(2(1 + 2D²)) xzpf ≈ 7.0 xzpf ≈ 2.1 × 10−18 mFor 16.2 µg at 5.96 GHz (the mode frequency stated for this geometry by Schrinski et al. 2023) and D = 1.61; the second line is the paper's measure of the split (supplement, eq. S29). This page's arithmetic.
The two branches are about seven times their own blur apart, so they are distinct in the sense that matters: a measurement of the displacement could, in principle, tell them apart. "Macroscopically distinct" in this field means distinct relative to quantum noise, not visible to the eye.
It also means the crystal never went anywhere. Freeze the motion at full swing and the atoms in the mode sit, in rms terms, about 2 × 10−18 m further "forward" in one branch than in the other; the crystal's centre of mass sits still. What is split is the collective coordinate of the mode, not any single atom: each atom's own zero-point jiggle, from all the crystal's other vibrations, is millions of times larger than the split. "A 16-microgram object in two places at once" is the wrong picture. "A 16-microgram vibration ringing two opposite ways at once" is the right one.
For scale, consider a far heavier object whose motion has been brought near its quantum ground state. In 2021 the LIGO collaboration cooled the differential motion of the four 40 kg mirrors of a gravitational-wave detector, a mode with an effective mass of 10 kg, to an average of 10.8 quanta, at a temperature of 77 nK.15 The zero-point motion of that mode is about 7.5 × 10−20 m, one twenty-two-thousandth of a proton (this page's arithmetic). LIGO's mode was near its ground state, never in a superposition, and it is not a cat. Quiet is achievable for heavy things. Two-at-once is much harder.
Chapter 7Why big cats die young
Why is the split so tiny? Because the world keeps asking which branch the crystal is in. Stray phonons, defects in the crystal, the qubit itself and any radiation that reaches the chip all interact with the vibration. Each interaction that could tell the two branches apart carries away a record of which one, even a record nobody reads, and each record weakens the interference. This is decoherence, an idea of Dieter Zeh's from 1970, developed by Wojciech Zurek in the early 1980s and worked out for scattering by Erich Joos and Zeh in 1985.8,16,17 For splits small compared with the wavelength of whatever is doing the probing, the rate grows with the split squared: twice the distance, four times faster.
For the crystal, the main culprit is the sound leaking away, with an energy lifetime T1 ≈ 84 µs. Each phonon that escapes is a small record of which way the crystal was ringing, and the paper's analysis gives
τcat ≈ T1 / (2α²)For large cats (Bild et al. 2023, supplement G). Because the split grows in proportion to α, this is the "split squared" law in another form.
The measured negativity of the D = 1.43 cat faded in about 10 µs; the paper's simulations give 24.7, 12.3 and 10.5 µs for the three sizes, and the bigger cats faded faster, as predicted.1 The 84 µs is how long the sound lasts, not how long the cat lasts. In Figure 1, press Play and watch it happen: the stripes vanish while the hills, which carry the energy, have hardly moved.
Now try to make the same crystal into a bigger cat. With the same T1 and the same law, a split of one proton diameter, 1.7 × 10−15 m, needs α ≈ 1,400, and the stripes would last about 2 × 10−11 s. A split of one atom's width, 10−10 m, would leave them about 6 × 10−21 s, from phonon loss alone (this page's arithmetic; illustrative). That is why every superposition record is a trade: an enormous mass at an absurdly small distance, as in the crystal, or a tiny mass far apart for a long time, as in the matter-wave experiments of the next chapter.
Decoherence explains why interference disappears, and why what is left behaves like a classical either-or. It does not say which of the two outcomes you will find, or why you find one at all. That is the measurement problem, and it is open: collapse models (Chapter 9) answer it one way, many-worlds and other interpretations another. One argument about whether empty space can fluctuate into anything at all (Nº 3) turns on the same idea: in the many-worlds picture its authors use, without something that records the difference, a quantum possibility never becomes an event.
Chapter 8Biggest by which ruler?
Is the heaviest cat also the biggest superposition? The main rival is matter-wave interferometry, which sends a beam of molecules or clusters through a series of gratings.18 An interference pattern appears downstream only if each particle passed through several slits at once, that is, if it was spread out over at least the grating period. The records are dated, and they move:
1999, Vienna: football-shaped C60 molecules, 60 carbon atoms each, through a grating with a 100 nm period.19
2015, Stanford: rubidium atoms whose wave packets were separated by 54 cm.20 Whether the interference proves a superposition of the two distant packets was disputed in a published comment, and the authors replied that it does.21
2019, Vienna: molecules heavier than 25 kDa, with up to about 2,000 atoms, in a 2-metre interferometer with gratings of 266 nm period.22
21 January 2026, Vienna: sodium clusters of more than 7,000 atoms on average (mean mass 172 kDa, about 8 nm across), flying at about 160 m/s through three gratings of ultraviolet light with a 133 nm period, spaced 0.983 m apart.23 The authors show that each cluster was delocalised over more than ten times its own diameter. The 133 nm is the grating period, not a measured distance between paths. The clusters spent about 12 ms in the interferometer (this page's arithmetic, 2 × 0.983 m ÷ 160 m/s). The journal title differs from the preprint's, which spoke of "nanoparticle Schrödinger cats".
Set the crystal beside the clusters. Its effective mass is 5.7 × 1013 clusters (this page's arithmetic). But the clusters' delocalisation, on the scale of the grating period, is about 6 × 1010 times larger than the crystal's split, and they kept it about a thousand times longer: 12 ms against 10 µs. Figure 3 places every superposition on one map, mass to the right and split upwards. Tap a point for its story, switch the crystal between its two rulers, turn on the band where Penrose's gravity would act within a second (Chapter 10), then switch to the second view, a single score explained below.
Figure 3🏆 Try it
Biggest by which ruler?
Switch the ruler
Selected
Mass
Split
Score μScore
Superpositions by mass and by the distance between their two branches, logarithmic axes, records as of 24 October 2026. The electron (single electrons building up an interference pattern, Tonomura et al. 1989) has no plotted split and sits on the strip at the bottom. For matter-wave interferometers the split is taken as the grating period (the scale over which each particle was delocalised; for the 2026 clusters the bar runs from ten times their 8 nm diameter to the 133 nm period); far-field set-ups spread further downstream. The crystal cat is drawn with either effective-mass definition (Figure 2). LIGO's 10 kg mode was cooled near its ground state, never put in a superposition; its marker sits at twice its zero-point motion. Hollow rings are not superpositions made in a laboratory: LIGO's cooled mode, proposals and a thought experiment. Shaded band: where a smooth uniform sphere of 3,000 kg/m³ would collapse within one second under the Diósi–Penrose model, between normalisations that differ by 8π (this page's estimate; a crystal mode's integral differs by a factor 3, invisible at this scale). Second view: macroscopicity μ (Nimmrichter and Hornberger 2013; Schrinski et al. 2023 for the crystal mode, a single-phonon state; Fein et al. 2019; Pedalino et al. 2026; the proposals from Nimmrichter and Hornberger 2013).Every solid dot is a real "both at once" experiment: farther right is heavier, higher means the two states were farther apart. Tap a dot for its story. The crystal is by far the heaviest, but its two states barely differ. Switch to the score to see which experiment tests quantum physics hardest: a different winner. Hollow rings are LIGO's quiet mirrors, proposals and Schrödinger's own cat, none of them a superposition made in a lab.
Among real superpositions, the crystal sits alone at the bottom right: by far the heaviest, by far the smallest split; only LIGO's hollow ring, a cooled mode that was never split, lies beyond it. The matter waves sit far up and to the left. Nothing real comes near the corner where Schrödinger's cat would be. Which point is "biggest" depends on how you weigh mass against distance and time.
Stefan Nimmrichter and Klaus Hornberger proposed one way to weigh them in 2013: macroscopicity, μ.24 Imagine the gentlest possible modification of quantum mechanics that would make large objects behave classically, characterised by how long it would let a single electron stay coherent, τe. Each experiment that sees interference rules out every modification strong enough to have spoiled it, and μ is the base-10 logarithm of the longest τe ruled out, in seconds. For an object smaller than the path separation, it takes a simple form:
μ ≈ log10[ (1/|ln f|) (M/me)² (t / 1 s) ]Nimmrichter and Hornberger 2013, eq. 8. M is the mass, t the coherence time, f the fraction of the expected interference visibility that was observed. Valid only when the separation exceeds the model's critical length, tens of nanometres to a micrometre. It reproduces 14.1 for the 2019 molecules and 15.2–15.7 for the 2026 clusters (this page's arithmetic; the published value is 15.5).
So μ rewards mass squared times time, but only when the separation is large enough to count in full. On this ruler the order changes.24,25,14,22,23 Two interfering sodium Bose–Einstein condensates (MIT, 1997) score 8.4. Fullerene molecules in 1999 scored 10.6. A bulk-acoustic crystal mode at ETH, the same kind of device but in a single-phonon state with a 1.0 µg effective mass, scores 11.3, "on par with state-of-the-art atom interferometers" in its authors' words. That is not the cat: we found no published μ for the cat state itself. The 2019 molecules score 14.1 and the 2026 clusters 15.5, the record. The crystal's atoms move far less than the critical length, so its mass is not squared in full. Proposals reach 19 to 23. Schrödinger's cat, as Nimmrichter and Hornberger idealise it (4 kg kept coherent across 10 cm for a second), would score about 57: some 41 orders of magnitude beyond the record.
A third family uses electrical circuits rather than moving matter. In 2000, groups at Stony Brook and Delft put superconducting loops into superpositions of currents circulating clockwise and anticlockwise at once,26 and cat states of microwave fields are now engineering components: in 2025 a logical memory was built from five "cat qubits".27 Heaviest, farthest and most macroscopic are three different titles, and as of 24 October 2026 they belong to three different experiments.
Part IIIDoes gravity kill cats?
Chapter 9A size limit for quantum mechanics?
Perhaps large things cannot stay in superpositions at all. Collapse models add a small random, nonlinear term to the Schrödinger equation: negligible for one particle, amplified for many, so that superpositions of large objects end by themselves. In the model proposed by Giancarlo Ghirardi, Alberto Rimini and Tullio Weber in 1986 (GRW), every nucleon is spontaneously localised to about 100 nm at random moments, at a rate λ ≈ 10−16 s−1.28 One nucleon would be hit about once every 300 million years; a body of 1023 nucleons about every 10−7 s (this page's arithmetic). A hit settles the outcome only if the branches are farther apart than that 100 nm; for smaller splits its effect shrinks with the split squared, which is why a split like the crystal's barely registers. Philip Pearle, and then Ghirardi, Pearle and Rimini, turned this into a continuous process, continuous spontaneous localisation (CSL), in 1989 and 1990.29,30,31
Collapse models are testable, and not only with cats. The random localisations jiggle every charged particle, and jiggling charges radiate. A collapse model therefore predicts a faint, steady glow of X-rays from ordinary matter. A detector built to be as quiet as possible, deep underground, can look for that glow without making any superposition at all.
The strongest such test so far came from a dark-matter detector. On 23 March 2026 the XENON collaboration published an analysis of low-energy events (1–140 keV) from the first science run of XENONnT, a liquid-xenon detector in the Gran Sasso underground laboratory in Italy, recorded between July and November 2021.32 For the Markovian (white-noise) version of CSL it set λ/rC² < 3.0 × 10−3 s−1 m−2 at 90% confidence, about two orders of magnitude beyond the previous best, from the Majorana Demonstrator in 2022.33 The values Ghirardi, Rimini and Weber originally proposed (λ = 10−16 s−1, rC = 10−7 m) are excluded at 9.1σ, which the authors describe as a first. Variants with coloured noise or dissipation are less constrained, and more XENONnT data are in hand.
So the strongest limits on collapse come from a detector looking for dark matter, not from cats. XENONnT's limit is the strongest for correlation lengths up to about 10 µm; at longer ones, quiet masses compete, among them the free-falling test masses of the LISA Pathfinder spacecraft, which a collapse model's random kicks would have made jitter.34 Cat experiments test the same models more directly, by keeping something coherent whatever it radiates, but the crystal's split is far too small to compete. The models that care most about cats are the ones that tie collapse to gravity.
Chapter 10Penrose's clock
Lajos Diósi in 1987 and 1989, and Roger Penrose, who first floated the idea in 1986 and made it precise in 1996, proposed that gravity sets the rate of collapse.35,36,37 Penrose's argument goes like this. Two branches of a superposition with different mass distributions come with two different curvatures of spacetime, and quantum mechanics has no clear way to superpose two spacetimes. He suggested that nature tolerates the mismatch only for a limited time, inversely proportional to the gravitational self-energy EG of the difference between the two mass distributions:
τ ≈ ħ / EG, EG = (G/2) ∬ Δρ(x) Δρ(y) / |x − y| d³x d³yΔρ is the difference of the two branches' mass densities. Normalisations differ: Diósi's convention, which XENONnT uses and which reproduces the numbers of Donadi et al. 2021, gives an EG 8π times larger than Penrose's (as the XENONnT 2026 supplement notes). This page brackets every collapse time between τ and τ/8π, a factor of about 25, and calls the result an estimate.
For point-like nuclei EG would be infinite, so each nucleus has to be smeared over some size R0. Penrose's natural choice was the spread of each nucleus's own position in the crystal, about 0.05 Å in cold germanium: the "parameter-free" version. In a paper published in September 2020, Sandro Donadi and colleagues searched data from a germanium detector in the Gran Sasso laboratory for the radiation this version predicts and found none, setting R0 > 0.54 Å and excluding it.38 Germanium data from the Majorana Demonstrator raised the bound to 2.5 Å (95% C.L.; published in 2022, corrected in 2023), and in March 2026 XENONnT pushed it to R0 > 4.9 Å (90% C.L.; 4.5 Å at 95%), eight to nine times Donadi's value.32,33 From the other side, if R0 were too large the model would fail to collapse everyday objects; Figurato and colleagues placed that limit near 10−4 m on an admittedly rough criterion.39
The fair summary is this: the simplest, parameter-free version of Penrose's idea is ruled out; versions with a free size survive, squeezed between underground detectors and the requirement that cats do collapse. Donadi and colleagues said as much themselves, and whether the excluded version is the one Penrose and Stuart Hameroff use in Orch OR, their speculative theory of consciousness, has been disputed in a preprint.40 "Penrose is ruled out" overstates the case.
For an object of uniform density the integral can be done in closed form:
EG = (Gm²/R)(2δ² − 3δ³/2 + δ⁵/5) for δ = d/2R ≤ 1 EG = (Gm²/R)(6/5 − 1/(2δ)) for δ ≥ 1 crystal mode, smooth density: EG ≈ 2πGρMeffd²A sphere of mass m and radius R displaced by d, in the normalisation above. For small d, EG ≈ (2π/3)Gρmd²: like decoherence, it grows with the split squared. The crystal line (this page's derivation) holds for an R0 above the 4.9 Å bound and well below about 0.3 µm, the 1.7 µm acoustic wavelength divided by 2π (wider smearing averages away the wave's density ripple); it depends only on Meffd², so on neither choice of ruler. Here d is the 1.9 × 10−18 m between the two branches' centres at full swing (the paper's 2.1 × 10−18 m also counts the zero-point motion both branches share), and because that difference swings with the sound, EG averaged over a vibration is half of 2πGρMeffd².
Figure 4 sets Penrose's clock against how long each superposition actually lasted. Pick an object and slide its split; the brass band is the collapse time, the violet flag the measured lifetime.
Figure 4🕰️ Try it
Penrose's clock
Pick an object, split it further
Smearing length R₀:How blurred is each atom's mass?
Penrose's clock (this page's estimate)
It actually lasted
Verdict
Diósi–Penrose collapse times τ = ħ/EG (this page's estimate). Uniform spheres use Penrose's formula for the self-energy of the difference of the two mass distributions; the crystal mode uses the smooth-density result EG = 2πGρMeffd², which depends only on Meffd² (Chapter 5), halved because the split swings with the sound and taken with d = 1.9 × 10−18 m, the distance between the two branches' centres (the slider shows the paper's measure, which also counts zero-point motion). The brass band spans published normalisations that differ by up to 8π ≈ 25; the violet flag marks how long the superposition lasted (dashed: planned). Valid for a smearing length R0 above the 4.9 Å bound of XENONnT (2026) and below the object's size (for the crystal mode, well below about 0.3 µm, its acoustic wavelength divided by 2π); Penrose's parameter-free choice (R0 ≈ 0.05 Å, the zero-point spread of the nuclei in germanium) is excluded (Donadi et al. 2021) and would give the crystal 470–12,000 years, still far too slow. Lifetimes: crystal negativity about 10 µs (Bild et al. 2023); clusters about 12 ms in the interferometer (this page's arithmetic from the 0.983 m grating spacing and 160 m/s, Pedalino et al. 2026); the diamond test's planned 2.5 s (Bose et al. 2017). Schrödinger's cat has no flag: its hour is a story, not a measurement. Densities assumed: dust speck 2,000 kg/m³, diamond 3,500 kg/m³, sodium cluster and cat about 1,000 kg/m³, sapphire 3,980 kg/m³. The cluster's split uses the 133 nm grating period as its scale; once a split exceeds an object's diameter (8 nm for the clusters), splitting it further gives almost the same time. The R0 chips (crystal only) smear each nucleus, or at 10−15 m each nucleon, into a uniform sphere of radius R0; for splits much smaller than R0 this multiplies EG by (R*/R0)³, with R* ≈ 0.9 Å for sapphire's nuclei and 0.32 Å for a nucleon (this page's estimate).Roger Penrose suggests that gravity can't put up with a mass being in two arrangements for long: the heavier it is and the farther apart, the sooner it must pick one. The gold band shows when, for each object (our rough estimate). The violet flag shows how long the real superposition lasted. Slide the split and watch the clock move. Only the proposed diamond test gets there in time. The blur buttons (crystal only) try versions of the idea that are already ruled out: even they leave the clock far too slow at the real split.
The verdicts, all this page's estimate:
The crystal cat: about 3–70 million years, against about 10 µs measured. Penrose's clock is more than a billion billion times too slow to have mattered. Even the excluded parameter-free smearing (R0 ≈ 0.05 Å, the germanium value) would give 470–12,000 years, and a smearing of about 10−15 m, the size of a nucleon, excluded long ago,34,41 would still only bring it down to between a second and a minute (at that scale the smeared unit is each nucleon, not each whole nucleus). Matteo Fadel, one of the experiment's authors, has used the cat's measured fading to test the model directly: it requires only R0 above about 10−17 m, far weaker than the underground bounds.62
The 2026 sodium clusters: 80–2,100 years, against about 12 ms in the interferometer. Any split well beyond their 8 nm diameter gives almost the same time: once the two copies no longer overlap, separating them further barely changes EG.
A 10 µm dust speck (density 2,000 kg/m³) split by its own diameter: 0.4–10 µs, by coincidence about the time the crystal cat actually survived. Nobody has made such a superposition.
Schrödinger's cat, 4 kg split by 10 cm: 1.2 × 10−27 to 3 × 10−26 s. That is the model's point: in this picture large superpositions end almost at once.
No superposition made so far comes near Penrose's clock. The heaviest cat is no test of gravitational collapse, because the clock counts mass × split², and the crystal has mass without split. A test needs both. One proposed experiment has them (Chapter 12).
Chapter 11Gravity's quantum ladder
Gravity already acts on quantum waves at the other end of the mass scale. In 1975 Roberto Colella, Albert Overhauser and Samuel Werner tilted a neutron interferometer so that its two paths ran at different heights, and saw Earth's gravity shift the interference.42 The two paths of a single neutron felt different gravitational potentials, and the neutron noticed.
A cleaner case is a neutron sitting in gravity. Ultracold neutrons move so slowly, a few metres per second, that a polished glass mirror reflects them. Above a horizontal mirror a neutron is in a simple well: gravity pulls it down, the mirror stops it. Quantum mechanics allows only certain energies:
En = anmngz0, z0 = (ħ² / 2mn²g)1/3 ≈ 5.87 µman = 2.338, 4.088, 5.521, … are the zeros of the Airy function Ai(−x), and the wavefunctions are Airy functions. anz0 is the height a classical neutron of that energy would reach.
On Earth that gives 1.41, 2.46 and 3.32 peV for the first three levels, with classical turning heights of 13.7, 24.0 and 32.4 µm (this page's arithmetic, which reproduces the published values).43 The first rung is lower than even a fine human hair is thick. Its energy, 1.41 peV, corresponds to 16 nK in temperature units, and a classical neutron bouncing that high would leave the mirror at 1.6 cm/s. The rungs are not evenly spaced. Valery Nesvizhevsky and colleagues saw them at the Institut Laue–Langevin in Grenoble in 2002: neutrons passing through a narrow gap between the mirror and an absorber above it got through not smoothly but in steps, as the gap grew.43,44
Figure 5 draws the six lowest rungs above the mirror and the frequencies that connect them. Pick a rung, then shake the mirror and look for the frequency that lifts neutrons out of the lowest one. Then try the Moon.
Figure 5🏀 Try it
Gravity's quantum ladder
Shake the mirror
Height of this rung
Energy
Jump from rung 1
Kicked up
Stationary states of an ultracold neutron above a horizontal mirror: V = mngz for z > 0, a hard wall at z = 0, ψn ∝ Ai(z/z₀ − an), z₀ = (ħ²/2mn²g)1/3 = 5.87 µm on Earth. Energies 1.407, 2.460, 3.321, 4.083, 4.780, 5.428 peV; dashed lines are the classical turning heights anz₀ (13.7 to 53.0 µm) (this page's arithmetic, matching Nesvizhevsky et al. 2002 and qBounce). The brass cloud is where the neutrons are; the violet outline is |ψn|² for the chosen rung. The strip shows the share of neutrons left in the lowest state after a drive with Rabi line shapes, a 20 ms interaction and full transfer on resonance (illustrative widths and depths); f1n = (En − E1)/h = 254.6, 463.0, 647.2, 815.6 and 972.5 Hz at g = 9.80665 m/s². qBounce measured the 1→6 transition at 972.81(12) Hz in 2021 (conference proceedings), implying a g 3.9σ above the local value; less precise repeat runs in 2023 agreed with the local value, and the next transitions up, 1→7 and 2→9 near 1,120 and 1,142 Hz (beyond this strip), first measured in 2024, gave a g about 2σ below it (Lachaume 2026, TU Wien thesis). Moon (1.62 m/s²) and Mars (3.71 m/s²): the same physics with their surface gravity; heights scale as g−1/3, energies and frequencies as g2/3. The neutron is a quantum wave in classical Newtonian gravity; this is not quantum gravity.Very slow neutrons bounce above a mirror, but only to certain heights, like the rungs of a ladder. Pick a rung to see how high it reaches. Then shake the mirror: at just the right frequency, neutrons jump up a rung, and the dips in the strip show which notes work. Try the Moon: weaker gravity, taller rungs.
The qBounce collaboration of TU Wien, working at the same reactor, turned this into a measuring tool. Shake the mirror at exactly the frequency of a transition, (En − E1)/h, and neutrons are kicked up a rung; an absorber removes them, and the transmitted beam dips. They call it gravity resonance spectroscopy.45 The transitions from the lowest rung lie at 254.6, 463.0, 647.2, 815.6 and 972.5 Hz for standard gravity (this page's arithmetic). The method has set limits on hypothetical short-range forces from some dark-energy and dark-matter models.46 In 2021 data, the 1→6 transition came out at 972.81(12) Hz; the value of g it implies is 3.9σ above the locally measured one.47 Less precise repeat runs in 2023 agreed with the local value, and in 2024 the team measured the next transitions up, 1→7 and 2→9, near 1,120 and 1,142 Hz, the highest so far, with a g about 2σ below it.63 These results are in conference proceedings and a 2026 doctoral thesis, not yet a journal paper.
What this is not: quantum gravity. The neutron is a quantum wave, but the gravity it sits in is the ordinary Newtonian field of the Earth, an external potential like the field between the plates of a capacitor. Nothing about gravity is quantised by this experiment, and the neutron is not a cat. It is the cleanest place where gravity shapes a quantum wave, at the light end of the scale.
Chapter 12Meeting near the Planck mass
The Planck mass is mP = √(ħc/G) = 21.76 µg (CODATA 2022).2 It is roughly the mass at which an object's quantum length, its Compton wavelength, becomes comparable to its gravitational length, the radius of a black hole of that mass. It is a natural unit, not a known threshold: no established theory says that quantum mechanics changes at the Planck mass.
Still, it is where the two frontiers meet. On the quantum side, the crystal cat is 0.74 Planck masses (0.046 on the 1.0 µg ruler; this page's arithmetic). On the gravity side, the lightest object whose own gravitational pull has been measured, as far as we know as of 24 October 2026, is a 90 mg gold sphere, in a 2021 experiment in Vienna.48 That is about 4,100 Planck masses and 5,600 times the cat's effective mass (this page's arithmetic). Gravity has also been measured acting on a levitated magnet of less than half a milligram, but there the source was a set of kilogram masses; the tiny particle was the probe.49 The heaviest superposition sits just below the Planck mass; the lightest measured source of gravity sits a few thousand times above it.
The experiment that would join the two was proposed in two companion papers published on 13 December 2017, by Sougato Bose and colleagues and by Chiara Marletto and Vlatko Vedral.50,51 Two diamonds of 10−14 kg, each carrying a spin, are each put into a superposition of two positions 250 µm apart, and fall side by side for about 2.5 s, interacting only through gravity. If they come out entangled, the argument runs, gravity must be able to carry quantum information, which a classical field cannot do. Seeing that entanglement would be strong evidence that gravity is quantum.
How strong is disputed. In June 2025 David Trillo and Miguel Navascués found that the Diósi–Penrose model, in which gravity stays classical, itself predicts gravitationally induced entanglement at short range, and argued that seeing entanglement would therefore not by itself prove gravity quantum.52 In May 2026 Tianfeng Feng, Vedral and Marletto replied that collapse-based models do not violate the entanglement witness, because of their nonlocal features.53 In October 2025 Joseph Aziz and Richard Howl raised a second challenge in Nature: describing the masses with full quantum field theory rather than as simple particles, they found that even classical gravity can entangle them through local processes, though with a different scaling from quantum gravity, so a convincing test must check how the entanglement grows, not only that it appears. Marletto, Vedral and colleagues dispute that conclusion too, as does Lajos Diósi, in preprints.60 The argument continues.
There is a further twist. On this page's estimate, Diósi–Penrose collapse would end each diamond's superposition in 0.5–12 ms, some 200 to 5,000 times sooner than the 2.5 s the experiment needs. If Penrose's idea is right in this form, the diamonds' superpositions would end long before the fall does. So the same experiment would test Penrose as well as quantum gravity. In Figure 4, the diamond test is the only object whose brass band lands before its violet flag.
Part IVWhat comes next
Chapter 13Bigger cats
Several routes lead towards bigger cats, and each fights the split-squared law in its own way.
Levitated nanoparticles. A glass nanosphere held by a laser in vacuum has no crystal mount to leak its motion into. In 2020 one was cooled to its motional ground state,54 and in 2021 two groups achieved quantum control of such particles, one in cryogenic free space and one at room temperature.55,56 In August 2025 Massimiliano Rossi and colleagues softened the trap and let a nanosphere's wavefunction spread to more than three times its initial coherence length.57 That is still far smaller than the particle itself; the goal is a coherence length comparable to the object's size.
Heavier matter waves. The 2026 paper already shows fringes from clusters of 0.4 to 1 million daltons, but at those masses the set-up cannot yet tell a quantum pattern from a classical shadow; slowing the clusters to about 25 m/s should. The Vienna group names clusters of millions of daltons as its next step, and a vertical interferometer that could gain about a hundred times in both mass and time, which on the μ ruler would be six orders of magnitude.23,58
Longer-lived crystal cats. Because τcat ≈ T1/2α², every gain in the phonon lifetime buys a bigger or longer-lived cat directly.
New proposals. In July 2026 a theory preprint proposed interference of superconducting microparticles above a picogram, levitated in shaped magnetic traps.59 It is a proposal, not an experiment.
Collapse limits. XENONnT has more data than its first science run, so the limits on CSL and on R0 are expected to tighten.32
As of 24 October 2026, no experiment has claimed gravitationally induced entanglement, and we found no cat state of motion heavier than ETH's. The heaviest cat ever made was split by an eight-hundredth of a proton, and that was the point. Heavy is easy. Far is hard. Gravity has not yet had its turn.
Chapter 14Glossary and sources
Superposition
A quantum state that contains two or more possibilities together, with a definite phase between them that shows up as interference.
Cat state
A superposition of two clearly distinguishable states; for an oscillator, usually two coherent states in opposite phases, |α⟩ ± |−α⟩.
Coherent state
The quantum version of a definite oscillation, blurred only by zero-point motion. |α|² is its mean number of quanta.
Phonon
One quantum of vibration, of energy hf.
Zero-point motion
The unavoidable quantum blur of an oscillator in its ground state, √(ħ/2Mω).
Wigner function, negativity
A map of a quantum state over position and momentum. Where it dips below zero, no classical mixture can explain the state.
Effective mass
The mass that, with a chosen reference displacement, gives a vibration mode its energy as if it were a mass on a spring. Only mass × displacement² is fixed.
Decoherence
The loss of interference when the environment records which branch a system is in.
T1
The energy lifetime of a mode or qubit: about 84 µs for the ETH phonon mode.
Transmon qubit
A superconducting circuit with two working energy levels, controlled with microwaves.
HBAR
High-overtone bulk acoustic-wave resonator: a crystal with a thin piezoelectric layer that hosts many standing sound waves.
Macroscopicity μ
The base-10 logarithm of the longest electron coherence time, in seconds, that an experiment rules out for a minimal classicalising modification of quantum mechanics.
Collapse model (GRW, CSL)
A modification of quantum mechanics in which superpositions of large objects end spontaneously, with a rate λ and a length rC.
Diósi–Penrose model, EG, R0
Collapse tied to gravity: lifetime ħ/EG, with EG the gravitational self-energy of the difference between two branches and R0 the size over which each nucleus is smeared.
Planck mass
√(ħc/G) = 21.76 µg, a natural unit of mass.
Ultracold neutron
A neutron slow enough, a few metres per second, to be reflected by material surfaces.
peV
Pico-electronvolt, 10−12 eV.
C.L., σ
Confidence level of a limit (90% or 95% on this page); σ counts standard deviations of an exclusion or a discrepancy.
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