Unit 5 · Entanglement & RealityChapter 22 of 25

Interpretations, Decoherence & Schrödinger's Cat

Same equations, wildly different stories about reality

  • 25 min read
  • 38 min listen
  • 22 videos
01Video briefing

Start with the preview

Start here — today's preview. Watch “The Interpretations of Quantum Mechanics” from Domain of Science before (or after) this session. The lab will wait. Mostly.

Today's preview

The Interpretations of Quantum Mechanics

Domain of Science17 min

Dominic Walliman's illustrated tour of the main interpretations of quantum mechanics and the measurement problem they are trying to solve. As you watch, note how each view answers two questions: is the wavefunction real, and does it ever collapse? Today we sort the same views by which of three claims they give up, then add the physics of decoherence.

Watch on YouTube

More from the video vault

Deep dive

Measure for Measure: Quantum Physics and Reality | World Science Festival

World Science Festival97 min

Brian Greene moderates a 2014 panel in which Sean Carroll argues for many worlds, Sheldon Goldstein for Bohmian mechanics and Rüdiger Schack for QBism, with the philosopher of physics David Albert pressing all three. Watch it after Part 6: every move in the debate maps onto today's trilemma.

Watch on YouTube
Bonus

Understanding Quantum Mechanics #5: Decoherence

Sabine Hossenfelder13 min

Hossenfelder explains how entanglement with the environment makes interference disappear, the subject of Part 7. Listen for her verdict on whether decoherence solves the measurement problem, and compare it with Part 8.

Watch on YouTube
  • The Interpretations of Quantum Mechanics — Domain of Science — https://www.youtube.com/watch?v=mqofuYCz9gs
  • Measure for Measure: Quantum Physics and Reality | World Science Festival — World Science Festival — https://www.youtube.com/watch?v=GdqC2bVLesQ
  • Understanding Quantum Mechanics #5: Decoherence — Sabine Hossenfelder — https://www.youtube.com/watch?v=igsuIuI_HAQ
02Cold open

Today's mission

Dr. Q · cold open

Don't panic — superpose! Last session nature voted against local realism, and you may have left thinking the hard part was over. It was not. Bell told us what the world cannot be; he never told us what it is. Today I seal a cat in a steel box with a speck of radioactive material, a Geiger counter and a vial of poison, much as Erwin Schrödinger did on paper in 1935, and we ask the question that has split physics for ninety years: what is in the box before anyone looks? Rival schools of thought tell rival stories, almost all of them from the very same equations. Then we meet the environment, the most relentless spy in the universe, and time how quickly it unmasks the cat. No real cats will be harmed. I checked the paperwork.

By the end of this session you will be able to:

  1. Explain why Schrödinger's 1935 cat was a critique of reading the wavefunction as a literal picture of reality, not a claim that cats can be half dead.
  2. State the measurement problem precisely and classify interpretations by which of three incompatible claims they give up.
  3. Compare what the Copenhagen, many-worlds, pilot-wave, objective-collapse, QBist and relational accounts say happens inside the box.
  4. Describe decoherence as entanglement with the environment and calculate how interference visibility decays with the number of environmental interactions.
  5. Estimate decoherence and GRW collapse times for microscopic and macroscopic objects.
  6. Explain why decoherence alone does not solve the measurement problem and why the choice among interpretations remains open.
03The lesson

Read it — or listen along

8 parts. Press play on any part and the paragraph being read lights up as Dr. Q speaks.

Part 1

A Cat Built to Mock

Late in 1935, months after Einstein, Podolsky and Rosen accused quantum mechanics of being incomplete, Erwin Schrödinger published an essay, 'The Present Situation in Quantum Mechanics'. It put a name to entanglement and, in one deadpan paragraph, introduced physics' most famous animal. A cat is shut in a steel chamber with what Schrödinger called an infernal device: a Geiger counter holding so little radioactive material that within an hour perhaps one atom decays, or, with equal probability, none does. A decay trips the counter, which releases a hammer that shatters a flask of hydrocyanic acid, killing the cat.

Now simplify the sample to a single atom with a one-hour half-life, and apply the Schrödinger equation to everything in the chamber. The equation is linear: if two states are possible evolutions, so is any superposition of them. After an hour the atom is in an equal superposition of decayed and undecayed, and because counter, hammer, flask and cat form a causal chain, linearity carries that superposition all the way up. The joint state becomes |undecayed⟩|alive⟩ + |decayed⟩|dead⟩, divided by √2: an entangled state like those of Chapter 20. The wavefunction, Schrödinger wrote, would contain 'the living and dead cat (pardon the expression) mixed or smeared out in equal parts'.

Schrödinger was not announcing that cats can be half dead. He was building a reductio ad absurdum, an argument that derives a ridiculous conclusion to discredit a premise: here, that the wavefunction is a literal, complete portrait of reality. A blurred photograph of a sharp object, he observed, is not the same as a crisp photograph of a fog bank, and for the cat the wavefunction resembles the blurred photograph. The modern question is sharper: what physical story turns that entangled state into the single, unsmudged cat we always find?

Watch this part

Part 2

The Measurement Problem, Stated Precisely

The cat wraps a precise difficulty called the measurement problem. Textbook quantum mechanics, as Chapter 15 showed, runs on two rules. Rule one: an isolated system evolves smoothly and deterministically by the Schrödinger equation. Rule two: on measurement the state collapses at random to one outcome, with probability equal to the squared magnitude of that outcome's amplitude (the Born rule). But a measuring device is made of atoms too. If rule one governs it, counter and cat end in a superposition and no jump ever happens; if rule two takes over, we need a physical definition of 'measurement' that says when, and the textbooks never supply one.

In 1995 the philosopher Tim Maudlin sharpened this into a trilemma of three claims that cannot all be true. First, the wavefunction is a complete description of a physical system. Second, it always evolves by the linear Schrödinger equation. Third, every measurement has a single, definite outcome. Accept any two and the cat argument forces you to reject the third. An interpretation of quantum mechanics, a proposed account of what the mathematics says about the world, can be classified by the claim it gives up, or by how it reinterprets the wavefunction. That is our map.

Watch this part

Part 3

Copenhagen: The Pragmatic Cut

The oldest answer belongs to the Copenhagen family, the overlapping views of Niels Bohr, Werner Heisenberg and their circle from the late 1920s. It was never one doctrine, and the name itself apparently first appears in a 1955 essay by Heisenberg. Bohr insisted that quantum phenomena can be described only through whole experimental arrangements, themselves described in classical language: a counter clicks or it does not. His central idea, complementarity, first presented at Como in 1927, adds that mutually exclusive arrangements reveal mutually exclusive aspects, such as sharp position and sharp momentum, both needed for a full account. For Bohr the wavefunction was a symbolic tool for predicting outcomes, not a picture of a thing, and he never spoke of a collapse of the wave packet.

The textbook version adds a pragmatic rule: divide the world into a quantum system and a classically described apparatus, separated by a movable boundary called the Heisenberg cut. John von Neumann formalized this in 1932 with his projection postulate, which on measurement replaces the state by the state matching the result. Putting the cut at the counter, the cat or the lab notebook gives identical predictions. Read in Bohr's spirit, the cat poses no riddle: the counter's irreversible avalanche of ions is already a measurement, so the cat is alive or dead long before anyone lifts the lid.

The price is vagueness. Copenhagen never says physically what makes something classical, or exactly when rule two takes over. John Bell's 1990 essay 'Against measurement' protested that a fundamental theory should not lean on a word it cannot define. Defenders reply that physics concerns what can be said about experiments, and in daily practice the attitude David Mermin summed up as 'shut up and calculate' serves most physicists well.

Watch this part

Part 4

Many Worlds: The Equation Is Never Interrupted

In 1957 Hugh Everett, a doctoral student of John Wheeler at Princeton, proposed the boldest repair: delete rule two. In his 'relative state' formulation the wavefunction of the whole universe always obeys the Schrödinger equation, and nothing ever collapses. A measurement is just an entangling interaction. After an hour the box holds one branch in which the atom is intact and the cat alive, and another in which the atom has decayed and the cat is dead, each with weight one half. Bryce DeWitt popularized it in 1970 as 'many worlds'.

Each branch contains a version of the observer who sees one definite cat: every outcome happens, though each copy of you sees just one. The branches are not universes stamped out by a cosmic photocopier but components of one vast wavefunction that have stopped interfering, through the process of Part 7. Supporters prize the economy: no extra particles, no extra dynamics, no special role for observers and, they argue, no action at a distance, since Bell's theorem assumes single outcomes.

The costs are an extravagant ontology and a puzzle about probability: if every outcome occurs, what does it mean that one has probability 0.9? Everettians identify probability with each branch's squared amplitude, or weight, and David Deutsch in 1999 and David Wallace later argued that a rational agent in a branching world should bet exactly by the Born rule. Whether those arguments succeed is still fiercely contested.

Watch this part

Part 5

Pilot Waves: Particles With Somewhere to Be

The second route keeps single outcomes and the Schrödinger equation by denying that the wavefunction is the whole story. In pilot-wave theory, sketched by Louis de Broglie at the 1927 Solvay Conference and rediscovered and completed by David Bohm in 1952, every particle has a definite position at every moment. The wavefunction still obeys Schrödinger's equation, but its job is to steer: a guiding equation sets each particle's velocity from the gradient of the wavefunction's phase. The theory is completely deterministic.

Randomness comes only from ignorance of starting positions. If positions in an ensemble begin distributed as |ψ|², a condition called quantum equilibrium, they stay so distributed, and every Born-rule prediction follows. In the double slit each electron passes through one slit while its guiding wave passes through both and sculpts the fringes. In the box the cat's atoms always have positions, so the cat is simply alive or dead; the unoccupied part of the wave becomes an 'empty wave' that, after decoherence, never again affects the particles.

The theory is explicitly nonlocal. For several particles the wavefunction lives in configuration space, the space of all the particles' positions taken together, so when particles are entangled one particle's velocity depends instantly on where the others are, however distant. That is exactly the price Bell's theorem demands of hidden variables, and Bell openly admired Bohm's theory. Quantum equilibrium ensures that the nonlocality can never carry a signal, but it sits awkwardly with relativity: simple relativistic versions need a hidden preferred notion of simultaneity.

Watch this part

Part 6

Rewriting the Rules: Collapse, QBism and Relations

The third route changes the Schrödinger equation itself. In 1986 GianCarlo Ghirardi, Alberto Rimini and Tullio Weber proposed that every particle occasionally suffers a spontaneous, random 'hit' that localizes it to about 10⁻⁷ metres. For one nucleon, a proton or neutron, the rate is about 10⁻¹⁶ per second, a hit every 300 million years or so, so atoms behave just as standard theory predicts. But in a macroscopic superposition the particles are entangled, so a hit on any one displaced particle collapses the whole state, and with some 10²³ nucleons the hits arrive every 10⁻⁷ seconds. The cat is collapsed long before it could be smeared.

Lajos Diósi in 1987 and, independently, Roger Penrose from 1989 onward argued that gravity does the collapsing: a superposition of two different arrangements of mass should decay in a time of roughly ħ divided by the gravitational self-energy of their difference. Collapse models are rival theories, not interpretations: they modify the dynamics, and their random hits jiggle particles, so charged ones should glow faintly. In 2020 Sandro Donadi, Angelo Bassi and colleagues looked for that glow with a germanium detector under the Gran Sasso massif in Italy and ruled out the parameter-free Diósi-Penrose model. Interference of ever heavier particles, most recently sodium clusters above 170,000 atomic mass units (Vienna, January 2026), squeezes the models from another side; yet as of the Stanford Encyclopedia's 2025 review, no experiment had reached the original GRW values.

Two further families reinterpret the wavefunction instead. QBism, pronounced like 'cubism' and grown from work begun in 2002 by Carlton Caves, Christopher Fuchs and Rüdiger Schack, treats a quantum state as an agent's personal degrees of belief about their own future experiences; collapse is that agent updating on new experience, so nothing physical happens to the cat when you open the box. Carlo Rovelli's relational quantum mechanics (1996) holds that properties exist only relative to other systems: relative to the cat the outcome is definite, while relative to a physicist outside the sealed box, cat and atom are rightly described as entangled. Critics ask what, then, the world is like in itself.

Watch this part

Part 7

Decoherence: The Environment Is Always Watching

Every interpretation must explain one stubborn fact: we never see interference between macroscopically different states. The explanation, called decoherence, was founded by H. Dieter Zeh in 1970 and developed by Wojciech Zurek in the early 1980s and by Erich Joos and Zeh in 1985. No real object is isolated: air molecules strike it, photons scatter from it, and it radiates heat. Each encounter leaves the environment slightly different depending on the object's state, so the environment becomes entangled with the object and carries a record of it, spread across countless particles.

That record kills interference, because two alternatives can interfere fully only if they leave everything else in the same final state. Physicists describe the object alone by its reduced density matrix, whose diagonal entries are the probabilities of each alternative and whose off-diagonal entries, called coherences, carry the ability to interfere. Entanglement multiplies each coherence by the overlap γ between the environment states recording the two alternatives. If each passing particle carries a little information, its γ is slightly below one, and N independent particles multiply the coherence by γ raised to the power N, which plunges exponentially.

A dust grain ten micrometres across in still air is struck by about 10¹⁸ gas molecules every second, each recording its position, so a superposition of two locations decoheres in about 10⁻¹⁸ seconds. Zurek estimated that for a one-gram object at room temperature, superposed over one centimetre, decoherence beats ordinary frictional relaxation by a factor of order 10⁴⁰. A warm, breathing cat has no chance of showing interference between alive and dead.

Experiments have watched it happen. In 1996 Serge Haroche's group in Paris put a few-photon microwave field into a superposition of two phases inside a superconducting cavity, a miniature Schrödinger cat, and saw its coherence fade faster the more different the components were; Haroche shared the 2012 Nobel Prize in Physics. In 2003 Klaus Hornberger, Markus Arndt, Anton Zeilinger and colleagues in Vienna sent C₇₀ molecules through an interferometer while admitting traces of gas: the fringe visibility fell exponentially with pressure, because a single collision erased a molecule's interference.

Watch this part

Part 8

What Decoherence Does Not Do

Decoherence is mainstream physics, not an interpretation. Yet the total state of cat, atom and environment is still a superposition evolving by the Schrödinger equation; nothing collapsed. The cat's reduced density matrix merely looks like a coin toss, alive or dead with probability one half each, once we ignore the environment. Philosophers call this an improper mixture: it comes from setting aside part of an entangled whole, not from ignorance of an outcome that has already happened. Decoherence explains why the two cats never interfere. It does not say which cat you see, or why you see only one.

Each interpretation uses decoherence differently. For many-worlds it defines the branches. For pilot-wave theory it stops empty waves from ever interfering again with occupied ones. For Copenhagen it explains why the cut can sit anywhere above the microscopic scale without changing a prediction. For collapse models it is the noise that must be suppressed before a genuine collapse could be detected.

For every experiment yet performed, all of these interpretations give identical predictions, because they share the same mathematics, and collapse models deviate by amounts too small to have been seen. Which story is true is an open question. When Nature surveyed physicists in 2025, the centenary of quantum mechanics, its headline said they disagree wildly about what the theory says about reality. I'm mad, not wrong: the experiments are settled; the story is not.

Watch this part

04Video shelf

Go deeper on video

19 more videos for this chapter, 14 of them from universities, research institutes and Nobel lectures. The clips under “Watch this part” in the lesson start at the moment that matters.

19 videos · 12 h

  • Explainer · YouTube

    Schrödinger's cat: A thought experiment in quantum mechanics - Chad Orzel

    TED-Ed

    A five-minute animated TED-Ed lesson in which the physicist Chad Orzel walks through the thought experiment, a good first look before reading Part 1. Keep Part 1's point in view as you watch: Schrödinger built the cat to ridicule the idea of a smeared-out cat, not to endorse it.

  • Lecture · Rutgers University

    What is the Measurement Problem and What Would Solve It- Tim Maudlin

    Rutgers Graduate-Undergrad Seminar in Math-Phys · Tim Maudlin

    The philosopher whose 1995 trilemma organizes this whole chapter explains, in a talk for Rutgers' online seminar in mathematical physics, what the measurement problem is and what a solution would have to do. Sort every solution he considers by which of the three claims in Part 2 it gives up.

  • Explainer · YouTube

    Does Consciousness Influence Quantum Mechanics?

    PBS Space Time

    Follows the Copenhagen cut (from 1:32) up the von Neumann chain (4:35), where it can be placed anywhere between atom and observer, to Wigner's proposal that consciousness causes collapse (6:00). Watch it alongside the callout in Part 3, which explains why the movable cut does not have to end in a mind.

  • Lecture · University of Washington

    The Many Worlds of Quantum Mechanics with Dr. Sean Carroll

    UW Video · Sean Carroll

    A public lecture by one of the best-known advocates of many worlds, starting at the chapter marker for the Everett interpretation (30:40); the many-worlds chapter begins at 39:56 and the 'too many universes' worry at 44:18. Earlier chapters cover Copenhagen (21:32), Schrödinger's cat (23:18) and the Heisenberg cut (25:54) if you want a review of Parts 1–3.

  • Demo · MIT Department of Mathematics

    The pilot-wave dynamics of walking droplets

    MITMathLab · Daniel M. Harris & John W. M. Bush

    Three minutes of footage from John Bush's MIT lab: an oil droplet bouncing on a vibrating bath is pushed along by the very waves it makes, a classical picture of a particle steered by its guiding wave. Treat it as an analogy, not evidence: the droplet's wave lives in ordinary space, whereas Bohm's wavefunction lives in configuration space, which is where the nonlocality of Part 5 comes from.

  • Explainer · YouTube

    Do we have to accept Quantum weirdness? De Broglie Bohm Pilot Wave Theory explained

    Looking Glass Universe

    A clear beginner's account of de Broglie–Bohm theory and its pros and cons: superposition first (1:05), then Bohmian mechanics (3:15) and the key takeaways (6:23). Check her list of costs against Part 5's: extra positions, explicit nonlocality and friction with relativity.

  • Lecture · Aarhus University

    Quantum Science Colloquium - Angelo Bassi, University of Trieste

    Aarhus Universitet · Angelo Bassi

    "Precision tests of models of spontaneous wave function collapse", a 2023 colloquium by one of the authors of the 2020 Gran Sasso search described in Part 6. It treats collapse models as what they are, rival theories that experiments can rule out; listen for which kinds of experiment constrain the collapse rate and how.

  • Interview · World Science Festival

    Is Quantum Reality in the Eye of the Beholder? | World Science Festival

    World Science Festival · Carlo Rovelli

    Carlo Rovelli, the originator of relational quantum mechanics, explains it himself, starting at the chapter on the relational view (12:47). Rewind to 3:50 for how he sees the measurement problem and many worlds; the question critics ask in Part 6, what the world is like in itself, is the one to keep in mind.

  • Lecture · Kavli Institute for Theoretical Physics

    Quantum Theory of the Classical ▸ KITP Public Lecture by Wojciech Zurek

    Kavli Institute for Theoretical Physics · Wojciech Zurek

    A public lecture at KITP by Wojciech Zurek, one of the founders of decoherence theory in Part 7, on how a quantum universe produces the familiar classical reality. Keep the callout on pointer states in mind as you watch: the question is why the environment lets only certain states of an object survive.

  • Explainer · YouTube

    How Decoherence Splits The Quantum Multiverse

    PBS Space Time

    Shows decoherence doing a specific job for one interpretation: in many-worlds it is what turns one wavefunction into separate, non-interfering branches. Ask yourself the question in Part 8: decoherence explains why the branches stop interfering, but does it explain why you find yourself in only one?

  • Lecture · IBM Quantum

    Density Matrices | Understanding Quantum Information & Computation | Lesson 09

    Qiskit · John Watrous · 2022–25

    The lecture from IBM Quantum Understanding Quantum Information & Computation (John Watrous, 2022–25) that goes with Chapter 22. The whole course is in the Lecture Hall.

  • Lecture · Caltech

    Ph CS 219A Lecture 2 Density Operator

    John Preskill · 2021

    The lecture from Caltech Ph/CS 219A Quantum Computation (John Preskill, 2021) that goes with Chapter 22. The whole course is in the Lecture Hall.

  • Lecture · Royal Institution

    The mind-bending reality of quantum mechanics - with Jim Al Khalili

    The Royal Institution · Jim Al-Khalili · 2025

    A full Royal Institution Discourse from physicist Jim Al-Khalili on why quantum mechanics is both the strangest and the most successful theory in science, from the 1920s pioneers to lasers, MRI and quantum sensing. Watch it after the lesson, and keep asking which claims are experimental facts and which are interpretations.

  • Lecture · Royal Institution

    A Brief History of Quantum Mechanics - with Sean Carroll

    The Royal Institution · Sean Carroll · 2020

    Sean Carroll tells the story from Planck and Einstein through Bohr, de Broglie and Schrödinger, then argues that the measurement problem is still open and makes his case for the many-worlds interpretation. Notice where the history ends and his interpretation begins.

  • Lecture · Nobel Prize

    2012 Nobel Lectures in Physics

    Nobel Prize · Serge Haroche & David J. Wineland · 2012

    Serge Haroche on trapping photons in a box to watch the quantum-to-classical boundary — decoherence — in action, then David Wineland on superposition and entanglement with trapped ions. The experiments that turned thought experiments into laboratory routine.

  • Series · Royal Institution

    Quantum Physics Lectures & Talks

    The Royal Institution · Various speakers

    Thirty evening talks from the Royal Institution's lecture theatre in London, where Faraday once lectured: quantum fields, quantum biology, sensors, the quantum internet and the meaning of it all. Pick any one; each stands alone.

  • Course · Stanford

    Quantum Entanglements, Part 1

    Stanford · Leonard Susskind · 2006

    Nine evenings on the strangest resource in physics — spin, density matrices, entangled states and Bell's theorem — taught by Susskind to a room of non-specialists. Pairs naturally with Unit 5.

  • Course · IBM Quantum

    Understanding Quantum Information & Computation

    Qiskit · John Watrous · 2022–25

    The clearest modern course on quantum information, from IBM Quantum's John Watrous: single and multiple systems, circuits, teleportation and superdense coding, Shor's and Grover's algorithms, density matrices and error correction. Mathematically honest without being heavy.

  • Course · Caltech

    Quantum Computation

    John Preskill · 2021

    The graduate course from the physicist who coined the terms "quantum supremacy" and "NISQ": density operators, measurement, channels, Bell inequalities, teleportation, circuits, Shor's factoring, Grover's search and quantum simulation. Advanced, and worth every minute.

Every video for Chapter 22 in the Video Library

05To the blackboard

Key equations

Equation 1

The pilot-wave guiding equation

dQkdt=ℏmk Im⁡ ⁣[∇kψψ] ⁣(Q1,…,QN,t)\frac{d\mathbf{Q}_k}{dt} = \frac{\hbar}{m_k}\,\operatorname{Im}\!\left[\frac{\nabla_k \psi}{\psi}\right]\!(\mathbf{Q}_1,\dots,\mathbf{Q}_N,t)

In de Broglie-Bohm theory each particle moves along the gradient of the wavefunction's phase. Because psi is evaluated at the positions of all N particles at once, an entangled particle's velocity depends instantly on where the distant ones are: the theory is explicitly nonlocal.

What each symbol means
SymbolMeaningUnit
Qₖactual position of particle km
mₖmass of particle kkg
ψwavefunction of all N particles, a function of every position and timedepends on N
ħreduced Planck constant, 1.055×10⁻³⁴J·s

Say it: “the velocity of particle k equals h-bar over its mass, times the imaginary part of the gradient of psi with respect to that particle's position, divided by psi, all evaluated at the actual positions of every particle at time t”

Equation 2

GRW mean collapse time

tˉ=1NλGRW,λGRW≈10−16 s−1,rC≈10−7 m\bar t = \frac{1}{N\lambda_{\text{GRW}}}, \qquad \lambda_{\text{GRW}} \approx 10^{-16}\ \text{s}^{-1}, \qquad r_C \approx 10^{-7}\ \text{m}

If N nucleons sit in different places in the two branches of a superposition, the first spontaneous hit on any of them collapses the whole state, so the collapse rate grows in proportion to N. One nucleon waits hundreds of millions of years; a cat waits picoseconds.

What each symbol means
SymbolMeaningUnit
t̄mean time until the first collapses
Nnumber of nucleons displaced between the branchesdimensionless
λ_GRWspontaneous localization rate per nucleons⁻¹
r_Cwidth of the localizationm

Say it: “the mean waiting time for a collapse equals one over N times the GRW rate, where the rate is about ten to the minus sixteen per second for each nucleon and each hit localizes to about ten to the minus seven metres”

Equation 3

The cat's reduced density matrix

ρcat=∣α∣2∣A⟩⟨A∣+∣β∣2∣D⟩⟨D∣+αβ∗ ⟨ED∣EA⟩ ∣A⟩⟨D∣+α∗β ⟨EA∣ED⟩ ∣D⟩⟨A∣\rho_{\text{cat}} = |\alpha|^2 |A\rangle\langle A| + |\beta|^2 |D\rangle\langle D| + \alpha\beta^{*}\,\langle E_D|E_A\rangle\,|A\rangle\langle D| + \alpha^{*}\beta\,\langle E_A|E_D\rangle\,|D\rangle\langle A|

Start from the entangled state alpha times alive-with-environment-record-A plus beta times dead-with-record-D, and ignore the environment. The diagonal terms are the Born probabilities; the off-diagonal coherences, which carry interference, are multiplied by the overlap of the two records. When the records are distinguishable, the overlap is zero and interference is gone.

What each symbol means
SymbolMeaningUnit
|A⟩, |D⟩alive and dead states of the catdimensionless
α, βcomplex amplitudes, with |α|² + |β|² = 1dimensionless
|E_A⟩, |E_D⟩environment states that recorded alive or deaddimensionless

Say it: “rho for the cat equals the squared magnitude of alpha times the alive projector, plus the squared magnitude of beta times the dead projector, plus two cross terms, each multiplied by the overlap between the environment state that recorded alive and the one that recorded dead”

Equation 4

Visibility after N weak records

VN=V0 ∣γ∣N,γ=⟨e1∣e2⟩V_N = V_0\,|\gamma|^{N}, \qquad \gamma = \langle e_1|e_2\rangle

Each independent environmental particle that can tell the alternatives apart multiplies the fringe visibility by its overlap. Even weak records, with overlap close to one, compound exponentially.

What each symbol means
SymbolMeaningUnit
V₀fringe visibility with no environmental interactionsdimensionless (0 to 1)
γoverlap of the two states a single environmental particle can end up indimensionless (size 0 to 1)
Nnumber of independent interactionsdimensionless

Say it: “the visibility after N interactions equals the starting visibility times the size of gamma raised to the power N, where gamma is the overlap between the two states each environmental particle can end up in”

Equation 5

Collisional decoherence

V=V0 e−Nˉ=V0 e−p/p0V = V_0\,e^{-\bar N} = V_0\,e^{-p/p_0}

When every collision fully records which path was taken, only particles that suffer no collision at all still interfere. For a random (Poisson) number of collisions that fraction is e to the minus the mean number, which is proportional to gas pressure. This is the law measured with C₇₀ molecules in Vienna in 2003.

What each symbol means
SymbolMeaningUnit
N̄mean number of collisions during the flightdimensionless
pbackground gas pressurePa or mbar
p₀decoherence pressure, at which one collision is expected per flightPa or mbar

Say it: “the visibility equals the starting visibility times e to the minus the mean number of collisions, which equals e to the minus the gas pressure divided by the decoherence pressure”

Equation 6

Zurek's decoherence-time estimate

τD=τR(λthΔx)2,λth=ℏ2mkBT\tau_D = \tau_R \left(\frac{\lambda_{\text{th}}}{\Delta x}\right)^{2}, \qquad \lambda_{\text{th}} = \frac{\hbar}{\sqrt{2 m k_B T}}

For an object in contact with a warm environment, a superposition of positions a distance delta x apart loses coherence faster than friction slows the object by the square of the ratio of the separation to the thermal de Broglie wavelength. Valid when delta x is well above that wavelength.

What each symbol means
SymbolMeaningUnit
τ_Ddecoherence times
τ_Rrelaxation (friction) time of the object's motions
λ_ththermal de Broglie wavelengthm
Δxseparation between the superposed positionsm
m, Tmass of the object and temperature of the environmentkg, K
k_BBoltzmann constant, 1.381×10⁻²³J/K

Say it: “the decoherence time equals the relaxation time times lambda thermal over delta x, squared, where lambda thermal is h-bar over the square root of two m k B T”

06Worked examples

Real numbers, step by step

Cover the steps, try the problem yourself, then reveal the solution one step at a time.

Example 1

Erasing a fringe, one photon at a time

Problem

An electron in a two-path interferometer scatters photons on its way through. Each photon ends in one of two slightly different states depending on the path, with overlap γ = 0.95. With no scattering the fringe visibility is 100 percent. Find the visibility after 10 and after 100 scattered photons, and how many photons push it below 1 percent.

  1. Step 1: Each independent scattering multiplies the visibility by γ, so after N photons V = 0.95 raised to the power N.

  2. Step 2: N = 10: 0.95¹⁰ ≈ 0.599, so the fringes keep about 60 percent of their contrast.

  3. Step 3: N = 100: 0.95¹⁰⁰ ≈ 0.00592, about 0.6 percent.

  4. Step 4: For V below 0.01, take logarithms (any base gives the same ratio): N must exceed log(0.01) ÷ log(0.95) = −2 ÷ (−0.02228) ≈ 89.8, so 90 photons are needed.

Answer

About 60 percent after 10 photons and about 0.6 percent after 100; 90 photons push the visibility below 1 percent

Why it matters: No single photon carried much information: alone, each would leave 95 percent of the contrast. Decoherence is collective. Many weak records compound exponentially, which is why it is so fast for anything with a busy environment.

Try it yourself first — then check each step.
Example 2

A dust grain in still air

Problem

A dust grain of radius 5.0 μm floats in air at 101,325 pascals and 293 K (20 degrees Celsius), in a superposition of two positions 10 μm apart. Treating air as nitrogen (molecular mass 28.0 atomic mass units, or 4.65×10⁻²⁶ kilograms), estimate the collision rate and the decoherence time, assuming each collision records the grain's position.

  1. Step 1: Number density: n = p ÷ (k_B T) = 101,325 ÷ (1.381×10⁻²³ × 293) ≈ 2.50×10²⁵ molecules per cubic metre.

  2. Step 2: Mean molecular speed: v̄ = √(8k_B T ÷ πm) = √(8 × 1.381×10⁻²³ × 293 ÷ (π × 4.65×10⁻²⁶)) ≈ 471 metres per second.

  3. Step 3: Collision rate on a sphere: Z = n v̄ π r² = 2.50×10²⁵ × 471 × (π × (5.0×10⁻⁶)²) = 2.50×10²⁵ × 471 × 7.85×10⁻¹¹ ≈ 9.3×10¹⁷ per second.

  4. Step 4: A nitrogen molecule's de Broglie wavelength at this speed, h ÷ (m v̄), is about 0.03 nm, some 300,000 times smaller than the separation of 10 μm, so one collision distinguishes the two positions. Coherence survives only until the first collision: τ_D ≈ 1 ÷ Z ≈ 1.1×10⁻¹⁸ seconds.

Answer

About 9×10¹⁷ collisions per second, so the superposition decoheres in roughly 10⁻¹⁸ seconds, about one attosecond

Why it matters: In that time light travels about 0.3 nm, roughly the width of an atom. Long before anything could look at the grain, the air has already recorded where it is.

Try it yourself first — then check each step.
Example 3

Zurek's estimate: a gram bead versus an electron

Problem

Use τ_D = τ_R (λ ÷ Δx)², where the thermal wavelength is λ = ħ ÷ √(2m k_B T), to compare a 1.00-gram bead at 300 K in a superposition of positions 1.00 cm apart with an electron at 300 K in a superposition of positions 1.00 nm apart.

  1. Step 1: Bead: 2m k_B T = 2 × 1.00×10⁻³ × 1.381×10⁻²³ × 300 ≈ 8.28×10⁻²⁴, whose square root is 2.88×10⁻¹². So λ = 1.055×10⁻³⁴ ÷ 2.88×10⁻¹² ≈ 3.66×10⁻²³ metres.

  2. Step 2: Bead ratio: τ_D ÷ τ_R = (3.66×10⁻²³ ÷ 1.00×10⁻²)² = (3.66×10⁻²¹)² ≈ 1.3×10⁻⁴¹. Even if friction took 10¹⁷ seconds, roughly the age of the universe, decoherence would take about 10⁻²⁴ seconds.

  3. Step 3: Electron: 2m k_B T = 2 × 9.109×10⁻³¹ × 1.381×10⁻²³ × 300 ≈ 7.55×10⁻⁵¹, whose square root is 8.69×10⁻²⁶. So λ ≈ 1.055×10⁻³⁴ ÷ 8.69×10⁻²⁶ ≈ 1.21×10⁻⁹ metres, or 1.21 nm.

  4. Step 4: Electron ratio: (1.21 ÷ 1.00)² ≈ 1.5. The separation is comparable to λ, so the formula, valid only well above that scale, no longer predicts any dramatic speed-up: decoherence is no faster than ordinary relaxation.

Answer

About 1.3×10⁻⁴¹ for the bead, Zurek's famous 'order 10⁻⁴⁰' result, versus about 1.5 for the electron

Why it matters: The ratio scales as 1 ÷ (m Δx²). The bead is about 10²⁷ times heavier and its separation 10⁷ times larger, which is why quantum coherence is routine for electrons and invisible for beads.

Try it yourself first — then check each step.
Example 4

GRW's amplifier: proton, molecule, cat

Problem

In the GRW model each nucleon suffers a spontaneous localization at a rate of about 1×10⁻¹⁶ per second. Find the mean waiting time for the first hit for one nucleon, for a C₇₀ molecule (840 nucleons), and for a cat of mass 4.0 kg (nucleon mass about 1.66×10⁻²⁷ kilograms), assuming every nucleon is displaced by more than 10⁻⁷ metres between the alive and dead branches.

  1. Step 1: The mean waiting time for N nucleons is t̄ = 1 ÷ (N λ).

  2. Step 2: One nucleon: t̄ = 1 ÷ 10⁻¹⁶ = 10¹⁶ seconds; dividing by 3.156×10⁷ seconds per year gives about 3.2×10⁸ years.

  3. Step 3: C₇₀: t̄ = 1 ÷ (840 × 10⁻¹⁶) ≈ 1.2×10¹³ seconds, about 380,000 years, enormously longer than the milliseconds a molecule spends in an interferometer.

  4. Step 4: Cat: N = 4.0 ÷ 1.66×10⁻²⁷ ≈ 2.4×10²⁷ nucleons, so N λ ≈ 2.4×10¹¹ per second and t̄ ≈ 4×10⁻¹² seconds.

Answer

About 300 million years for one nucleon, about 380,000 years for C₇₀, and about 4 picoseconds for the cat

Why it matters: One rule leaves atoms and molecules fully quantum yet makes cats classical almost instantly. Even if only 1 percent of the cat's nucleons were displaced, collapse would still come in about 0.4 nanoseconds.

Try it yourself first — then check each step.
07Myth busters

What everyone gets wrong

Read the myth, decide whether you believed it, then bust it.

  • Myth #1

    In the Copenhagen interpretation the cat is literally half dead and half alive until someone opens the box.

    Truth

    Schrödinger designed the cat to ridicule exactly that literal reading. In Copenhagen-style views the wavefunction is a tool for predicting outcomes, not a portrait of a half-dead animal, and the Geiger counter's irreversible click already counts as a measurement; read in Bohr's spirit, the cat is alive or dead long before the lid is lifted. Even the formal superposition is not a cat at 50 percent health: it is a statement about the probabilities of two complete outcomes.

  • Myth #2

    Decoherence completely solves the measurement problem.

    Truth

    Decoherence explains, with superb experimental support, why interference between macroscopically distinct states vanishes almost instantly and why pointer states such as definite positions are stable. But the total state of system plus environment remains a superposition evolving by the Schrödinger equation, and the reduced state only looks like a classical mixture once the environment is ignored. Decoherence does not select which outcome occurs or explain why we see one; each interpretation must still supply that.

  • Myth #3

    In many-worlds, everything you can imagine happens in some universe.

    Truth

    Only outcomes produced by the Schrödinger equation occur, weighted by their squared amplitudes. The branches are decohered components of one wavefunction, not freely invented realities, and they cannot communicate with one another.

  • Myth #4

    Interpretations are pure philosophy; nothing about them can ever be tested.

    Truth

    The interpretations proper agree on every standard prediction, but collapse models change the dynamics and are being tested: in 2020 an underground experiment at Gran Sasso ruled out the parameter-free Diósi-Penrose model. The debate also drives physics, as when Bohm's theory inspired Bell's theorem.

08Interactive lab

Your turn at the controls

Welcome to the Cat Box. Inside: one radioactive atom with a one-hour half-life, a Geiger counter, a hammer, a sealed vial and a strictly simulated cat. Close the lid, run the clock, then put on one of five pairs of interpretation goggles, Copenhagen, many-worlds, pilot-wave, objective collapse or QBism, and watch the same box tell five different stories while the statistics never change. Next door, the decoherence simulator lets you fire environmental particles at a two-path interference experiment and watch its fringes fade.

Your tasks

0/4

How it connects to the theory

The fringe visibility falls as the starting visibility times the overlap raised to the power N, exactly as in worked example 1; when every hit is a complete record, the decay follows the exponential law of the 2003 Vienna fullerene experiment. Each lens is one escape route from Maudlin's trilemma, the four A's of the mnemonic, and the matching game checks that you can tell which claim each interpretation gives up. The unchanging 50 percent is the point: interpretations differ in story, not in prediction, and decoherence removes the fringes without ever choosing a cat.

The Cat Box: Choose Your Interpretation loads as you scroll down.

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09Memory aids

Make it stick

Memory trick

The cat's report card: four A's and a D. Picture it pinned to the box. The four A's are the ways out of the measurement problem. Add something: pilot-wave theory adds particle positions. Alter the equation: GRW and Diósi-Penrose collapse change Schrödinger's law. Accept every outcome: many-worlds keeps them all. Adjust what ψ means: Copenhagen, QBism and relational quantum mechanics treat it as a tool, a belief or a relation. The D is Decoherence, which Doesn't Decide: it explains why the cat looks classical, never which cat you get. To use it, take any interpretation and ask which A it earns; and if you are ever tempted to say decoherence solved everything, remember that it only got a D.

Analogy — and where it breaks

Decoherence is like a secret at a crowded party. While only two people know whether you were in the kitchen or the garden, the story could still be quietly undone; once every guest has heard a slightly different version, nobody can ever gather all the versions back. Interference needs the alternatives to leave no trace, and the environment is an incurable gossip: every air molecule and photon carries a tiny record, and the records multiply. Where it breaks: gossip eventually settles on one true story, but decoherence never picks one, since the global state still holds both versions. And no guest needs to listen or understand; the records are physical correlations, not anyone's knowledge.

The whole chapter in one line

Rival stories, same predictions so far: decoherence explains why cats never look smeared, but which story is true remains open.

Leitner flashcards

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10Games

Play it into long-term memory

Match the vocabulary, then take the Quiz Show. Score 70% or better to tick it off your checklist.

Vocab match · timed

Vocab Match

Match each term to its definition, against the clock.

  • 12 pairs in 2 rounds
  • 100 points a match, more on a streak
  • −25 per mistake · speed bonus each round
  • Finish with 3 mistakes or fewer to win
Live from the lab

Dr. Q's Quantum Quiz Show

Dr. Q, your host

Welcome, contestants! 8 questions, 30 seconds each, and one mad scientist judging you, lovingly. Answer fast for a speed bonus; answer right in a row and your points multiply.

  • 100 per answer
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11Worksheet

Prove it on paper

Answer every question, check your work, and read the explanations — the stretch challenge is for the truly mad.

14 questions12 terms1 challenge

Work through these questions with the lesson closed, then check yourself against it. For calculations show every step and give answers to the precision of the data, two or three significant figures. Useful relations: visibility after N interactions V = V₀ γ^N; collisional decoherence V = V₀ e^(−p/p₀); GRW mean waiting time t̄ = 1/(Nλ) with λ ≈ 1×10⁻¹⁶ s⁻¹ per nucleon; nucleon mass ≈ 1.66×10⁻²⁷ kg; Born rule P = |amplitude|².

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Part A

Vocabulary

Measurement problem
The conflict between linear Schrödinger evolution, which produces superpositions of outcomes, and the single definite outcomes we observe.
Copenhagen interpretation
The family of views from Bohr, Heisenberg and colleagues that treats the wavefunction as a predictive tool and measurement as a primitive, classically described event.
Heisenberg cut
The movable boundary between the system treated quantum mechanically and the apparatus treated classically.
Many-worlds interpretation
Everett's 1957 proposal that the universal wavefunction never collapses and every measurement outcome occurs in its own branch.
Pilot-wave theory
The de Broglie-Bohm theory, in which particles always have definite positions and move as directed by the wavefunction through a guiding equation.
Quantum equilibrium
In pilot-wave theory, the condition that particle positions are distributed as |ψ|², which reproduces the Born rule and forbids signalling.
Objective collapse model
A modified quantum dynamics, such as GRW or Diósi-Penrose, in which wavefunctions collapse spontaneously at rates that grow with size or mass.
QBism
The view that quantum states encode an agent's personal degrees of belief, so that collapse is the updating of those beliefs.
Relational quantum mechanics
Rovelli's 1996 interpretation in which states and properties are defined only relative to other physical systems.
Decoherence
The suppression of interference between alternatives when a system becomes entangled with an environment that records them.
Pointer state
A state, such as a definite position, that survives continual monitoring by the environment and therefore looks classical.
Improper mixture
A state that looks like a classical probability mixture only because part of an entangled whole has been ignored.

Part B

Questions

Auto-checked except short answers, which you mark yourself.

  1. Question 1.Multiple choice

    What was Schrödinger's main purpose in describing the cat in 1935?

  2. Question 2.True or false

    In de Broglie-Bohm pilot-wave theory, each electron in a double-slit experiment passes through both slits.

  3. Question 3.Multiple choice

    Which of Maudlin's three claims does the GRW collapse model reject?

  4. Question 4.Fill in the blank

    The loss of interference that occurs when a system becomes entangled with an environment that records its state is called .

  5. Question 5.True or false

    In Everett's many-worlds interpretation the wavefunction of the universe never collapses.

  6. Question 6.Fill in the blank

    In QBism, a quantum state represents an agent's personal degrees of about the outcomes of their future actions on the world.

  7. Question 7.Multiple choice

    Why can the nonlocality of Bohmian mechanics never be used to send a faster-than-light message?

  8. Question 8.True or false

    After decoherence, the joint state of cat, atom and environment is no longer a superposition.

  9. Question 9.Short answer

    Using the idea of which-path records, explain why a dust grain in air decoheres far faster than an electron in a well-isolated interferometer.

  10. Question 10.Short answer

    What is the essential difference between an objective collapse model and an interpretation such as many-worlds, and how has a collapse model been tested?

  11. Question 11.Calculation

    Each environmental photon scattered by a particle in a two-path interferometer has overlap γ = 0.90 between its two possible final states. Starting from 100 percent visibility, what is the fringe visibility after 20 photons?

    Give a number and units. 6.63×10⁻³⁴, 6.63e-34 and 6.63 x 10^-34 all work.

  12. Question 12.Calculation

    In a fullerene interferometer the vacuum visibility is V₀ = 0.40 and the decoherence pressure is p₀ = 0.80×10⁻⁶ mbar. Find the visibility at p = 1.2×10⁻⁶ mbar and the fraction of molecules that cross without any collision.

    This one asks for more than one value — give each, with its units.

  13. Question 13.Calculation

    A 1.0 μg dust grain (1.0×10⁻⁹ kg) is placed in a superposition of two positions more than 10⁻⁷ m apart. According to GRW, what is the mean time before a spontaneous collapse?

    Give a number and units. 6.63×10⁻³⁴, 6.63e-34 and 6.63 x 10^-34 all work.

  14. Question 14.Calculation

    In a version of the cat box, a single radioactive atom with a half-life of 1.0 hour controls the poison. What probability does every interpretation assign to finding the cat alive after 3.0 hours, and what is the magnitude of the 'alive' amplitude?

    This one asks for more than one value — give each, with its units.

Part C · optional, dangerous, extremely rewarding

Mad scientist challenge

Decohere a dust grain by degrees. A grain is in the superposition α|L⟩ + β|R⟩ with |α|² = |β|² = 1/2, and each environmental particle that hits it ends in |e_L⟩ or |e_R⟩ with real overlap ⟨e_L|e_R⟩ = cos θ. (a) Show that after N independent hits the off-diagonal element of the grain's reduced density matrix is (1/2)(cos θ)^N. (b) If each hit carries only weak information, θ = 0.10 rad, how many hits reduce the coherence to one millionth of its starting value? (c) In still air at room temperature a grain of radius 5 μm suffers about 9.3×10¹⁷ collisions per second. Even with such weak records, how long does that take? (d) Explain what this calculation has not shown.

12Wrap-up

Recap & sign-off

Key takeaways

  • Schrödinger's 1935 cat was a reductio: amplifying quantum indefiniteness to everyday scale shows how absurd a literal reading of the wavefunction becomes.
  • The measurement problem: a complete wavefunction, linear evolution and single outcomes cannot all hold, and each interpretation abandons or reinterprets one of them.
  • Copenhagen treats the wavefunction as a predictive tool and measurement as a pragmatic cut; read Bohr's way, the counter settles the cat's fate long before the lid opens.
  • Many-worlds (Everett, 1957) keeps the Schrödinger equation everywhere and lets every outcome occur in its own decohered branch; its open problem is probability.
  • Pilot-wave theory (de Broglie 1927, Bohm 1952) adds definite positions guided by ψ; it is deterministic and explicitly nonlocal, yet forbids signalling.
  • Collapse models (GRW 1986, Diósi-Penrose) alter the dynamics and can be tested; QBism and relational quantum mechanics reinterpret the state as belief or relation.
  • Decoherence entangles objects with their environment and erases interference in about 10⁻¹⁸ seconds for a dust grain in air, but it never chooses an outcome.
  • Every mainstream interpretation agrees with every experiment so far; which one, if any, is right remains open.
Dr. Q signs off

So the cat is fine, or it is not, and either way it never looked smeared, because the air in the box gossiped about it within an attosecond. Which story about reality is true? The equations will not say, and I refuse to fake a verdict. But engineers drew a practical lesson from all this: coherence is fragile, precious and useful. Next session we stop fearing superposition and start computing with it. Chapter 23: Qubits and Quantum Computing. Bring patience; decoherence will be waiting.

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