Skip to content

13.7

Quantum foundations: collapse, macrorealism, and Wigner's friend

Decoherence explains "why we never see the interference", but not "why there is only one outcome". A century on, the measurement problem remains open — but it has turned from a philosophical debate into a research field with an experimental budget.

Recommended first

After this section you should be able to

  • State precisely what the measurement problem is, and which half of it decoherence has solved
  • Outline the price paid by each of three routes — many-worlds, objective collapse (GRW/CSL), and QBism — while staying neutral
  • Derive the Leggett–Garg inequality, and explain what it and Wigner's-friend experiments each put to the test

Thirteen chapters into this book, you might assume the foundations of quantum mechanics were poured and set long ago. But one question has hung in the air from the 1927 Solvay conference to this day: when, and by what right, does the wavefunction collapse?

There is a crack hidden in the list of postulates from section 3.7. The postulates say: left alone, a system evolves unitarily, deterministically, linearly, by the Schrödinger equation; but the moment it is “measured”, it suddenly jumps at random to some eigenstate by the Born rule. Two sets of rules, welded together by the word “measurement”. Yet isn’t a measuring device made of atoms? The apparatus, the experimenter, the whole laboratory building should obey the Schrödinger equation — so where does the second set of rules come from? At what moment, and by what agency, does “both this and that” become “just this”?

This is the measurement problem. It is not a student’s confusion; it is an open case in the very structure of the theory. The good news: over the past thirty years it has gone from after-dinner philosophy to a research field with precise theorems, decisive experiments, and grant budgets.

Settle the accounts first: which half decoherence solved

The decoherence theory of section 10.5 must take the stage first, because it is so often mistaken for the whole answer. What it genuinely solves is: why the interference of macroscopic superpositions is never seen. The environment “peeks” at macroscopic objects incessantly (every scattered photon, every colliding gas molecule carries away position information), and the off-diagonal elements of the reduced density matrix decay to zero in a vanishingly short time — the “dead + alive” coherence of a cat drains into the environment on a timescale of order 102310^{-23} seconds, never to be recovered by any experiment.

But keep the books honest: decoherence turns the coherent superposition dead+alive\ket{\text{dead}}+\ket{\text{alive}} into a mixed state (section 10.2) with half-and-half weights — a “list of probabilities”. It does not answer: why, in this particular run of the experiment, did this particular outcome appear? The final step from “list” to “single fact” is still unaccounted for. That is the remaining, hard half of the measurement problem.

Three routes, three invoices

To deal with the remaining half, each of the mainstream programmes has chosen to grit its teeth and swallow a particular cost. Here they are, laid out in three columns — what it claims / what it pays / whether experiment can tell it apart. This book takes no side.

Many-worlds (Everett, 1957). Claim: delete the collapse postulate; the universal wavefunction evolves unitarily forever. Measurement is just entanglement spreading, and in every branch there is a “you” seeing one definite outcome — all outcomes happen, in different branches. Cost: ontologically extravagant beyond measure (uncountably many parallel branches); the more technical soft spot is the status of probability — if every branch is realised, what does “outcome A has probability 1/3” even mean? Derivations of the Born rule from decision theory exist, but whether they succeed is still contested. Experimental discrimination: in principle impossible — its predictions coincide with standard quantum mechanics in full.

Objective collapse models (GRW 1986 / CSL). Claim: collapse is a real physical process. Modify the Schrödinger equation by adding a weak stochastic nonlinear term: each nucleon spontaneously localises its wavefunction (to a width of 10710^{-7} m) on average once every 101610^{16} seconds. For a single particle that is once in hundreds of millions of years, so quantum mechanics proceeds as usual; a macroscopic object has 102310^{23} nucleons and suffers 10710^{7} localisations per second — superpositions die instantly. The word “measurement” retires from the postulates. Cost: two new constants of nature conjured from nothing; the collapse noise implies a faint violation of energy conservation. Experimental discrimination: yes! It predicts that interference fails for sufficiently large molecules, and predicts a measurable background of spontaneous radiation. It is the only one of the three that sticks its neck out — large-molecule interferometry (now up to 2.5×1042.5\times10^4 atomic mass units) and cryogenic mechanical oscillators are steadily tightening its parameter space.

QBism and its relational cousins. Claim: the wavefunction is not a property of the world but the user’s state of belief — quantum mechanics is a normative handbook for “how to place bets on measurement outcomes”. Collapse is nothing but Bayesian updating: you saw the result, so of course you revise your bets. The measurement problem dissolves: there never was a physical collapse to explain. Cost: giving up the realist picture of “a quantum state independent of the observer”; “for whom is this outcome a fact?” becomes a statement that needs a subject, and the objectivity of science has to be re-argued. Experimental discrimination: in principle impossible — it is a reinterpretation of the same predictions.

Turning “macrorealism” into a measurable number: the Leggett–Garg inequality

Bell’s inequality (section 9.4) tests local realism with two spatially separated parties. Leggett and Garg (1985) turned the same logic around — towards time: a test of the everyday belief that “a macroscopic object is in a definite state at every moment”.

Wigner’s friend: putting the observer inside the wavefunction

Finally, the sharpest thought experiment of the present day. Wigner (1961) imagined: his friend, inside a sealed laboratory, measures a spin and obtains a definite outcome; but Wigner, standing outside, must by quantum mechanics describe “friend + spin” as an entangled superposition — for the friend the fact is settled; for Wigner it is not. Who is wrong? Or is “fact” itself relative?

In 2018, Frauchiger and Renner forged this into a theorem. Give each of two observers a friend “nested inside the wavefunction”, and let them reason about each other’s reasoning. They proved that the following three innocent-sounding assumptions cannot all hold: (Q) quantum mechanics applies to every system, observers included; (C) correct inferences by different observers can be chained together; (S) a measurement has a single outcome. Together with the related “local friendliness” inequality experiments (proof-of-principle demonstrations with photons playing the “friend” since 2019), this work backs every interpretation against the wall and makes it declare its position: many-worlds drops (S), objective collapse drops (Q), QBism drops (C). There is no free exit — and that is exactly its value as a theorem: it does not rule who is right, but it ensures nobody can pretend the bill isn’t theirs.

Where to dig deeper

Introductory reviews: Zurek’s long article on decoherence (Rev. Mod. Phys. 2003), the review by Bassi and colleagues on objective collapse models and their experimental bounds (Rev. Mod. Phys. 2013), and the Leggett–Garg test review (Emary et al., Rep. Prog. Phys. 2014). The original Frauchiger–Renner paper (Nat. Commun. 2018) has a modest technical barrier and is worth reading yourself — and as you read, try to find the loophole on your own: that is the standard initiation rite of the field.

The next section throws the question “where did the information go?” at a limiting case: drop a book into a black hole, wait for the black hole to evaporate away completely — is the book’s information still in the universe?

Section 96 of 106 · use to turn the page