Why rare events happen: a quantum interpreter ✛

Original: "The Quantum Mechanics of Rare Events: From Quantum Walks to Stochastic Inflation"
arXiv:2608.06319v1 · 2026-08-06 · CC BY 4.0 · 1 min
Rare events are like mistakes made by an interpreter distracted by rustling noises. In the quantum world, their probability can be calculated if we account for how small disturbances accumulate.

An interpreter in a courtroom is distracted by every rustle: the creak of a chair, a cough, the rustle of papers. By the end of the day, they are not translating what the witness said, but what they heard through the noise. Rare translation errors are not the result of one loud shout, but the accumulation of many small noises.

In the quantum world, rare events arise in a similar way: a particle can end up far from its expected position not because of one giant leap, but because of many coordinated small steps. Scientists have found a way to compute the probability of such events. It turns out that one must take into account not only the usual measure of difference between distributions, but also how exactly we measure the system. It is as if the interpreter also loses information by choosing words from a limited vocabulary.

For a simple model, quantum walk, the probability of a rare event is not less than the square of the modulus of a special wave function. This gives a lower bound that is easy to compute.

This method was applied to the early Universe, where rare fluctuations could generate black holes. It turned out that previous calculations might have underestimated the frequency of such events. Now, like an interpreter who knows their weaknesses, we can more accurately predict when to expect errors.

In a classical random walk, the probability that all N steps go in the same direction is exponentially small, but it is precisely such collective fluctuations, not a single giant jump, that are usually responsible for rare events. In the quantum case, the situation is analogous: the distribution tail may be determined not by quantum tunneling but by the coordinated behavior of many small quantum steps.

P(x=N\alpha) \propto e^{-N I(\alpha)}
The probability of a rare event decays exponentially with the number of steps N, and the decay rate is independent of N and depends only on the scaled coordinate α.
P(\mu) \propto e^{-N S_{rel}(\mu \| \nu)}, \quad S_{rel}(\mu \| \nu) = \sum_s \mu(s) \log \frac{\mu(s)}{\nu(s)}
The more the empirical distribution differs from the true one, the lower the probability of observing it; the exponent is proportional to the number of steps N and the relative entropy.
P(x) \geq |\psi_{WKB}(x)|^2
The probability of finding the particle at point x is not less than the squared modulus of the WKB wave function, which allows one to estimate distribution tails knowing only the ground state.
Scientists
Max BornAlbert EinsteinJohn Stewart Bell
Concepts
stochastic inflation quantum fluctuation inflation quantum cosmological inhomogeneities statistical mechanics fluctuation-dissipation theorem inflationary cosmology fluctuation stochastic fluctuations random walk Fermi–Dirac statistics complex system dynamics statistics non gaussianity refined inflationary dynamics probability distribution droplet cosmological collider statistical noise Boltzmann equation classical physics