Fixed at x = 30 nm · half-width 4 nm
Space = play/pause · R = reset
A free particle (zero potential, V = 0) is the first system in every quantum mechanics textbook. Classically it is trivial: a particle moves at constant velocity with a perfectly sharp position and momentum at every instant. Quantum-mechanically, even this minimal case reveals dramatic departures from that picture.
A Gaussian packet localises the particle at the cost of a spread in momentum (Heisenberg relation Δx·Δp ≥ ℏ/2). The packet spreads as it evolves:
A classical free particle never spreads — this broadening is a purely quantum effect. Different momentum components travel at different speeds, pulling the packet apart.
In this pedagogical setup, the detector is modeled phenomenologically; this is no longer a strictly free-particle Hamiltonian once detection is included. We therefore treat this as a particle with a phenomenological detector and ask: how does a detection event happen? The three views displayed here give different answers:
Important distinction: the lower |ψ|² strip is a position distribution at fixed time, while detector clicks are modeled as time-of-arrival events in a finite detector window.
Gaussian wave packet (free-particle propagator):
where σ(t) = σ0√(1+τ²), τ = ℏt/(mσ0²), x̅(t) = x0 + vgt, and the phase φ includes a carrier wave, a chirp term, and a Gouy-like phase.
The particle velocity in the pilot-wave view is:
Wave packet: different parts of the packet carry different local phase gradients. Particles near the front feel a larger phase gradient (higher “local k”) and are pushed forward; particles at the rear are slowed. This velocity differential is what spreads the packet. The pilot-wave velocity vB at the particle’s current position is shown in the readout panel.
Compared to the classical prediction v = ℏk/m, a Bohmian particle born near the leading edge of the packet starts slightly faster; one born near the trailing edge starts slower. In an ensemble all particles spread exactly with |ψ|², reproducing the Born-rule statistics.
The group velocity is the speed of the envelope (and the pilot-wave particle near the packet centre). The phase velocity is the speed of the wavefronts, which are not directly observable.
In a rigorous treatment the detector would enter the Hamiltonian as an imaginary (absorbing) potential −i W(x), so that the Schrödinger equation becomes
This causes local amplitude decay at rate W/ℏ: the probability density “leaks” out of the detector region, representing absorption. In this simulation the analytic free-particle wavefunction is multiplied by a smooth exponential damping factor inside the detector window as a pedagogical approximation:
where f(x) is a smooth profile that equals 1 inside the detector and tapers to 0 outside over a narrow edge, and γ = 0.02 fs−1 is a fixed absorption rate (corresponding to an imaginary-potential strength W ≈ γℏ ≈ 13 meV). This is not a full numerical PDE solve but correctly captures the qualitative physics: the wave amplitude is reduced in the detector region as the packet passes, providing backreaction on the guidance field in the pilot-wave view.
Lengths in nm · times in fs · energies in eV · mass = electron mass.
| Aspect | Classical | Collapse view | Pilot-wave view | Many-worlds view |
|---|---|---|---|---|
| Particle position | Always definite | Undefined before detection; updates on measurement | Always definite; guided by the velocity field | Undefined; different branches after detection |
| Particle velocity | v = p/m, constant | Momentum distribution |\u03c6̃(k)|²; only mean = ℏk/m | v(x,t) = (ℏ/m) Im(∂xψ/ψ), varies with position | Each branch carries its own momentum amplitude |
| Why does the packet spread? | It does not | Momentum uncertainty: Δk > 0 components disperse | Phase gradient of the evolving ψ pushes the front faster and slows the rear | Branches “diverge” in configuration space |
| Detection event | Trivial: particle hits detector | Born-rule probability; wavefunction collapses | Particle trajectory enters window; conditional wavefunction shows effective collapse | Universe branches; wavefunction never collapses |
| Role of V = 0 | No force; constant velocity | Free propagation away from detector; effective absorbing region during detection | Guidance from phase field; detector represented by an effective absorbing region | Free propagation with branch-dependent detection outcomes |
| vgroup = 2vphase? | N/A | Yes — purely kinematic (ω = ℏk²/2m) | Yes — particle near centre moves at vgroup | Yes — same dispersion relation |