How does a particle get from A to B? Feynman's answer: it takes every path at once. Each history contributes a little arrow (a complex phase e^(iS/ℏ) set by its action S), and you add all the arrows. Wild paths have wildly spinning phases that cancel; the paths near the classical trajectory all point the same way and survive. Watch the phasors add — and watch the classical path emerge as ℏ shrinks.
⟨B|A⟩ = Σ_paths e^(iS[path]/ℏ)
S = ∫(½m v² − V) dt is the action of each path. Every conceivable trajectory — straight, looping, absurd — contributes a unit-length arrow whose angle is S/ℏ. The probability is the squared length of the total sum.
δS = 0. That stationary path is exactly the classical trajectory — Newton's laws are the principle of least action!
e^(iS/ℏ) becomes e^(−S_E/ℏ) in imaginary time, connecting quantum mechanics to statistical mechanics (the partition function is a path integral). Feynman diagrams are its perturbative expansion. Lattice QCD computes it numerically. It underlies string theory, quantum gravity, and the worldline formalism. "Sum over everything, let the phases sort it out" turned out to be how the universe computes.