Abstract

Suppose that particle detectors are placed along a Cauchy surface ΣΣ in Minkowski space-time, and consider a quantum theory with fixed or variable number of particles (i.e., using Fock space or a subspace thereof). It is straightforward to guess what Born's rule should look like for this setting: The probability distribution of the detected configuration on ΣΣ has density ∣ψΣ∣2|ψ_Σ|^2, where ψΣψ_Σ is a suitable wave function on ΣΣ, and the operation ∣⋅∣2|\cdot|^2 is suitably interpreted. We call this statement the "curved Born rule." Since in any one Lorentz frame, the appropriate measurement postulates referring to constant-tt hyperplanes should determine the probabilities of the outcomes of any conceivable experiment, they should also imply the curved Born rule. This is what we are concerned with here: deriving Born's rule for ΣΣ from Born's rule in one Lorentz frame (along with a collapse rule). We describe two ways of defining an idealized detection process, and prove for one of them that the probability distribution coincides with ∣ψΣ∣2|ψ_Σ|^2. For this result, we need two hypotheses on the time evolution: that there is no interaction faster than light, and that there is no propagation faster than light. The wave function ψΣψ_Σ can be obtained from the Tomonaga--Schwinger equation, or from a multi-time wave function by inserting configurations on ΣΣ. Thus, our result establishes in particular how multi-time wave functions are related to detection probabilities.

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