Einstein causality in curved spacetime #
This is the curved-spacetime counterpart of Minkowski Einstein causality. There is
no quasilocal algebra in curved spacetime, so local commutativity is phrased
inside a common containing basis algebra 𝔘(B): if B₁, B₂ are completely
spacelike and both contained in B, then the images of 𝔘(B₁) and 𝔘(B₂) in
𝔘(B) commute. This file pushes that into Hilbert space: under any
*-representation π of the containing algebra 𝔘(B) - in particular the GNS
representation of any state on 𝔘(B) - the spacelike-separated local observables
commute as bounded operators.
Main results #
Physicslib4.AQFT.HaagKastlerCurved.HaagKastlerNet.einstein_causality: causality in any representation of the containing algebra.Physicslib4.AQFT.HaagKastlerCurved.HaagKastlerNet.exists_gns_einstein_causality: the GNS specialization.
Einstein causality in a representation (curved spacetime). For any
*-representation π of a containing basis algebra 𝔘(B), the images of the
local observables of two completely spacelike-separated subregions B₁, B₂ ⊆ B
commute as bounded operators. This is Commute.map applied to the curved local
commutativity commute_of_spacelike.
Einstein causality on a GNS Hilbert space (curved spacetime). For any
state ω on a containing basis algebra 𝔘(B) there is a GNS triple (H, π, Ω)
reproducing ω in which the local observables of completely spacelike-separated
subregions commute as operators on H.