Axiom 5 (Isometric Covariance), curved spacetime #
This file formalises the blueprint declaration
def:isometric-covariance-in-curved-spacetime (Axiom 5 of the
Haag-Kastler axioms on a Lorentzian spacetime, Chapter 10
(sections/sec10/haag-kastler-axioms-in-curved-spacetime) of the
AQFT-in-Lean blueprint):
A member
Οof the group of isometries ofMconnected to the identity acts onπ(π)via a unital*-isomorphismΞ±_Ο : π(π) β π(Ο(π)), whereΟ(π)is the image of the basis set. The action satisfies (1)Ξ±_π = id, (2)Ξ±_{Ο'Β·Ο} = Ξ±_{Ο'} β Ξ±_Ο, and (3) it commutes with the isotony monomorphismi(Axiom 2).
Main definitions #
Physicslib4.AQFT.HaagKastlerCurved.IsometricCovariance: aProp-valued predicate on aLocalNet Mand its Axiom 2 isotony family asserting Axiom 5.
Modelling notes #
The Minkowski analogue (
LorentzCovariance) uses the identity component of the inhomogeneous Lorentz group. Here the analogous role is played by the abstract groupM.Isomof isometries connected to the identity, acting onM.Carrier; the induced pointwise action onSet M.Carrier(Ο β’ B = Ο(B)) supplies the blueprint'sΟ(π).Conditions (1) and (2) carry cross-fiber identifications
U.algebra (1 β’ B) = U.algebra BandU.algebra ((Ο'Β·Ο) β’ B) = U.algebra (Ο' β’ (Ο β’ B))coming fromone_smul/mul_smul, implemented asEq.mpr/congrArg. This matches the MinkowskiLorentzCovarianceencoding verbatim.
Axiom 5 in curved spacetime (isometric covariance): the isometries connected to the identity act on the net, compatibly with isotony.
In curved spacetime the PoincarΓ© group of the Minkowski axioms is replaced by the symmetries the
spacetime actually has: the group M.Isom of isometries of M connected to the identity. A generic
spacetime has no isometries other than the identity, and then the axiom says little. The axiom
asks for a unital *-isomorphism Ξ±_Ο : π(B) β π(Ο(B)) for every such isometry Ο and every region
B, where Ο(B) is the image of B under Ο, such that
- Ξ±_1 is the identity;
- Ξ±_(Ο'Ο) = Ξ±_Ο' β Ξ±_Ο; and
- Ξ±_Ο commutes with the isotony family i of Axiom 2: whenever Bβ β Bβ are basis sets, Ξ±_Ο β i(Bβ, Bβ) = i(Ο(Bβ), Ο(Bβ)) β Ξ±_Ο.
In condition 3, Ο(Bβ) and Ο(Bβ) are basis sets with Ο(Bβ) β Ο(Bβ) because isometries preserve
basis sets (the interface field LorentzianSpacetime.isBasisSet_smul) and images preserve
inclusions (Set.smul_set_mono), so no further hypothesis is needed. The predicate takes the
isotony family as a parameter, so the action respects the net's own embeddings.
HaagKastlerNet.covEquiv chooses the maps Ξ±_Ο. There is no quasilocal algebra for them to act
on; on a region fixed by Ο they give automorphisms of its algebra (HaagKastlerNet.stabAut).
Implementation note: π(1 β’ B) and π(B), and π((Ο'Ο) β’ B) and π(Ο' β’ (Ο β’ B)), are different types
that are equal only propositionally, so conditions 1 and 2 transport along those equalities
(one_smul, mul_smul) with Eq.mp. For a geometric spacetime, M.Isom is the oriented identity
component of its isometry group (toAbstractIdentityComponent).
Blueprint: def:isometric-covariance-in-curved-spacetime
Equations
- One or more equations did not get rendered due to their size.