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DefinitionDefinition: AI-adaptedProof: AI-adaptedPipeline-generatedprecheck passjudge pass (gpt-6-luna)verified 2026-11-04 (gpt-6.1-sol)
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Single M5 worldvolume tensor action

Physical scope

Source-normalized local bosonic PST functional for one smooth oriented six-dimensional timelike worldvolume and one abelian chiral two-form; overall physical tension, global patching, and multiple-M5 dynamics are not supplied.

Definition

Let (M11,gM) be the oriented Lorentzian CJS background of Eleven-Dimensional CJS Supergravity Bosonic Action. Let Σ6 be a smooth oriented six-manifold and let ι:Σ6→M11 be a smooth embedding (an injective immersion that is a homeomorphism onto its image). In dimensionless worldvolume coordinates define the normalized induced metric by g:=ℓp−2ι∗gM, where ℓp>0 is the Planck length from the CJS postulate; require g, with components gmn, to be nondegenerate Lorentzian with signature (−+++++). For this local formula, restrict to embeddings whose image lies in an open set V⊂M11 carrying smooth potentials C(3)∈Ω3(V) and C(6)∈Ω6(V); C(3):=ℓp−3C3,CJS∣V is the dimensionless normalization of the local CJS three-form, and C(6) is a supplied dimensionless local dual potential in the source convention. This rescaling is part of the adopted local field normalization; the CJS action does not itself supply C(6). Write P=ι∗ for pullback to Σ6. No transition data between potential patches or global Wess–Zumino functional is specified.

Use dimensionless worldvolume coordinates ξm, m=0,…,5, and adopt the source-normalized dimensionless field convention for the displayed local functional, with ℏ=c=1. In this convention gmn, Amn, Hmnl, a, and H~mn are dimensionless; this normalization is an adopted convention and does not follow from setting ℏ=1 alone. The overall physical tension is suppressed and fixed separately. Then g=det⁡(gmn)<0. Let A2∈Ω2(Σ6) be one real antisymmetric worldvolume two-form, written A2=12Amndξm∧dξn, and let a∈C∞(Σ6,R) be an auxiliary scalar. With the source's component convention set Fmnl=2(∂lAmn+∂mAnl+∂nAlm),F3=13!Fmnl dξm∧dξn∧dξl=2dA2,Hmnl=Fmnl−P[C(3)]mnl,H∗mnl=εmnlpqr3!−gHpqr, where ε012345=+1 is the oriented alternating symbol and indices are raised with g. Restrict to the non-null auxiliary-scalar branch (∂a)2:=gmn∂ma ∂na>0, and set H~mn=Hmnl∗∂la(∂a)2. For fixed g and a with spacelike da, at each ξ∈Σ6 let Dξ be the connected component, in the usual finite-dimensional real vector-space topology, containing 0∈Λ3Tξ∗Σ6 of the set of h∈Λ3Tξ∗Σ6 for which det⁡ ⁣(gmn(ξ)+i(∗gh)mnl∂la(ξ)(∂a)2(ξ))<0, where (∗gh)mnl:=εmnlpqrhpqr/(3!−g). Restrict the smooth field configurations to those with H3(ξ)∈Dξ for every ξ, and take the pointwise positive real square root −det⁡(g+iH~). On this domain define the source-normalized functional SPST=∫Σ6d6ξ[−det⁡(gmn+iH~mn)+−g4(∂a)2 ∂ma H∗mnlHnlp ∂pa]+∫Σ6(P[C(6)]+12F3∧P[C(3)]). The display first specifies a local six-form density L. If Σ6 is compact, set S=∫Σ6L. On a noncompact worldvolume use the local action in the following precise sense: for two admissible configurations q,q0 agreeing outside a compact subset of the interior, define S[q]−S[q0]:=∫Σ6(L[q]−L[q0]). The difference density is smooth and compactly supported, so this integral is finite. This notation defines the difference directly and does not subtract divergent numbers; no finite total action on a noncompact worldvolume is asserted.

This defines the single-abelian bosonic PST source convention on the stated potential patch; it does not define global patching or multiple-M5 dynamics.

Facts & Assumptions

Given: The stated smooth embedding and its induced Lorentzian metric, the source-normalized local fields and potential patch, and the non-null positive branch for da.

[F1]

The current CJS postulate fixes the physical eleven-dimensional C3,CJS normalization and mostly-plus spacetime convention; the Definition states its dimensionless rescaling (Eleven-Dimensional CJS Supergravity Bosonic Action).

[F2]

Finite chart localization defines the integral of smooth compactly supported top forms, independently of the charts, and gives ∫dη=0 for compactly supported (n−1)-forms on a boundaryless oriented manifold; apply this to the interior when the support avoids the boundary (Finite chart localization gives choice-free integration and compact Stokes).

[A1]

The differential form C(6) is used locally as the source's dual potential; the CJS carrier does not provide a global independent C6 field.

[A2]

PST transformations and the reported nonlinear self-duality equation below are source-reported local model data; they are not supplied by the source-free CJS action.

Proof

Given: The definitions of F3 and H3, a smooth local gauge parameter χ∈Ω2(V), and the source-reported transformations δC(3)=2dχ, δC(6)=−dχ∧C(3), and δA2=P[χ].

1.1givenalgebra

In components, Fmnl is twice the cyclic component formula for dA2, so F3=2dA2. Therefore dF3=2d2A2=0.

2.1F1F2A1A2step 1.1algebra∎

Pullback commutes with d, so the adopted transformations give δF3=2d(P[χ])=P[δC(3)], hence δH3=0. Both kinetic densities depend on the background potentials through H3 and are therefore unchanged. Suppressing pullback symbols only in the following worldvolume identity, the Wess–Zumino integrand varies by δ ⁣(C(6)+12F3∧C(3))=−dχ∧C(3)+dχ∧C(3)+F3∧dχ=2d(A2∧dχ). For a finite total action on a compact boundaryless worldvolume, Stokes gives zero variation. On a noncompact worldvolume the same conclusion holds for action differences when P[χ] has compact support in the interior: the displayed primitive then has compact support. For a worldvolume with boundary use compact support in its interior as well. No unrestricted Stokes claim at infinity is made.

Source-reported dynamics and the scalar functional

Pasti–Sorokin–Tonin define Vmn:=−2−(∂a)2g δ−det⁡(gpq+iH~pq)δH~mn. Their Eq. (9) reports the A2 equation εlmnpqr∂n ⁣(∂pa(∂a)2(Hqrs∂sa−Vqr))=0, and Eq. (10) reports that, after an appropriate gauge fixing of δAmn=12∂[ma φn], its general solution reduces to the nonlinear self-duality equation Hqrs∂sa−Vqr=0. The source cites earlier PST work for the gauge-fixing step and does not give the complete nonlinear variation proof.

Eq. (17) of the pinned PDF prints the auxiliary term with Hmnp, so the index m occurs three times in ∂ma H∗mnlHmnp∂pa. This is not a scalar under the Einstein summation convention. The paragraph immediately preceding Eq. (17) explicitly instructs replacement of the field strength in Eq. (1) by Eq. (16). Applying that instruction to its correctly contracted auxiliary density gives ∂ma H∗mnlHnlp∂pa, with each dummy index occurring exactly twice. The local functional above is defined by this explicit substitution into Eq. (1), followed by the displayed Wess–Zumino addition, rather than by treating the ill-typed printed component of Eq. (17) as a scalar. No erratum is asserted.

The Born–Infeld density and auxiliary density are added, as in both source equations; they are not multiplied. At H3=0 the first density is −g and the second vanishes. For real g and H~, transposition shows det⁡(g+iH~)=det⁡(g−iH~), its complex conjugate, so this determinant is real. At zero field it is g<0; the stated negative-determinant component therefore supplies the real positive square-root branch. These checks establish a well-typed local definition in the source convention. The nonlinear field equation and PST gauge-reduction assertion above remain explicitly source-reported model data; this definition does not claim an independent proof of that variation or supply it as a mathematical theorem.

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