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Classical finite-regularity charged-scalar system and relative action

Definition

Let M be a smooth Hausdorff, second-countable, oriented four-manifold without boundary. Its smooth structure is retained throughout. A classical finite-regularity trivial-potential configuration consists of a time-oriented C3 Lorentzian metric g of signature (−,+,+,+), a global real C2 one-form A, and a global complex C2 scalar φ. Fix c,GN,μ0,Kφ>0, λ,Λ∈R, and V∈C∞(U;R) for an open U⊂R containing ∣φ∣2(M). Set κE=8πGN/c4. The curvature sign, length-coordinate convention x0=ct, and SI assignments are those of Trivial-potential classical charged-scalar Einstein–Maxwell system; only these formulas and conventions are imported, not that item's smooth-field restriction.

The Levi-Civita connection and curvature here are defined by their coordinate formulas for this C3 metric. Define

Fab:=∂aAb−∂bAa,Pa:=Daφ:=∂aφ−iλAaφ,

DaPb:=∇aPb−iλAaPb,Eφ:=gabDaPb−V′(∣φ∣2)φ,

Lφ:=gabPa‾Pb+V(∣φ∣2),ja:=KφλIm⁡(φ‾Pa),

Tabφ:=KφRe⁡(Pa‾Pb)−Kφ2gabLφ,TabEM:=μ0−1(FacFbc−14gabFcdFcd).

Conjugate charged derivatives use the opposite gauge sign. All indices are raised with g−1. Thus F,P are C1, j,Tφ,TEM are C1, Eφ and ∇aFab are continuous, and the Einstein tensor G is C1. The classical charged-scalar equations are the pointwise equations

dF=0,∇aFab=−μ0jb,Eφ=0,Gab+Λgab=κE(TabEM+Tabφ).

Here dF=0 already follows from F=dA with A∈C2. These are equations for the declared classical fields; they do not assert existence, smoothness improvement, or a weaker distributional theory.

For a continuous compactly supported real top form ω, define IM(ω) by a finite smooth cutoff localization near its support and the signed Riemann integrals of the resulting chart coefficients, extended by zero. The construction and its independence are proved below. For a complex top form extend IM by integrating its real and imaginary parts separately. For a configuration X=(g,A,φ) put

L(X):=[c316πGN(R(g)−2Λ)−14μ0cFabFab−Kφ2cLφ]volg.

If X1=X0 outside a compact set, its relative total action is S(X1;X0):=IM(L(X1)−L(X0)). The scalar and Maxwell relative actions are defined by their respective summands. No subtraction of divergent global integrals is intended. When the separate global integrals are defined and finite, this agrees with their difference.

Allowed independent directions are smooth compactly supported symmetric inverse-metric tensors qab, real one-forms α, and complex scalars η. Near zero parameter use

gε−1=g−1+εq,Aε=A+εα,φε=φ+εη.

The parameter interval is restricted to preserve signature, time orientation, and the potential domain. Stationarity means that the derivative of the relative total action vanishes for every such direction. These definitions include the original smooth trivial-potential system as a subclass, with its same action coefficients and tensors. They do not change the separate nontrivial-circle-bundle formulation or impose an integer condition on the real coupling λ.

Facts & Assumptions

Given: The smooth underlying oriented manifold, classical fields, constants, potential domain and compact directions in the Definition.

[F1]

Trivial-potential classical charged-scalar Einstein–Maxwell system supplies the displayed tensor formulas and SI conventions in its smooth sector. Their classical meaning at the regularity declared here is established directly below.

[F2]

Finite chart localization gives choice-free integration and compact Stokes provides finitely many nonnegative smooth functions with compact chart supports whose sum is one near any prescribed compact set. Only this smooth cutoff construction is used, not its smooth-form integration conclusion for the continuous coefficients here.

[F3]

A compactly supported Riemann integrand admits the global change-of-variables formula from a diffeomorphism near the relevant compact preimage applies to an injective C1 coordinate change with invertible derivative and any compactly supported Riemann-integrable coefficient inside its image.

[F4]

Every continuous function on a closed nondegenerate rectangle in Rm is Riemann integrable makes continuous coefficients on a closed nondegenerate rectangle Riemann integrable.

[F5]

Linearity, monotonicity, the absolute-value estimate and coordinate-slice additivity for the Riemann integral in Rm supplies finite linearity, monotonicity and the absolute-value estimate on nondegenerate rectangles. Constants have their constant value times rectangle volume by their Darboux sums.

Proof

technique · verify the classical tensor orders, construct the compact integral, and check that compact directions stay in the declared domain
1.1givenF1algebra

In a smooth chart, inversion of a nondegenerate C3 matrix is C3; the Christoffel formula therefore gives a C2 connection and the curvature formula a C1 tensor. Smooth coordinate changes preserve these regularities. The ordinary chain and product rules give F,P∈C1, the stated continuous Euler–Lagrange expressions, and C1 current and stress. Symmetry of g−1 makes gabPa‾Pb real and Re⁡(Pa‾Pb) symmetric; the Maxwell quadratic is also symmetric. The coordinate transformation laws follow by the chain rule, so all displayed equations compare global tensors. Commuting the continuous second partial derivatives of A gives dF=0.

1.2givenF2F3F4F5constructalgebra

Let K=supp⁡ω. Apply [F2] and multiply ω by its finitely many cutoffs. Each continuous coefficient has compact support strictly inside its chart, so zero extension is continuous and has a bounding rectangle; [F4] defines its finite integral. On a chart overlap the top-form coefficient transforms by the determinant of the smooth coordinate change. Its orientation sign converts that determinant to the absolute determinant, so [F3] gives the same signed integral in either chart. For two finite localizations (χi) and (τj), insert χiω=∑jχiτjω and the corresponding identity with i,j exchanged. Every product has compact support in the chart intersection. Finite linearity from [F5] and the overlap identity make both sums equal to the same double sum. Thus IM is well defined, linear and local. Empty support gives the empty sum zero.

2.1givenF1step 1.1step 1.2algebra

Each action density has continuous coefficients. Configurations agreeing off a compact set have density difference supported in that set, including the curvature term, because their derivatives agree on its open complement. Step 1.2 therefore defines every stated relative action. For three mutually compactly differing configurations the density differences add on the union of their compact supports, so their relative actions add. On smooth fields the construction is precisely the same finite chart integral and the formulas in [F1]; hence it agrees with the original smooth relative action.

2.2givenstep 1.1step 1.2constructalgebra

On the union K of the three direction supports, nondegeneracy and the chosen time cone persist under a uniformly small perturbation: use finitely many chart neighborhoods of the compact set and take the minimum of their positive parameter bounds. The attained set ∣φ∣2(K) is a compact subset of the open set U, so uniform convergence of ∣φ+εη∣2 keeps it inside U for small ε; outside K nothing changes. The resulting metric is C3 and the matter fields are C2, with δgab=−gacgbdqcd. The action densities and their parameter derivatives are continuous on compact parameter-chart rectangles. Consequently these directions are actual variations of the declared class, not only formal symbols.

3.1givenF3step 1.1step 1.2algebra∎

A real C3 function χ gives A′=A+dχ∈C2 and φ′=eiλχφ∈C2. The product rule gives P′=eiλχP and F′=F, so the action density is unchanged. Pullback by a smooth orientation-preserving diffeomorphism also preserves the classical class and the density formulas. For compactly supported transformations, step 1.2 and [F3] give invariance of the relative action. These are mathematical invariances, not a physical adoption or a solution-existence theorem.

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