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The reciprocal-potential invariant determines the end spin bound

Statement

Let M>0 and S=(S1,S2,S3) be constants and J=∣S∣, using the Euclidean norm. Let (X,g) be a smooth Lorentzian four-manifold of signature (−,+,+,+). Supply an open subset E⊂X and a smooth coordinate chart (t,x1,x2,x3) on E with coordinate range I×{x∈R3:∣x∣>R}, where I is a nonempty open interval and R>0. Set r=∣x∣=(∑i=13(xi)2)1/2. Write gab for the components of the inverse metric (equivalently the unique inverse matrix of the nondegenerate matrix (gab)), use a,b=0,1,2,3 with x0=t, and use i,j=1,2,3 for spatial indices. Assume ∂tgab=0 and gij=δij+O(r−1). Suppose smooth real functions y,z satisfy ∂ty=∂tz=0, y=r/(2M)+O(1) and z=(S⋅x)/(2M2r)+O1(r−1). In this chart, h=O(r−k) means ∣h(t,x)∣≤Cr−k for sufficiently large r, uniformly in t and direction; tensor-component estimates are componentwise. For the remainder h=z−(S⋅x)/(2M2r), O1(r−1) means both ∣h∣≤Cr−1 and ∣∂ih∣≤Cr−2 for every spatial index i, with the same uniformity. Define B=z2+4M2(y2+z2)gab∂az∂bz. Then B=J2/(4M4)+O(r−1). For the conditional conclusion, suppose g,y,z are defined smoothly on a connected open domain D⊂X containing E, and supply a nonempty open subset V⊂D. If this same scalar B is constant on D and 0≤B<1/4 on V, then J<M2. The constancy and the bound on V are explicit inputs, not consequences of the asymptotic expansion.

Facts & Assumptions

[F1]

A smooth Lorentzian metric of signature (−,+,+,+) is symmetric and nondegenerate, has smooth chart components and admits a timelike vector at every point. A smooth timelike field on an open set is a time orientation there. The inverse-metric interface applies to a time-oriented restriction and defines ♭p(v)=gp(v,⋅), ♯p=♭p−1 and gp−1(α,β)=gp(♯pα,♯pβ), with matrix components gab. Step 1.1 constructs suitable local restrictions and shows that these definitions agree independently of their time orientations. The particular chart, stationarity, decay bounds and sets D,V are explicit data in the Statement. Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model The inverse metric, musical isomorphisms and index raising

[F2]

Sum, product, quotient and chain rules apply to differentiable real functions, with a nonzero denominator for the quotient rule and the composition defined near the point for the chain rule. Apply these rules to each spatial coordinate with the other coordinates fixed. On positive arguments, (u1/2)′=1/(2u1/2); here r2>R2>0. Sum, product, quotient, and chain rules from difference quotients Continuity and derivatives of positive-base real powers

Proof

Given: The hypotheses in the Statement.

Goal: Establish the stated asymptotic formula and conditional spin bound.

1.1givenF1algebra

Fix any point p of the domain where the inverse metric is used. By [F1] there is a timelike vector v∈TpX. In a chart about p, extend its four components as constants to obtain a smooth field N=∑a=03va∂a. The function q↦gq(Nq,Nq) is continuous and negative at p, so it is negative on an open neighborhood W of p. Thus (W,g∣W,N) meets the inverse-metric interface's time-orientation hypothesis. Its maps ♭q, ♯q and gq−1 are determined solely by gq, not by N or W, so definitions obtained this way agree on every overlap. Their chart components are the unique inverse of (gab), and bilinearity gives g−1(dz,dz)=∑a,b=03gab∂az∂bz. This establishes the contraction wherever needed without assuming a global time orientation or choosing neighborhoods simultaneously.

1.2givenF2algebra

Put n=x/r, so ∑ini2=1, with Euclidean lowering Si=Si and ni=ni. By [F2], ∂ir=xi/r=ni and ∂i((S⋅x)/r)=(Si−ni(S⋅n))/r. Differentiating the expansion for z is therefore justified by the stated derivative bound on its remainder and gives ∂iz=(Si−ni(S⋅n))/(2M2r)+O(r−2). Since ∣S⋅n∣≤∑i∣Si∣, the leading coefficients are uniformly bounded. Expanding the finite sum of squares, using ∑i(Si−ni(S⋅n))2=J2−(S⋅n)2, gives ∑i(∂iz)2=(J2−(S⋅n)2)/(4M4r2)+O(r−3).

2.1givenF1step 1.1step 1.2algebra

Each ∂iz is O(r−1), so ∑i,j(gij−δij)∂iz∂jz=O(r−3) by the componentwise metric bound and the finite number of terms. Since ∂tz=0, every temporal or mixed term in the contraction vanishes. Thus gab∂az∂bz=(J2−(S⋅n)2)/(4M4r2)+O(r−3).

3.1givenF1step 1.2step 2.1algebra

The other expansions give 4M2(y2+z2)=r2+O(r) and z2=(S⋅n)2/(4M4)+O(r−1): expand y=r/(2M)+O(1) and the bounded leading term of z. Multiplying the contraction from step 2.1 by r2+O(r) gives (J2−(S⋅n)2)/(4M4)+O(r−1). Adding z2 cancels the angular term, yielding B=J2/(4M4)+O(r−1).

4.1givenstep 3.1algebra∎

If B is a single constant on D, its value equals the limit along the end, hence B=J2/(4M4). Since V is nonempty, the assumed bound there then gives J2/(4M4)<1/4. Multiplication by 4M4>0 and J≥0 imply J<M2. No global metric isometry or independent angular-momentum conservation law was used.

Remarks

The original horizon-neighborhood application is included by taking V to be its nonempty open portion in D. The calculation requires exactly the chart and differentiated estimates stated above; the conditional implication uses only the constancy on D and the bound on V. No causal property of a horizon is an additional premise of this calculation.

Depends on

Used by · 1

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