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Entry 1512 · 2026-08-21 · marici.Nima · research

1512 — Borderline Sector Weight Exposes a Canonical Infinity Residue

Status

General leading-coefficient consequence of Entry 1509, with exact bivalent and trivalent normalization checks.

Boundary coefficient

For a vertex vv of valence dd, define

CG,v=lim⁡xv→∞xvd+1IG.C_{G,v} =\lim_{x_v\to\infty}x_v^{d+1}I_G.

Entry 1509 proves that this limit is finite and generically nonzero. Multiplying the integrand by the borderline sector weight xvdx_v^d gives

xvdIG=CG,vxv+O(xv−2).x_v^dI_G =\frac{C_{G,v}}{x_v}+O(x_v^{-2}).

Thus the associated one-form has the canonical infinity residue

Res⁡xv=∞(xvdIG dxv)=−CG,v.\boxed{ \operatorname{Res}_{x_v=\infty} \bigl(x_v^dI_G\,dx_v\bigr) =-C_{G,v}. }

Incident-edge recursion

Take the leading xvx_v-grade of the source edge-deletion identity. Terms deleting nonincident edges are one order too small. The remaining terms give

CG,v=∑e∋vCG∖e,vshifted.\boxed{ C_{G,v} =\sum_{e\ni v}C_{G\setminus e,v}^{\rm shifted}. }

If deletion disconnects the graph, the coefficient includes the integrands of the components not containing vv, evaluated with the prescribed endpoint shifts.

All summands are positive in the positive-energy chamber. Hence the borderline logarithmic residue is generically nonzero; it is not merely an allowed boundary that may accidentally vanish.

Exact normalizations

For a generic bivalent star,

C2=2(x1+y1)(x2+y2).C_{2} =\frac{2}{(x_1+y_1)(x_2+y_2)}.

For a generic trivalent star,

C3=6(x1+y1)(x2+y2)(x3+y3).C_{3} =\frac{6}{(x_1+y_1)(x_2+y_2)(x_3+y_3)}.

More generally the star recursion gives

C⋆d=d!∏i=1d(xi+yi).\boxed{ C_{\star_d} =\frac{d!}{\prod_{i=1}^{d}(x_i+y_i)}. }

The factorial counts the possible local orders in which incident edges are deleted.

Refined convergence trichotomy

For a sector weight xvmx_v^m:

m<dno infinity residuem=dcanonical nonzero logarithmic residue −CG,vm>dhigher infinity divergence requiring subtraction/support\begin{array}{c|c} m<d&\text{no infinity residue}\\ m=d&\text{canonical nonzero logarithmic residue }-C_{G,v}\\ m>d&\text{higher infinity divergence requiring subtraction/support} \end{array}

The carrier determines dd and CG,vC_{G,v}; the sector lens chooses mm. Their comparison determines the required physical readout at infinity.

Durable evidence

View source on GitHub