Pairwise closure of power-law resistor networks and sharp three-terminal elimination defects

We characterize when eliminating the interior vertices of a finite positive-weight power-law resistor network preserves an energy given by a sum of pairwise terms with the same exponent. For every fixed 1<p<∞, p≠2, this holds exactly when each connected component of the interior graph meets at most two boundary vertices. The criterion is independent of the positive weights. The proof treats zero voltage drops directly: second differences handle p<2, while an active quadratic energy and a zero-drop energy of order p handle p>2. For a three-terminal star with sorted weights A≥B≥C>0, the best uniform pairwise approximation error on boundary data of oscillation at most one is comparable, with constants depending only on p, to C(B/A)^(1/(p−1)). For fixed positive weights it has a strictly positive first-order coefficient in |p−2|. We also give first-order weak-arm limits and transfer the estimates to stars whose arms are arbitrary two-terminal networks.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-03
DOI
https://doi.org/10.5281/zenodo.23918413
Primary Topic
Geometric Analysis and Curvature Flows
Type
preprint
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preprint

Pairwise closure of power-law resistor networks and sharp three-terminal elimination defects

Zihuan Xu
Zenodo (CERN European Organization for Nuclear Research)
Geometric Analysis and Curvature Flows
preprint

Pairwise closure of power-law resistor networks and sharp three-terminal elimination defects

Zihuan Xu
preprint en

Abstract

We characterize when eliminating the interior vertices of a finite positive-weight power-law resistor network preserves an energy given by a sum of pairwise terms with the same exponent. For every fixed 1<p<∞, p≠2, this holds exactly when each connected component of the interior graph meets at most two boundary vertices. The criterion is independent of the positive weights. The proof treats zero voltage drops directly: second differences handle p<2, while an active quadratic energy and a zero-drop energy of order p handle p>2. For a three-terminal star with sorted weights A≥B≥C>0, the best uniform pairwise approximation error on boundary data of oscillation at most one is comparable, with constants depending only on p, to C(B/A)^(1/(p−1)). For fixed positive weights it has a strictly positive first-order coefficient in |p−2|. We also give first-order weak-arm limits and transfer the estimates to stars whose arms are arbitrary two-terminal networks.

Zenodo (CERN European Organization for Nuclear Research)
Capital Normal University (CN)
Geometric Analysis and Curvature Flows
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Pairwise closure of power-law resistor networks and sharp three-terminal elimination defects — Zihuan Xu · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS