Alphabeta Math
RemarkRemark: AI-adaptedProof: Not applicable
How statement and proof provenance work

The first chip identifies the source of the statement or construction; the second identifies the source of its local proof or verification.

  • Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
  • AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
  • AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.

These labels describe origin, not correctness: citations and verification chips remain separate evidence.

Introductory Harrison asymptotic claims

PDF p. 6: §1.4, first two paragraphs

Statement

In the article's mass-one stationary vacuum setting, with the chosen Harrison family, §1.4 (PDF p.6) prints the spatial one-form estimate (Wq)i=(q+r−1)O(r−3), and the uniform denominator expression Dq=4(q+r−1)2(1+O5(r−1)) for q∈[0,1]. It states that every gq for q>0 is asymptotically flat in normalized coordinates tq≍t/q, xq=qx, and that these ends recede to infinity in the original spacetime coordinates. It also states that g0 is no longer asymptotically flat and that its spatial sections are asymptotically cylindrical with limiting area 4π.

These are preserved as attributed introductory claims. The one-form order differs from the detailed §2.3 estimate on PDF p.10, (Wq)i=(1−q)2(W0)i−4q(1−q)g0i=(q+r−1)O5(r−2). The latter follows from the chosen primitive bound (W0)i=O5(r−3) and g0i=O6(r−2), through the local weighted-decay lemma. At q=0 the introductory expression asks for O(r−4), whereas this detailed argument supplies O5(r−3). The extra order in the introductory formula remains unestablished here: neither a proof of it nor a geometric counterexample under the article's complete hypotheses is supplied. The two formulas are retained distinctly; this remark is not a supplier for the stronger estimate and does not assert an article defect.

For the denominator, coordinate and spatial-limit mechanisms, the five local lemmas give complete conditional calculations from the explicitly supplied end, normalized potential and primitive bounds. Under those hypotheses, the positive-parameter normalization lemma establishes an asymptotically flat designated spacetime end for each fixed q>0. At q=0, the cylinder lemma establishes the asymptotically cylindrical geometry of the specified spatial coordinate sections and their limiting coordinate-sphere area; this spatial calculation alone does not establish the broader assertion excluding every possible asymptotically flat spacetime end or slicing. The exact positive-parameter time normalization is tq=dqt/(4q), not just a choice up to scale; the same pole-evaluation constant dq=Dq(p) used in the one-form contraction is required. The O5 constants for normalized coordinates are controlled on q∈[δ,1] with δ>0 fixed. A fixed rq=R represents original radius R/q, while q=0 is handled directly in the original spatial coordinates, not by substituting zero in tq,xq.

Facts & Assumptions

[F1]

Differentiated asymptotic bounds and parameter uniformity defines differentiated Cartesian bounds and the distinction between fixed-parameter and uniform estimates. Stationary Harrison one-form and metric and Mass-one convention and Harrison denominator fix the tensor, contraction and mass-one pole normalization.

[F2]

Smooth invariant Harrison primitive near the horizon and at infinity supplies the radial end primitive with (W0)i=O5(r−3), and Regular Harrison Einstein–Maxwell family supplies the chosen polynomial family Wq=(1−q)2W0−4q(1−q)T♭, under their precise recorded mass-one GR/SBS and original maximality hypotheses. Those hypotheses remain attached to these existence inputs; no broader existence conclusion is inferred from the formal calculations.

[F3]

Mass-one Ernst decay and uniform Harrison denominator bounds establishes the normalized potential and uniform denominator estimates from the stated stationary mass-one end and supplied Ernst equation. The differentiated spatial decay supplied by the Harrison lift proves the detailed one-form order with no additional cancellation assumption.

[F4]

Uniform spatial components and the cylinder scale estimates the spatial metric, Positive-parameter normalized time and spatial ends gives the exact positive-parameter normalization and its parameter range, and The zero-parameter spatial cylinder and its limiting area gives the zero-parameter spatial cylinder and limiting coordinate-sphere area.

Justification

Given: The attributed introductory formulas and the declared end data and suppliers.

Goal: Explain the conditional calculations and the limits of the stronger printed estimate.

1.1 The introductory formulas and their detailed counterpart are source-attribution content, not imported premises proving themselves. The one-form comparison in [F3] identifies exactly the additional decay requested at zero parameter, and leaves it unresolved without promoting the scalar non-implication example to a spacetime counterexample. [given, F1, F2, F3]

2.1 The denominator and the end conclusions in [F3]–[F4] are conditional consequences of explicit end data and the supplied primitive; [F2] records the scope in which the independently authored construction provides that primitive. They do not infer a new, stronger one-form bound or a weaker construction hypothesis. In particular, the normalized component bounds in [F4] establish an asymptotically flat designated end for every fixed q>0; at q=0, [F4] establishes the cylinder only for the specified spatial sections. The article's assertion that g0 is no longer asymptotically flat is retained as attribution; the spatial calculation alone does not exclude every other possible spacetime end or slicing. Radu's independent §3.3 (3.28) prints the same mass-one normalized potential expansion, and (3.19) with the subsequent normalized time gives τ=dqt/4 and s=τ/q, matching the exact time scale used here. Those passages are contextual comparison, not an extra unrecorded logical input. Accordingly all introductory claims, including the stronger printed one-form order, remain visible with their distinct evidence and limits. [F2, F3, F4, step 1.1] ∎

Depends on

Dependency tree · 2 levels

Each result is drawn at its shortest distance from this item. Arrows run from prerequisites to the items that use them; this item has a heavier outline. External source nodes link directly to the cited text. The view shows up to two dependency steps; open a prerequisite to continue.

External dependencies

Alexandru F. Radu, Rigidity of stationary black holes with small ADM angular momentum · §1.1 (1.1); §3.2 (3.19); §3.3 (3.28)–(3.29)

For comparison only, (3.28) prints $\sigma=1-2/r+O_6(r^{-2})$. Equation (3.19) sets $\tau=D_q(p)t/4$; the following sentence sets $s=\tau/q$ for $q>0$. After (3.29), $x'=qx$ accompanies this unit asymptotic time. With the local notation $d_q=D_q(p)$, these are the potential expansion and exact time normalization compared in Justification 2.1.

Hypotheses: Radu v1, smooth stationary vacuum spacetime under GR, SBS and original maximality (§1.1), rescaled to M=1; normalized Ernst potential, chosen horizon pole p, and fixed q>0 for unit asymptotic time. No angular-momentum smallness is used in these comparisons.

Reading limits: Retrieved v1 HTML; read §1.1, (3.19) and its following sentence, and (3.28)–(3.29) with adjacent paragraphs. Use is limited to the displayed comparison. No proof audit, stronger decay, or additional theorem is imported.

Sources