Newtonian limit recovery
In the weak-field, slow-motion regime, the chart shadow of the linearized tau-Einstein equation is the Newtonian gravitational equation nabla^2 Phi = 4 pi G rho, where G = (c^3/hbar) iota_tau^2. Newton's force law F = -m nabla Phi follows immediately.
What this page is
This is a public Results-lane surface for a noteworthy Physics Registry item. It is generated from the Corpus Registry triage catalogue and keeps the generic Result catalogue unchanged.
Registry evidence
- Registry item: V.T28
- Type: theorem
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 2 · Chapter 14
Result summary
In the weak-field, slow-motion regime, the chart shadow of the linearized tau-Einstein equation is the Newtonian gravitational equation nabla^2 Phi = 4 pi G rho, where G = (c^3/hbar) iota_tau^2. Newton’s force law F = -m nabla Phi follows immediately.
Related Results surfaces
- No existing public Results surface is linked yet; this record is promoted as a standalone Registry-backed result.
Reading role
Read as a standalone Registry-backed noteworthy result.
Claim boundary
This page reports a Registry-backed internal result surface. It is not an external validation claim, a scientific consensus claim, or independent acceptance.
Curation rationale
- physics-facing terms: gravitational, shadow
- result-facing terms: law
- theorem/proposition-class item appears externally legible enough for standalone review
Review notes
- No additional review notes recorded.