Neutron node EW stability
In the carrier Star_n(C) with baryon count above the Chandrasekhar threshold, every interior neutron node is EW-stable. The stability is controlled by the weak-sector coupling kappa(A;1) = iota_tau: beta decay costs more energy than it releases when node density exceeds a critica
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.T43
- Type: theorem
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 2 · Chapter 17
Result summary
In the carrier Star_n(C) with baryon count above the Chandrasekhar threshold, every interior neutron node is EW-stable. The stability is controlled by the weak-sector coupling kappa(A;1) = iota_tau: beta decay costs more energy than it releases when node density exceeds a critical value.
Related Results surfaces
Reading role
Use as Registry evidence for an existing Results surface.
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: energy, neutron
- candidate is better handled as evidence for an inferred existing public surface
Review notes
- No additional review notes recorded.