Neutron star phase sequence
Neutron star phase sequence: a one-parameter family of inequality crossings parameterized by density rho: crystal -> drip (mu_n > 0) -> pasta (theta varies) -> core (kappa drops); each arrow is an inequality crossing in defect-tuple space.
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.P55
- Type: proposition
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 4 · Chapter 33
Result summary
Neutron star phase sequence: a one-parameter family of inequality crossings parameterized by density rho: crystal -> drip (mu_n > 0) -> pasta (theta varies) -> core (kappa drops); each arrow is an inequality crossing in defect-tuple space.
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: neutron
- candidate is better handled as evidence for an inferred existing public surface
Review notes
- No additional review notes recorded.