No Shrink---restatement
In the tau-framework, the total boundary-character amplitude of a black hole region is non-decreasing. Black holes do not evaporate. Their Bekenstein-Hawking temperature T_H is a property of the readout layer, not a rate of mass loss. The No Shrink Theorem is restated: Hawking ra
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.T141
- Type: theorem
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 7 · Chapter 68
Result summary
In the tau-framework, the total boundary-character amplitude of a black hole region is non-decreasing. Black holes do not evaporate. Their Bekenstein-Hawking temperature T_H is a property of the readout layer, not a rate of mass loss. The No Shrink Theorem is restated: Hawking radiation has KMS structure from the omega-crossing but does not carry mass-energy away.
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: black, energy, mass, temperature
- result-facing terms: readout
- theorem/proposition-class item appears externally legible enough for standalone review
Review notes
- No additional review notes recorded.