Encyclopedia Gravity Gravity Planck Star From Jcost
ARTICLE 4 claims 4 theorems
Gravity Planck Star From Jcost
A Planck star is a proposed bounce of a collapsing black hole; the framework's module proves only general properties of its cost function, not the bounce.
Planck star bounce
A Planck star is a hypothetical object proposed in loop quantum gravity and related approaches: instead of a collapsing black hole ending in a singularity, quantum effects become strong near the Planck length and halt the collapse, producing a bounce that could later explode. The name comes from the Planck scale, roughly 10-35 meters, where quantum gravity is expected to dominate. The idea is that the star's radius never shrinks below a minimum set by that scale.
In Recognition Science, the framework's module ledger (a discrete record of events) defines a cost function on ratios of two masses, J(m/e) = (m/e + e/m)/2 - 1, which measures how far the ratio is from unity. The module then proves three facts about this function: it equals zero when the two masses are equal, it is never negative for positive inputs, and the threshold phi - 3/2 is positive. These are general properties of the cost function, not specific to Planck stars.
The research note in the module records an intended application: a Planck star bounce at radius r_min = phi^(N/2) times the Planck length, with a bounce density rho_bounce = rho_Pl * phi^(-3N/2). For N = 100, that density is about 10^-50 times the Planck density. But the module itself does not define what m and e are in gravitational terms. The three proved facts hold for any positive masses, so they do not establish the bounce.
What the module does establish, in plain language, is a small certificate: a structure that packages the three cost properties and a proof that this structure is inhabited. That is a machine-checked guarantee that the cost function behaves as expected, not a derivation of Planck stars. The bounce remains a research direction, not a result.
THEOREM domainCost_at_eq · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem domainCost_at_eq (r : ℝ) (h : r ≠ 0) : domainCost r r = 0 := by
unfold domainCost; rw [div_self h]; exact Jcost_unit0
THEOREM domainCost_nonneg · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem domainCost_nonneg (m e : ℝ) (hm : 0 < m) (he : 0 < e) : 0 ≤ domainCost m e := by
unfold domainCost; exact Jcost_nonneg (div_pos hm he)
THEOREM canonicalThreshold_pos · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem canonicalThreshold_pos : 0 < canonicalThreshold := by
unfold canonicalThreshold; linarith [phi_gt_onePointFive]
THEOREM cert_inhabited · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem cert_inhabited : Nonempty PlanckStar3Cert := ⟨cert⟩
What this page does not claim
The module does not prove that Planck stars exist or that a bounce occurs. The module does not derive the bounce density or radius from the cost function. The framework's cost function alone does not force the Planck star scenario.
Verify this page
Every tagged claim above names its theorem. To check one yourself rather than trust this page, elaborate the source module with Lean 4 and audit its axiom basis:
$ lake env lean IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
expected axiom basis: [propext, Classical.choice, Quot.sound] (the Lean kernel's standard three; no RS-specific axioms)
A page whose claims cannot be reproduced this way does not ship. In production, every anchor links to the exact declaration in the public source release, and this block carries the build receipt for the page itself.
Derived articles
This page is generated by a question-recursion engine: the questions its answers raise become the next pages. The current agenda, with open targets marked red:
- What physical definition of m and e would turn the cost function into a theorem about Planck stars?
- How does the phi-ladder scaling relate to the Planck star bounce radius?
- What observational signature would distinguish a Planck star bounce from a classical black hole?
MACHINE LAYER · GROUNDED CLAIM TABLE · CLICK TO EXPAND
THEOREM domainCost_at_eq · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem domainCost_at_eq (r : ℝ) (h : r ≠ 0) : domainCost r r = 0 := by unfold domainCost; rw [div_self h]; exact Jcost_unit0The module defines a cost function on ratios of two masses, J(m/e) = (m/e + e/m)/2 - 1, and proves it equals zero when the two masses are equal. domainCost_at_eq · IndisputableMonolith/Gravity/PlanckStarFromJCost.leanTHEOREM domainCost_nonneg · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem domainCost_nonneg (m e : ℝ) (hm : 0 < m) (he : 0 < e) : 0 ≤ domainCost m e := by unfold domainCost; exact Jcost_nonneg (div_pos hm he)The module proves the cost function is never negative for positive inputs. domainCost_nonneg · IndisputableMonolith/Gravity/PlanckStarFromJCost.leanTHEOREM canonicalThreshold_pos · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem canonicalThreshold_pos : 0 < canonicalThreshold := by unfold canonicalThreshold; linarith [phi_gt_onePointFive]The module proves the threshold phi - 3/2 is positive. canonicalThreshold_pos · IndisputableMonolith/Gravity/PlanckStarFromJCost.leanTHEOREM cert_inhabited · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean
theorem cert_inhabited : Nonempty PlanckStar3Cert := ⟨cert⟩The module provides a certificate structure that packages these three cost properties and proves it is inhabited. cert_inhabited · IndisputableMonolith/Gravity/PlanckStarFromJCost.lean