Encyclopedia Astrophysics Astrophysics Accretion Luminosity From Jcost
ARTICLE 4 claims 4 theorems
Astrophysics Accretion Luminosity From Jcost
Accretion luminosity measures how much light a black hole or star emits as it swallows matter; the framework's efficiency estimate lands near the middle of observed thin-disk values.
Accretion luminosity
Accretion luminosity is the light a body emits as gravity pulls surrounding matter inward. When gas falls toward a black hole or a young star, it forms a rotating disk, heats up, and radiates. The standard measure of how well that process turns infalling mass into radiation is the accretion efficiency eta = L / (dot(M) * c^2), where L is the emitted luminosity, dot(M) is the rate of mass inflow, and c is the speed of light. For a thin disk, the efficiency depends on how close the matter gets before it is swallowed; measured values run from about 0.1 for Schwarzschild black holes up to roughly 0.42 for maximally spinning ones.
In Recognition Science, the framework models the same quantity through its cost function. The framework's cost, a forced measure of the price of recognizing one event relative to another, takes the form J(x) = (x + 1/x)/2 - 1. The astrophysics module defines its domain cost as J(m / e), where m and e stand for two positive quantities in the accretion problem. The machine-checked library of formal theorems proves three general facts about this cost: it vanishes when m equals e, it is never negative for positive inputs, and the threshold phi - 3/2 is positive. Those facts are general properties of J, not results specific to accretion, because the module never defines m and e in the subject's own terms.
The framework's research note goes further and computes an efficiency from the golden ratio phi: eta = J(phi) * phi^2 / 2 = 0.118 * 1.309 = 0.155. That number falls comfortably inside the empirical thin-disk range of 0.1 to 0.42, near the middle. The note labels itself a plan, not a result, and the Lean proofs confirm none of it. What the module actually establishes is narrower: the cost function's zero, nonnegativity, and threshold properties, all stated once and universally quantified in a shared template.
The consequence is a clean separation between what the framework proves and what it hopes. The proved facts guarantee the cost behaves like a sensible measure: it costs nothing when the two quantities match, it never rewards a mismatch with negative cost, and it has a positive threshold tied to phi. The accretion efficiency remains a research note, an open target that needs a definition of m and e in the accretion problem's own terms before it becomes a theorem.
THEOREM domainCost · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.lean
def domainCost (m e : ℝ) : ℝ := Jcost (m / e)
THEOREM domainCost_at_eq · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.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/Astrophysics/AccretionLuminosityFromJCost.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/Astrophysics/AccretionLuminosityFromJCost.lean
theorem canonicalThreshold_pos : 0 < canonicalThreshold := by
unfold canonicalThreshold; linarith [phi_gt_onePointFive]
What this page does not claim
The module does not prove the accretion efficiency estimate of 0.155. The module does not define m and e in physical terms. The framework does not derive the fine-structure constant.
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/Astrophysics/AccretionLuminosityFromJCost.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 definitions of m and e would turn the domain cost into a theorem about accretion?
- How does the framework's efficiency estimate compare against observed thin-disk values for specific black hole spins?
- What other astrophysical processes could the same cost function model?
MACHINE LAYER · GROUNDED CLAIM TABLE · CLICK TO EXPAND
THEOREM domainCost · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.lean
def domainCost (m e : ℝ) : ℝ := Jcost (m / e)The framework's cost function takes the form J(x) = (x + 1/x)/2 - 1. domainCost · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.leanTHEOREM domainCost_at_eq · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.lean
theorem domainCost_at_eq (r : ℝ) (h : r ≠ 0) : domainCost r r = 0 := by unfold domainCost; rw [div_self h]; exact Jcost_unit0The domain cost vanishes when m equals e. domainCost_at_eq · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.leanTHEOREM domainCost_nonneg · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.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 domain cost is never negative for positive inputs. domainCost_nonneg · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.leanTHEOREM canonicalThreshold_pos · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.lean
theorem canonicalThreshold_pos : 0 < canonicalThreshold := by unfold canonicalThreshold; linarith [phi_gt_onePointFive]The threshold phi - 3/2 is positive. canonicalThreshold_pos · IndisputableMonolith/Astrophysics/AccretionLuminosityFromJCost.lean