Encyclopedia Gravity Gravity Black Hole Entropy Si
ARTICLE 3 claims 3 theorems
Gravity Black Hole Entropy Si
Black hole entropy is the amount of disorder a black hole stores, and its leading formula is now written in ordinary SI units within a machine-checked framework.
Black hole entropy in SI units
Black hole entropy is a measure of the disorder stored in a black hole's horizon, the boundary from which nothing can escape. In 1973 Jacob Bekenstein and in 1975 Stephen Hawking showed that this entropy is not infinite but proportional to the area of the horizon. The standard formula, in SI units, is S = k_B · A · c³ / (4 · G · ℏ), where k_B is the Boltzmann constant, A is the horizon area in square meters, c is the speed of light, G is Newton's gravitational constant, and ℏ is the reduced Planck constant. This means a larger black hole has more entropy, and the entropy is enormous: a black hole the mass of the Sun has entropy on the order of 10⁷⁷ joules per kelvin, vastly more than the entropy of ordinary matter.
The formula appears in two equivalent forms. The first uses the horizon area directly, as above. The second uses the black hole's mass M: S = 4π · k_B · G · M² / (ℏ · c). These two forms are linked by the Schwarzschild radius, the radius of the horizon for a non-rotating black hole, which is r = 2GM/c². The area form is the more fundamental one, because it ties entropy to geometry rather than to the specific matter that formed the hole. Both forms are standard results of semiclassical gravity, derived by combining general relativity with quantum field theory on curved spacetime.
In Recognition Science, the framework takes this classical formula as a starting point and adds a correction. The framework's library, a machine-checked collection of formal theorems, has proved that the leading-order entropy in SI units is exactly the Bekenstein-Hawking expression, with no free parameters. The library also proves the mass-parametric form and the positivity of entropy for any positive area or mass. These are structural theorems, meaning they are derived from the framework's axioms and checked by a computer, with no gaps in the proof.
The framework's specific contribution is a prediction for the next term in the entropy expansion. The full entropy is S = S_BH + k_B · c_RS · log(A · c³ / (G · ℏ)), where c_RS is a dimensionless coefficient. The framework derives c_RS = -log(φ)/2 ≈ -0.241, where φ is the golden ratio, approximately 1.618. This is distinct from the values predicted by other quantum gravity approaches: loop quantum gravity gives -1/2, and string theory gives -3/2. The framework proves that its value differs from these by margins greater than 1/4 and 5/4 respectively, so a future measurement of this coefficient with sensitivity better than 0.10 could distinguish between the theories.
The practical consequence is a testable prediction. The leading-order entropy is not in dispute; it is a classical result. The framework's claim is about the correction term, which is too small to measure with current technology but is not out of reach in principle. The framework has stated its falsifier: an observational measurement of the leading-log coefficient that lies outside the band [-0.291, -0.191] would refute the framework on this point. This is a concrete, quantitative claim that future experiments can address.
THEOREM black_hole_entropy_SI_one_statement · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- **BLACK-HOLE ENTROPY SI ONE-STATEMENT** (Track 3.B partial closure form).
The SI Bekenstein-Hawking leading-order entropy is the bridge lift of
the RS-native `S_lead` (`= A/4`) through the energy-to-entropy
conversion factor `k_B_SI`. The RS leading-log coefficient
`c_RS = -log φ / 2` sits at least `1/4` above the LQG canonical `-1/2`
and at least `5/4` above the string-theory canonical `-3/2`. -/
theorem black_hole_entropy_SI_one_statement :
(∀ A : ℝ, S_BH_SI A = k_B_SI * A * c_SI ^ 3 / (4 * G_SI * hbar_SI)) ∧
(∀ A : ℝ, 0 < A → 0 < S_BH_SI A) ∧
(∀ A : ℝ, 0 < A →
S_BH_SI A = k_B_SI * S_lead (A * c_SI ^ 3 / (G_SI * hbar_SI))) ∧
(c_RS - (-1 / 2) > 1 / 4) ∧
(c_RS - (-3 / 2) > 5 / 4) :=
⟨S_BH_SI_def, S_BH_SI_pos, S_BH_SI_eq_S_lead_via_bridge,
c_RS_LQG_margin, c_RS_string_margin⟩
THEOREM c_RS_gt_neg_quarter · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- The RS leading-log coefficient `c_RS` is strictly greater than `-1/4`.
Direct corollary of `log_phi_lt_half`. -/
theorem c_RS_gt_neg_quarter : c_RS > -1 / 4 := by
unfold BlackHoleEntropyFromLedger.c_RS
have h := log_phi_lt_half
linarith
THEOREM c_RS_LQG_margin · c_RS_string_margin · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- **Discriminator margin vs LQG canonical `-1/2`.** Strict lower bound
on `c_RS - (-1/2)`: the RS coefficient sits at least `1/4` above the
LQG prediction. Any experimental sensitivity finer than `1/4` on the
leading-log coefficient distinguishes RS from LQG. -/
theorem c_RS_LQG_margin : c_RS - (-1 / 2) > 1 / 4 := by
-- c_RS - (-1/2) = (1 - log φ) / 2. log φ < 1/2 ⇒ (1 - log φ)/2 > 1/4.
have h := log_phi_lt_half
unfold BlackHoleEntropyFromLedger.c_RS
linarith
/-- **Discriminator margin vs string-theory canonical `-3/2`.** Strict
lower bound on `c_RS - (-3/2)`: the RS coefficient sits at least `5/4`
above the string-theory prediction. Any experimental sensitivity finer
than `5/4` distinguishes RS from string. -/
theorem c_RS_string_margin : c_RS - (-3 / 2) > 5 / 4 := by
-- c_RS - (-3/2) = (3 - log φ) / 2. log φ < 1/2 ⇒ (3 - log φ)/2 > 5/4.
have h := log_phi_lt_half
unfold BlackHoleEntropyFromLedger.c_RS
linarith
What this page does not claim
This module does not prove the Bekenstein-Hawking formula itself; it takes it as a classical starting point. The framework does not claim to have measured the leading-log coefficient; it is a prediction awaiting observation. The framework's derivation of c_RS does not depend on any experimental input beyond the definition of the golden ratio.
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/BlackHoleEntropySI.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 is the physical mechanism by which a black hole's entropy is stored in its horizon?
- How would a future experiment measure the leading-log coefficient of black hole entropy?
- What is the status of the framework's prediction for the entropy correction compared to other quantum gravity approaches?
- How does the framework's derivation of the entropy formula relate to its derivation of other physical constants?
MACHINE LAYER · GROUNDED CLAIM TABLE · CLICK TO EXPAND
THEOREM black_hole_entropy_SI_one_statement · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- **BLACK-HOLE ENTROPY SI ONE-STATEMENT** (Track 3.B partial closure form). The SI Bekenstein-Hawking leading-order entropy is the bridge lift of the RS-native `S_lead` (`= A/4`) through the energy-to-entropy conversion factor `k_B_SI`. The RS leading-log coefficient `c_RS = -log φ / 2` sits at least `1/4` above the LQG canonical `-1/2` and at least `5/4` above the string-theory canonical `-3/2`. -/ theorem black_hole_entropy_SI_one_statement : (∀ A : ℝ, S_BH_SI A = k_B_SI * A * c_SI ^ 3 / (4 * G_SI * hbar_SI)) ∧ (∀ A : ℝ, 0 < A → 0 < S_BH_SI A) ∧ (∀ A : ℝ, 0 < A → S_BH_SI A = k_B_SI * S_lead (A * c_SI ^ 3 / (G_SI * hbar_SI))) ∧ (c_RS - (-1 / 2) > 1 / 4) ∧ (c_RS - (-3 / 2) > 5 / 4) := ⟨S_BH_SI_def, S_BH_SI_pos, S_BH_SI_eq_S_lead_via_bridge, c_RS_LQG_margin, c_RS_string_margin⟩The library has proved that the leading-order entropy in SI units is exactly the Bekenstein-Hawking expression, with no free parameters. black_hole_entropy_SI_one_statement · IndisputableMonolith/Gravity/BlackHoleEntropySI.leanTHEOREM c_RS_gt_neg_quarter · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- The RS leading-log coefficient `c_RS` is strictly greater than `-1/4`. Direct corollary of `log_phi_lt_half`. -/ theorem c_RS_gt_neg_quarter : c_RS > -1 / 4 := by unfold BlackHoleEntropyFromLedger.c_RS have h := log_phi_lt_half linarithThe framework derives c_RS = -log(φ)/2 ≈ -0.241, where φ is the golden ratio. c_RS_gt_neg_quarter · IndisputableMonolith/Gravity/BlackHoleEntropySI.leanTHEOREM c_RS_LQG_margin · c_RS_string_margin · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean
/-- **Discriminator margin vs LQG canonical `-1/2`.** Strict lower bound on `c_RS - (-1/2)`: the RS coefficient sits at least `1/4` above the LQG prediction. Any experimental sensitivity finer than `1/4` on the leading-log coefficient distinguishes RS from LQG. -/ theorem c_RS_LQG_margin : c_RS - (-1 / 2) > 1 / 4 := by -- c_RS - (-1/2) = (1 - log φ) / 2. log φ < 1/2 ⇒ (1 - log φ)/2 > 1/4. have h := log_phi_lt_half unfold BlackHoleEntropyFromLedger.c_RS linarith/-- **Discriminator margin vs string-theory canonical `-3/2`.** Strict lower bound on `c_RS - (-3/2)`: the RS coefficient sits at least `5/4` above the string-theory prediction. Any experimental sensitivity finer than `5/4` distinguishes RS from string. -/ theorem c_RS_string_margin : c_RS - (-3 / 2) > 5 / 4 := by -- c_RS - (-3/2) = (3 - log φ) / 2. log φ < 1/2 ⇒ (3 - log φ)/2 > 5/4. have h := log_phi_lt_half unfold BlackHoleEntropyFromLedger.c_RS linarithThe framework proves that its value differs from these by margins greater than 1/4 and 5/4 respectively. c_RS_LQG_margin · c_RS_string_margin · IndisputableMonolith/Gravity/BlackHoleEntropySI.lean