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Eq. (34): AdS black-hole entropy grows like M(d−2)/(d−1)M^{(d-2)/(d-1)}M(d−2)/(d−1)

Proved
GravityNonRenorm.ads_bh_entropy_eq34

by Lucas · Oct 9, 2026 · Mathlib 0df444a (Lean v4.33.1)

black-holesquantum-gravity

Let d≥3d\ge3d≥3, GN>0G_N>0GN​>0 and RAdS>0R_{\rm AdS}>0RAdS​>0. For each mass MMM let rH(M)r_H(M)rH​(M) be the largest positive zero of the Schwarzschild–AdS metric function

f(r)=1−ωd−2GNMrd−3+r2RAdS2,f(r)=1-\frac{\omega_{d-2}G_NM}{r^{d-3}}+\frac{r^2}{R_{\rm AdS}^2},f(r)=1−rd−3ωd−2​GN​M​+RAdS2​r2​,

and let SAdS(M)=Vol(Sd−2) rH(M)d−2/(4GN)S_{\rm AdS}(M)=\mathrm{Vol}(S^{d-2})\,r_H(M)^{d-2}/(4G_N)SAdS​(M)=Vol(Sd−2)rH​(M)d−2/(4GN​). Then, as M→∞M\to\inftyM→∞,

SAdS(M)=Θ ⁣(Md−2d−1).S_{\rm AdS}(M)=\Theta\!\left(M^{\frac{d-2}{d-1}}\right).SAdS​(M)=Θ(Md−1d−2​).

This is Eq. (34): large AdS black holes have entropy growing like M(d−2)/(d−1)M^{(d-2)/(d-1)}M(d−2)/(d−1).

Preamble
import Definitions.Def_GravityNonRenorm_Defs
import Mathlib

open GravityNonRenorm Filter Asymptotics
Formal statement
namespace GravityNonRenorm
theorem ads_bh_entropy_eq34 (d : ℕ) (hd : 3 ≤ d) (G RAdS : ℝ) (hG : 0 < G) (hRAdS : 0 < RAdS) :
    (fun M : ℝ => adsBHEntropy d G M RAdS) =Θ[atTop]
      (fun M : ℝ => M ^ (((d : ℝ) - 2) / ((d : ℝ) - 1))) := by sorry
end GravityNonRenorm
Source
Assaf Shomer, A pedagogical explanation for the non-renormalizability of gravity, arXiv:0709.3555v2 [hep-th] (2007), https://arxiv.org/abs/0709.3555
Read-back

What the Lean code literally says, in plain math · Aristotle (Harmonic)

Non-blind read-back — not independent testimony. This read-back was written by the same agent that drafted the Lean statement (at the explicit request of the proposal owner), not by a blind, independent auditor. The author knew the intended meaning and the source paper while writing it, so it must not be mistaken for independent testimony; reviewers should compare it against the Lean code themselves.

For every natural number d≥3d\ge3d≥3 and all reals G>0G>0G>0, RAdS>0R_{\rm AdS}>0RAdS​>0, the function M↦adsBHEntropy(d,G,M,RAdS)M\mapsto\mathrm{adsBHEntropy}(d,G,M,R_{\rm AdS})M↦adsBHEntropy(d,G,M,RAdS​) is Θ\ThetaΘ of M↦M(d−2)/(d−1)M\mapsto M^{(d-2)/(d-1)}M↦M(d−2)/(d−1) as M→+∞M\to+\inftyM→+∞ (exponent computed in the reals, real power). Unfolded, adsBHEntropy(d,G,M,RAdS)=sphereArea(d−2) rHd−2/(4G)\mathrm{adsBHEntropy}(d,G,M,R_{\rm AdS})=\mathrm{sphereArea}(d-2)\,r_H^{d-2}/(4G)adsBHEntropy(d,G,M,RAdS​)=sphereArea(d−2)rHd−2​/(4G) where rHr_HrH​ is the real supremum of {r>0: 1−ωd−2GM/rd−3+r2/RAdS2=0}\{r>0:\ 1-\omega_{d-2}GM/r^{d-3}+r^2/R_{\rm AdS}^2=0\}{r>0: 1−ωd−2​GM/rd−3+r2/RAdS2​=0} (value 000 if that set is empty or unbounded). For d=3d=3d=3 the power rd−3r^{d-3}rd−3 is r0=1r^0=1r0=1, so the defining equation becomes 1−ω1GM+r2/RAdS2=01-\omega_1GM+r^2/R_{\rm AdS}^2=01−ω1​GM+r2/RAdS2​=0. Here f=Θ(g)f=\Theta(g)f=Θ(g) as x→∞x\to\inftyx→∞ (Mathlib's IsTheta along atTop) means: there are constants c1,c2>0c_1,c_2>0c1​,c2​>0 and x0x_0x0​ such that ∣f(x)∣≤c1∣g(x)∣|f(x)|\le c_1|g(x)|∣f(x)∣≤c1​∣g(x)∣ and ∣g(x)∣≤c2∣f(x)∣|g(x)|\le c_2|f(x)|∣g(x)∣≤c2​∣f(x)∣ for all x≥x0x\ge x_0x≥x0​.

Human review
  • Endorsed by Shuze Chen · Oct 10, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Lucas · Oct 10, 2026

    Confirmed by the mission captain (proposal self-audit).

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