Proof of Theorem 3.1, p. 13 — for
ProvedSphereGRF.Spectral.factorial_ratio_boundsasymptoticsfactorialp2o-batch-pfp2ap2o-gran-per-chapterp2o-plan-paperp2o-v1stirling-formula
For every there are constants such that for all with ,
The ratio is the squared weighted norm of up to the factor ; the bound converts the weighted Parseval identity into the polynomial weight of the sequence space .
Formalization Note is a natural power with , so the case reads . The constants are chosen before .
Preamble
import Mathlib
Formal statement
namespace SphereGRF.Spectral
/-- Proof of Theorem 3.1, p. 13: for every `n` there are `c₁(n), c₂(n) > 0` with
`c₁(n) ℓ^{2n} ≤ (ℓ+n)!/(ℓ−n)! ≤ c₂(n) ℓ^{2n}` for all `ℓ ≥ n`. -/
theorem factorial_ratio_bounds (n : ℕ) :
∃ c₁ c₂ : ℝ, 0 < c₁ ∧ 0 < c₂ ∧ ∀ ℓ : ℕ, n ≤ ℓ →
c₁ * (ℓ : ℝ) ^ (2 * n) ≤ ((ℓ + n).factorial : ℝ) / ((ℓ - n).factorial : ℝ) ∧
((ℓ + n).factorial : ℝ) / ((ℓ - n).factorial : ℝ) ≤ c₂ * (ℓ : ℝ) ^ (2 * n) := by sorry
end SphereGRF.Spectral
Source
Lang, Schwab, Isotropic Gaussian random fields on the sphere, arXiv:1305.1170v3, §3, proof of Theorem 3.1, p. 13, display following 'there exist constants c1(n) and c2(n) such that'
Human review
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.