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Distance of a standard Gaussian vector to a fixed subspace: if rank⁡B+d≤N\operatorname{rank}B+d\le NrankB+d≤N then P{dist⁡(g,col⁡B)2≤u}≤(eu/d)d/2\mathbb P\{\operatorname{dist}(g,\operatorname{col}B)^2\le u\}\le (eu/d)^{d/2}P{dist(g,colB)2≤u}≤(eu/d)d/2

Proved
GaussianMatrix.gaussian_dist_colspace_small_ball

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

chi-squaregaussianprojectionrotation-invariancesmall-ball

Let ggg be a standard Gaussian vector in RN\mathbb R^NRN (independent N(0,1)N(0,1)N(0,1) coordinates) and let BBB be a fixed real N×pN\times pN×p matrix with column space col⁡B⊆RN\operatorname{col}B\subseteq\mathbb R^NcolB⊆RN. Let d≥1d\ge1d≥1 be an integer with rank⁡B+d≤N\operatorname{rank}B+d\le NrankB+d≤N, and let

dist⁡(g,col⁡B)=inf⁡c∈Rp∥g−Bc∥2.\operatorname{dist}(g,\operatorname{col}B)=\inf_{c\in\mathbb R^p}\|g-Bc\|_2 .dist(g,colB)=c∈Rpinf​∥g−Bc∥2​.

Then for every real uuu with 0≤u≤d0\le u\le d0≤u≤d,

P{dist⁡(g,col⁡B)2≤u}  ≤  (e ud)d/2.\mathbb P\big\{\operatorname{dist}(g,\operatorname{col}B)^2\le u\big\}\;\le\;\Big(\frac{e\,u}{d}\Big)^{d/2}.P{dist(g,colB)2≤u}≤(deu​)d/2.

Choose orthonormal vectors w1,…,wdw_1,\dots,w_dw1​,…,wd​ in (col⁡B)⊥(\operatorname{col}B)^\perp(colB)⊥ (possible since its dimension is N−rank⁡B≥dN-\operatorname{rank}B\ge dN−rankB≥d). By Bessel's inequality, ∥g−Bc∥2≥∑k≤d⟨wk,g−Bc⟩2=∑k≤d⟨wk,g⟩2\|g-Bc\|^2\ge\sum_{k\le d}\langle w_k,g-Bc\rangle^2=\sum_{k\le d}\langle w_k,g\rangle^2∥g−Bc∥2≥∑k≤d​⟨wk​,g−Bc⟩2=∑k≤d​⟨wk​,g⟩2 for every ccc. By rotation invariance of the standard Gaussian, (⟨wk,g⟩)k≤d(\langle w_k,g\rangle)_{k\le d}(⟨wk​,g⟩)k≤d​ is a standard Gaussian vector in Rd\mathbb R^dRd, so the probability is at most P{χd2≤u}≤(eu/d)d/2\mathbb P\{\chi^2_d\le u\}\le(eu/d)^{d/2}P{χd2​≤u}≤(eu/d)d/2.

This is the fixed-subspace ingredient for small-ball estimates of the smallest singular value: applied conditionally on the other columns of a Gaussian matrix, it controls the distance of one column to the span of the others.

Formalization Note. The law of ggg is Measure.pi fun _ : Fin N => gaussianReal 0 1; ∥v∥2\|v\|_2∥v∥2​ is Real.sqrt (v ⬝ᵥ v); B.rank is Mathlib's Matrix.rank. The case p=0p=0p=0 (trivial subspace) is included.

Preamble
import Definitions.Def_GaussianMatrix_basic

open MeasureTheory ProbabilityTheory
open scoped Matrix
Formal statement
namespace GaussianMatrix

theorem gaussian_dist_colspace_small_ball {N p d : ℕ} (B : Matrix (Fin N) (Fin p) ℝ)
    (hd : 1 ≤ d) (hrank : B.rank + d ≤ N) (u : ℝ) (hu : 0 ≤ u) (hud : u ≤ d) :
    (Measure.pi fun _ : Fin N => gaussianReal 0 1)
      {g | (⨅ c : Fin p → ℝ, Real.sqrt ((g - B *ᵥ c) ⬝ᵥ (g - B *ᵥ c))) ^ 2 ≤ u}
      ≤ ENNReal.ofReal ((Real.exp 1 * u / d) ^ ((d : ℝ) / 2)) := by sorry

end GaussianMatrix
Source
standard fact: if V ⊆ R^N is a fixed subspace of dimension ρ and g is standard Gaussian, then ‖P_{V^⊥} g‖² ~ χ²_{N−ρ}; with the χ² lower tail P{χ²_d ≤ u} ≤ (eu/d)^{d/2} for 0 ≤ u ≤ d (Laurent–Massart, Ann. Statist. 28 (2000), Lemma 1, or a Chernoff bound).

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