Metadata
bibkey: bauschkedeutschhundal2007alternating
authors: Heinz H. Bauschke, Frank Deutsch, Hein Hundal
year: 2007
title: Characterizing arbitrarily slow convergence in the method of alternating projections
doi: null
url: https://arxiv.org/pdf/0710.2387v1
claim: For two closed linear subspaces of a real or complex Hilbert space, the actual projection-product powers converge in norm on each vector to the intersection projection.
strata_touched: []
license: arXiv assumed-1991-2003; citation only
triage: anchor
Alternating orthogonal projections
Theorem 1.1 on printed page 1 of arXiv:0710.2387v1 states the classical von Neumann two-subspace strong convergence theorem. The ambient Hilbert space is real or complex, the subspaces are closed and linear, and the conclusion concerns the unaveraged projection-product powers on every vector. No positive Friedrichs angle, finite dimension, separability or convergence rate is required. Theorem 1.2 and the following discussion concern additional operator-norm and rate statements, which are distinct from pointwise strong convergence.
C. Badea, S. Grivaux and V. Müller, The rate of convergence in the method of alternating projections, arXiv:1006.2047v1, equation (1.1) on page 1, also states the strong convergence formula; its subsequent discussion distinguishes convergence in operator norm and angle-dependent rates.
The Lean proof uses the pinned Mathlib orthogonal-projection and mean ergodic theorems directly. Projection energy gives asymptotic regularity. A fixed finite averaging window then transfers Cesàro convergence to convergence of the actual powers. This is a proof of established mathematics. The citations supply the classical statement; no external Lean source or article text is copied, and the original von Neumann publication is not the source of a direct quotation here.
Verified locator
https://arxiv.org/pdf/0710.2387v1, printed page 1, Theorem 1.1: the classical von Neumann two-subspace strong convergence theorem for closed linear subspaces of a real or complex Hilbert space.