OAI/Analysis/OInfinity/ToeplitzCompression.lean
11 declarations, 0 contain sorry, 0 declared as axioms
Finite Toeplitz rows compressed by an almost central projection
These are the quantitative estimates in the projection-splitting step for a finite row of canonical O∞ isometries. In addition to almost centrality, a coisometric compression needs small compression of the original vacuum projection. No projection with these properties is assumed to exist here.
- def
OAI.WeakPureInfiniteness.toeplitzRowCompressionline 21Source documentation
Compression in the ambient algebra, with relative unit
q.def toeplitzRowCompression (q : E) (s : I → E) (i : I) : E := q * s i * q
- def
OAI.WeakPureInfiniteness.toeplitzRowVacuumline 24Source documentation
The defect of the finite isometry row before compression.
def toeplitzRowVacuum (s : I → E) : E := 1 - ∑ i, s i * star (s i)
- lemma
OAI.WeakPureInfiniteness.compression_projection_normline 26 - lemma
OAI.WeakPureInfiniteness.compression_contract_mul_leftline 30 - lemma
OAI.WeakPureInfiniteness.compression_contract_mul_rightline 34 - lemma
OAI.WeakPureInfiniteness.toeplitz_star_commutator_normline 39Source documentation
The adjoint has the same commutator error.
lemma toeplitz_star_commutator_norm (q x : E) (hqs : star q = q) : ‖q * star x - star x * q‖ = ‖q * x - x * q‖ := by … - lemma
OAI.WeakPureInfiniteness.toeplitzRowCompression_gramline 48Source documentation
Exact defect formula for the compressed Gram matrix.
lemma toeplitzRowCompression_gram (q : E) (s : I → E) (hq : q * q = q) (hqs : star q = q) (hs : ∀ i j, star (s i) * s j = if i = j then 1 else 0) (i j : I) : star (toeplitzRowCompression q s i) * toeplitzRowCompression q s j - (if i = j then q else 0) = q * star (s i) * (q * s j - s j * q) * q := by … - lemma
OAI.WeakPureInfiniteness.toeplitzRowCompression_gram_boundline 66Source documentation
Every Gram entry is controlled by one generator commutator.
lemma toeplitzRowCompression_gram_bound (q : E) (s : I → E) (hq : q * q = q) (hqs : star q = q) (hs : ∀ i j, star (s i) * s j = if i = j then 1 else 0) (hns : ∀ i, ‖s i‖ ≤ 1) (δ : ℝ) (hcomm : ∀ i, ‖q * s i - s i * q‖ ≤ δ) (i j : I) : ‖star (toeplitzRowCompression q s i) * toeplitzRowCompression q s j - (if i = j then q else 0)‖ ≤ δ := by … - lemma
OAI.WeakPureInfiniteness.toeplitzRowCompression_coisometryline 87Source documentation
The coisometry defect contains the compressed original vacuum explicitly.
lemma toeplitzRowCompression_coisometry (q : E) (s : I → E) (hq : q * q = q) (hqs : star q = q) : (∑ i, toeplitzRowCompression q s i * star (toeplitzRowCompression q s i)) - q = (∑ i, q * s i * (q * star (s i) - star (s i) * q) * q) - q * toeplitzRowVacuum s * q := by …Mentions: OAI.WeakPureInfiniteness.toeplitzRowCompression, OAI.WeakPureInfiniteness.toeplitzRowVacuum
- lemma
OAI.WeakPureInfiniteness.toeplitzRowCompression_coisometry_boundline 109Source documentation
Approximate centrality and small vacuum compression give the finite coisometry estimate used before perturbing a Toeplitz row to a Cuntz row.
lemma toeplitzRowCompression_coisometry_bound (q : E) (s : I → E) (hq : q * q = q) (hqs : star q = q) (hns : ∀ i, ‖s i‖ ≤ 1) (δ : ℝ) (hcomm : ∀ i, ‖q * s i - s i * q‖ ≤ δ) : ‖(∑ i, toeplitzRowCompression q s i * star (toeplitzRowCompression q s i)) - q‖ ≤ (Fintype.card I : ℝ) * δ + ‖q * toeplitzRowVacuum s * q‖ := by …Mentions: OAI.WeakPureInfiniteness.toeplitzRowCompression, OAI.WeakPureInfiniteness.toeplitzRowVacuum
- lemma
OAI.WeakPureInfiniteness.toeplitz_complementary_compression_boundline 137Source documentation
The two relative compressions recover each generator up to twice its commutator error. No smallness is asserted for either complementary projection.
lemma toeplitz_complementary_compression_bound (q x : E) (hq : q * q = q) (hqs : star q = q) : ‖q * x * q + (1 - q) * x * (1 - q) - x‖ ≤ 2 * ‖q * x - x * q‖ := by …