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Woo Young Lee Lecture Notes on Operator Theory

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CHAPTER 3.<br />

HYPONORMAL AND SUBNORMAL THEORY<br />

projecti<strong>on</strong> of K <strong>on</strong>to H, then S ∗n f = P N ∗n f, f ∈ H. If f 0 , · · · , f n ∈ H then<br />

∑<br />

⟨S j f k , S k f j ⟩ = ∑ ⟨N j f k , N k f j ⟩<br />

j,k<br />

j,k<br />

= ∑ ⟨N ∗k N j f k , f j ⟩<br />

j,k<br />

= ∑ ⟨N j N ∗k f k , f j ⟩<br />

j,k<br />

= ∑ ⟨N ∗k f k , N ∗j f j ⟩<br />

j,k<br />

∥ ∑ ∥∥∥∥<br />

2<br />

=<br />

N ∗k f<br />

∥<br />

k .<br />

So (3.3) holds.<br />

(b) ⇒ (c): Put g k = S k f k . Then (3.3) implies<br />

∑<br />

⟨S j g k , S k g j ⟩ = ∑ ⟨S j+k f k , S j+k f j ⟩.<br />

j,k<br />

j,k<br />

k<br />

So (3.4) holds.<br />

(c) ⇒ (a): See [C<strong>on</strong>2].<br />

(b) ⇒ (d): If B 0 , · · · , B n ∈ C ∗ (S), let f k = B k f. Then<br />

(3.3) ⇐⇒<br />

⟨ ∑<br />

j,k<br />

B ∗ j S ∗k S j B k f, f<br />

⟩<br />

≥ 0.<br />

(d) ⇒ (b): By Zorn’s lemma,<br />

any operator = ⊕ star-cyclic operator.<br />

So we may assume that S has a star-cyclic vector e 0 , i.e., assume H = cl [C ∗ (S)e 0 ].<br />

If B 0 , · · · , B n ∈ C ∗ (S) then (3.3) holds for f k = B k e 0 . Since (3.3) holds for a dense<br />

set of vector, (3.3) holds for all vectors.<br />

(a) ⇒ (e): Let N = ∫ zdE(z) be the spectral decompositi<strong>on</strong> of N, a normal<br />

extensi<strong>on</strong> of S acting <strong>on</strong> K ⊇ H. Let P be the orthog<strong>on</strong>al projecti<strong>on</strong> of K <strong>on</strong>to H.<br />

Define<br />

Q(△) := P E(△)| H for every Borel subset △ of C.<br />

89

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