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C star algebra
Definition
A possibly nonunital complex Banach algebra is a complex vector space equipped with an associative complex-bilinear multiplication (A bounded bilinear map between normed spaces for the bilinearity convention) and a norm under which is a Banach space (Banach space, Real and complex scalar conventions for normed spaces), such that the norm is submultiplicative:
No multiplicative identity is assumed, and no real-algebra or unital convention is imported from elsewhere.
A complex C*-algebra is a possibly nonunital complex Banach algebra equipped with an involution , , which is conjugate-linear (Real and imaginary parts, complex conjugation, and modulus) and satisfies
The last identity is the C*-identity. Two immediate consequences are worth recording, and both are proved from the displayed axioms alone:
- the involution is isometric: . Indeed gives when , and applying this inequality to and using gives ; the case is trivial;
- no norm-uniqueness assertion is part of this definition: such a theorem needs additional hypotheses and proof, and does not follow merely by naming the displayed C*-identity.
Let and be complex C*-algebras. A bounded star-homomorphism, or bounded -homomorphism, is a bounded complex-linear map (A bounded linear operator between normed spaces) satisfying
A star-homomorphism is not required to be unital, and it is not required that a unit be present or preserved; when and both happen to be unital, is called unital if . The bounded nonunital star-homomorphisms are the arrows of the locally compact duality theorem on this page (Locally compact Gelfand duality), with properness imposed there through Approximate unit and proper C star morphism.
Remarks
- The zero algebra. is a C*-algebra in this sense; it is not unital in the above convention, since its only element equals both candidate identities and the unital definition requires . The zero algebra is treated separately in the representation theorems, where it corresponds to the empty space.
- Isometry of the involution is a theorem, not an axiom. It is derived above from the C*-identity, and is used whenever an estimate for is needed without an inner product or a Hilbert-space adjoint.
- A bounded star-homomorphism is automatically contractive, and injective one is isometric; neither statement is used as a definition, and neither is proved here.
Depends on
Used by
- Algebraic unitization of a star algebra Definition
- Approximate unit and proper C star morphism Definition
- C star algebra generated by a normal operator Definition
- Self-adjoint positive unitary and normal elements Definition
- Bounded Hilbert operators form a C star algebra Lemma
- C star spectral radius equals norm for normal elements Lemma
- Characters on a unital commutative C star algebra preserve star Lemma
- Continuous functional calculus produces a regular PVM Lemma
- Spectral permanence for unital c star subalgebras Lemma
- Bounded normal operator abstract spectral theorem Theorem
- Commutative Gelfand duality Theorem
- Commutative Gelfand Naimark Theorem
- Continuous functional calculus for bounded normal operators Theorem
- Continuous functional calculus for bounded self adjoint operators Theorem
- Every commutative C star algebra has an approximate unit Theorem
- Locally compact Gelfand duality Theorem
- Minimal C star unitization Theorem
- Nonunital commutative Gelfand Naimark Theorem
- Positive square root Theorem
- Spectral mapping for continuous normal functional calculus Theorem
Dependency tree · two levels
12 results within two dependency steps of this one, each drawn at its shortest distance from it. An arrow runs from a result to what uses it, so the chart reads left to right and ends at this result, which carries a heavier outline. Every node is a link to that result. Click elsewhere on the chart to enlarge it.
Sources
- Vahid Shirbisheh, Lectures on C-star Algebras, v2 — Definitions 2.1.1, 2.1.18 and §3.1, printed pp. 11–13 and 54–61 (standard reference, not scraped)
- Dana P. Williams, Lecture Notes on the Spectral Theorem — Definitions 3.8 and 4.1, printed pp. 8–9 (standard reference, not scraped)