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I have shown you some field theoretic constructions of conformal field theories,
notably these non-abelian current algebras and stress energy tensors,
in the way the physicists would do it by constructing free fields on a Fox space
and then doing some standard constructions like WIC products and play with that.
In this lecture I want to do basically the same thing again,
but in a more mathematical language, in the language of operator algebras.
And we have notably C-star algebras.
C-star algebra is an algebra which, well roughly speaking,
I don't want to give the formal definition,
but it has an algebra that has all the properties like a star subalgebra on a Hilbert space
should have a closed, topologically closed, a norm closed star subalgebra on a Hilbert space should have.
So whenever you have the intention of representing an algebra on a Hilbert space,
then you should start from a C-star algebra to begin with.
But the C-star algebra itself may be something more abstract,
and it may have different representations on different Hilbert spaces, which may be inequivalent,
but it consists of bounded operators that have a conjugate, an adjoint,
and it has a norm, and the norm and the adjoint satisfy the same relations
as they would do for bounded operators on a Hilbert space.
And yeah, okay, so this is the language I will use now.
And in particular, it means that we will not look at fields anymore,
and field operators, which are necessarily unbounded operators, with a single exception.
But rather things, in order to make the contact with the fields,
you should think of the objects that I am constructing as exponentials of self-adjoint unbounded operators,
turning them into unitary operators.
And we have already seen the Weyl algebra,
which is defined as one starts with a linear real symplectic space of functions,
could just be the Schwarz functions on the real line or something like this.
And so one has a symplectic form, which is an excursion metric
and a real valued skew symmetric form on this space of functions.
And then you define these relations, plus saying that each of these W is unitary,
which by virtue of these equations implies that the adjoint of this is W of minus F.
And then one can show that these relations define a unique C star algebra.
The star operation is manifestly here.
And the non-trivial question is, is there a norm on this algebra?
And it turns out, yes, there is a unique norm.
And then one may close the algebra generated by these unitaries,
close this algebra under this norm, and the result is a C star algebra,
which carries the name of CCR.
This stands for canonical commutation relations.
And the only input was sigma.
Yeah, your symplectic vector space with a symplectic form.
So this is a C star algebra.
And the next thing is, how do I get representations of a C star algebra on a Hilbert space?
And here the basic tool is, this is unspecific, C, well, A, any C star algebra.
And then the basic tool is the GNS construction, a Gelfand-Neumann-Neumark-Sieger construction.
And it is the following.
If I have an omega, a state on A.
State means it's a linear functional.
It is real valued on the self-adjoint elements.
Presenters
Prof. Karl-Henning Rehren
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Dauer
01:24:42 Min
Aufnahmedatum
2013-10-11
Hochgeladen am
2013-10-28 09:00:13
Sprache
de-DE